Mars Pathfinder
Imager for Mars Pathfinder
Experiment Data Record
Compact Disc - Read Only Memory
Software Interface Specification
PF-400-8.02
July, 1998
Version 1.8
Elizabeth Duxbury
JPL
Jet Propulsion Laboratory
4800 Oak Grove Drive
Pasadena, California 91109-8099
A PDS KEYWORDS AND THEIR DEFINITIONS
ADC | Analog to Digital Converter |
AIM | Attitude Information Management |
APXS | Alpha Proton X-Ray Spectrometer |
ASCII | American Standard Code for Information Interchange |
ASI/MET | Atmospheric Structure Instrument/Meteorology Package |
BTC | Block Truncation Coding |
CAHV | Camera model described by four vectors C, A, H and V |
CAHVOR | Camera model CAHV which accounts for CCD and non-linear distortions |
CBE | Current Best Estimate |
CCD | Charge-Coupled Device |
CD-ROM | Compact Disc - Read Only Memory |
CD-WO | Compact Disc - Write Once |
c.g. | center of gravity |
CODMAC | Committee On Data Management And Computation |
COSPAR | Committee On Space Research |
dB | Decibel |
DCT | Discrete Cosine Transform |
DN | Data Number or Digital Number |
DOS | Disc Operating System |
DPW | Data Preparation Workbook |
DSN | Deep Space Network |
E&H | Engineering and Health |
EDL | Entry, Descent, and Landing |
EDR | Experiment Data Record |
EEPROM | Electronically Eraseable Programmable Read Only Memory |
EH&A | Engineering, Housekeeping, and Accountability |
EOF | End of File |
EST | Eastern Standard Time |
ETR | Eastern Test Range |
FOV | Field of View |
GEM | Graphite Epoxy Motor |
GMT | Greenwich Mean Time |
HFS | Hierarchical File System |
HGA | High Gain Antenna |
HTML | HyperText Markup Language |
IAG | International Association of Geodesy |
IAU | International Astronomical Union |
IBM | International Business Machines® |
ICT | Integer Cosine Transform |
IDL | Interactive Data Language |
IMP | Imager for Mars Pathfinder |
ISA | Integrated Support Assembly |
ISO | International Standards Organization |
IVP | Image Vector Pointing |
JPEG | Joint Photographic Experts Group |
JPL | Jet Propulsion Laboratory |
LCT | Linear Cosine Transform |
LGA | Low Gain Antenna |
LPL | Lunar and Planetary Laboratory |
LREU | Lander Remote Engineering Unit |
LST | Local Solar Time |
Mbytes | Megabytes |
MESUR | Mars Environmental Survey |
MFEX | Microrover Flight Experiment |
MFX | Martian Surface Fixed coordinate frame (check) |
MGA | Medium Gain Antenna |
MIPL | Multimission Image Processing Laboratory |
MIPS | Multimission Image Processing Subsystem |
MIPS | Millions of Instructions Per Second |
MLL | Mars Local Level coordinate frame (check) |
MPF | Mars Pathfinder |
MPFL | Mars Pathfinder Lander |
MPFR | Mars Pathfinder Rover |
MSB | Most Significant Bit (or Byte) |
MSW | Microsoft® Word |
NAIF | Navigation and Ancillary Information Facility |
NASA | National Aeronautics and Space Administration |
NCS | Nutation Control System |
NIST | National Institute of Standards and Technology |
NSSDC | National Space Science Data Center |
PAM-D | Payload Assist Module-D |
PC | Personal Computer |
Adobe® Portable Document Format | |
PDS | Planetary Data System |
PDT | Pacific Daylight Time |
PF | Pathfinder |
PIO | Public Information Office |
PROM | Programmable Read Only Memory |
PRT | Platinum Resistance Thermometer |
PSDD | Planetary Science Data Dictionary |
PST | Pacific Standard Time |
RAD | Rocket Assisted Descent |
RAM | Random Access Memory |
RF | Radio Frequency |
RFS | Radio Frequency Subsystem |
RICE | A lossless compression algorithm developed by Bob Rice of JPL |
RPM | Revolutions Per Minute |
RSI | Research Systems Incorporated® |
RVR | Rover |
SAT | Science Advisory Team |
SFDU | Standard Formatted Data Unit |
SIS | Software Interface Specification |
SOG | Science Operations Group |
SPICE | Spacecraft Planet Instrument C-matrix Events |
sps | samples per second |
TBD | To Be Determined |
TC | thermocouple |
TCM | Trajectory Correction Maneuver |
TDS | Telemetry Delivery Subsystem |
TMU | Telemetry Modulation Unit |
UAMS | Upper Atmosphere Mass Spectrometer |
UHF | Ultra High Frequency |
UOFA | University of Arizona |
USGS | United States Geological Survey |
UTC | Universal Time Coordinated |
VICAR | Video Image Communication and Retrieval system |
VL | Viking Lander |
VME | VersaModule European, a reliable, multiple-processor, bus architecture |
VMS | Virtual Memory System |
XAR | Extended Attribute Record |
Item | Assignee | Closure Date |
---|
1.0 INTRODUCTION
1.1 Content Overview
This Software Interface Specification (SIS) describes the form and content of the Imager for Mars Pathfinder (IMP) Experiment Data Record (EDR) Compact Disc - Read Only Memory (CD-ROM).
The IMP EDR CD-ROMs shall be generated by the Multi-mission Image Processing Subsystem (MIPS) at the Jet Propulsion Laboratory in order to distribute the data acquired by the IMP to the project scientists and later to the Planetary Data System (PDS).
An attached PDS label shall be included with each data file. Documentation files shall be provided which inform the user about the organization and content of each disc, the definition of the labels, and the index files containing information about all the data files stored in the data set.
All PDS label formats and documentation are based on the Planetary Data System Data Preparation Workbook (reference 1).
All data formats are based on the Planetary Science Data Dictionary Document (PSDD) (reference 3).
The specifications in this document apply to all IMP EDR CD-ROMs that are produced during the Mars Pathfinder mission.
Applicable documents used in producing this specification include:
2.0 INTERFACE CHARACTERISTICS
2.1 Operations Perspective
2.1.1 Data Source, Destinations, and Transfer Method
IMP EDR CD-ROMs shall be produced by MIPS for distribution to the Mars Pathfinder Project. MIPS shall use freely available CD-ROM publishing software, which shall reside at MIPS, to produce premastered CD-WOs for delivery and release to the mastering vendor for production of CD-ROMs. The mastering vendor will ship the discs to MIPS for distribution and archiving. Copies of the CDs will be archived with the Imaging Node of the PDS and with the National Space Science Data Center.
2.1.2 Generation Method and Frequency
The IMP EDR CD-ROM data shall be generated using MIPS software. The EDR data processing includes decoding and decompressing the IMP image data in single frame form. These data products conform to NASA level 0 or CODMAC level 2 data products. (A more complete description of the EDRs is available in the IMP EDR SIS, reference 5, a copy of which will be included on the CDs.) MIPS will then pre-master the data to CD-WO.
The CD-ROMs shall be produced as rapidly as possible on a best efforts basis. It is intended that the first CD volume should be published within six months of receipt of the data.
Each CD-ROM shall contain at most 650 Mbytes of data. Within this limitation, as many data files as can fit on a CD-ROM will be included. This is expected to result in the publication of a three volume set.
2.3 Interface Medium Characteristics
IMP EDR CD-ROM physical characteristics shall conform to ISO-9660 level 1 industry standards (reference 4).
2.4 Backup and Duplicate Copies
The CD-ROM contents shall be stored on magnetic disc until a validated master has been produced. CD-WO copies of the disc shall be retained at MIPS.
3.0 CD-ROM CONTENT AND FORMAT
This section describes in detail the format and content of the IMP EDR CD-ROM.
IMP EDR CD-ROM data shall be formatted in accordance with Planetary Data System specifications (references 1-3). The format is described below.
The IMP EDR CD-ROM format shall be compatible with various computer systems including IBM PC, Apple Macintosh, Sun, and Digital VAX. However, the data files will not contain extended attribute records, so users of older VMS systems may have dificulty reading them. The EDR CD-ROM format shall be in accordance with the ISO-9660 level 1 Interchange Standard (reference 4).
The following paragraphs describe file formats for the various kinds of files contained on the CD-ROMs.
Text files (.TXT suffix) may exist in any directory, including the root directory. They are ASCII files with attached PDS labels, and provide information about the data on the CD (as in the AAREADME.TXT file) or about data in a specific directory. All text files are streams of bytes with both a carriage return character (ASCII 13) and a line feed character (ASCII 10) as the line terminator. This allows the files to be read by the HFS, DOS, UNIX, and VMS operating systems.
The following is a sample PDS label for an AAREADME.TXT file.
PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 1997-07-04 INTERCHANGE_FORMAT = ASCII NOTE = "This file describes the format and content of this CD-ROM." END_OBJECT = TEXT END
Document files exist in the document directory, and include textual material describing the mission, spacecraft, instruments, data sets, and calibration. The MPF Image Browser also consists of HTML formatted document files, located in the browse directory. Possible formats for these documents include Adobe Portable Document Format (".PDF"), HyperText Markup Language (".HTM"), and plain ASCII (".ASC"). At least one copy of each document file must be in either plain ASCII or HTML. Illustrations and images for these documents are stored in separate GIF or JPEG formatted files, which are also considered to be document files.
All ASCII and HTML files are streams of bytes with both a carriage return character (ASCII 13) and a line feed character (ASCII 10) as the line terminator. The ASCII files can be read on any operating system. The HTML files can be read with most World Wide Web browsers that are capable of displaying tables. The PDF documents are a binary format that can be read with the Adobe Acrobat Reader, available from "http://www.adobe.com". GIF and JPEG images can be displayed using many commonly available image display programs.
All document files are described by detached PDS labels. The PDS label file has the same name as the document file(s) it describes, with the extension ".LBL", unless the single label describes multiple files that make up the same document, (ex., "CALIB001.GIF", "CALIB002.GIF", "CALIB003.GIF"). In this case, the label file has a similar name to the document, ex. "CALIB.LBL". The following is a sample detached PDS label file, entitled "VOLSIS.LBL", describing this document, found in the "VOLSIS.HTM" and "VOLSIS.PDF" files.
PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM ^HTML_DOCUMENT = "VOLSIS.HTM" ^PDF_DOCUMENT = "VOLSIS.PDF" OBJECT = HTML_DOCUMENT DOCUMENT_NAME = "Mars Pathfinder IMP EDR CD-ROM SIS" DOCUMENT_TOPIC_TYPE = VOLUME_SIS INTERCHANGE_FORMAT = ASCII DOCUMENT_FORMAT = HTML PUBLICATION_DATE = 1998-07-01 END_OBJECT = HTML_DOCUMENT OBJECT = PDF_DOCUMENT DOCUMENT_NAME = "Mars Pathfinder IMP EDR CD-ROM SIS" DOCUMENT_TOPIC_TYPE = VOLUME_SIS INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = PDF PUBLICATION_DATE = 1998-07-01 END_OBJECT = PDF_DOCUMENT END
Catalog files (".CAT" suffix) exist in the catalog directory, with the exception of the VOLDESC.CAT file which is located in the root directory. These are ASCII files formatted as PDS catalog objects (see reference 2). All catalog files are streams of bytes with both a carriage return character and a line feed character as the line terminator. This allows the files to be read by the HFS, DOS, UNIX, and VMS operating systems.
Copies of some catalog files are also included in HTML format. These files are indicated with the suffix ".HTM" and are kept in the document, rather than the catalog, directory.
Tabular files (.TAB suffix) are ASCII files formatted for direct reading into many database management systems on various computers. All fields are separated by commas, and character fields are enclosed in double quotation marks ("). (Character fields are padded with spaces to keep quotation marks in the same columns.) Character fields are left justified, and numeric fields are right justified. The "START_BYTE" and "BYTES" values listed in the labels do not include the commas between fields or the quotation marks surrounding character fields. The records are of fixed length, and the last two bytes of each record contain the ASCII carriage return and line feed characters. This allows a table to be treated as a fixed length record file on computers that support this file type and as a normal text file on other computers.
All tabular files are described by detached PDS labels. The PDS label file has the same name as the data file it describes, with the extension .LBL; for example, the file INDEX.TAB is accompanied by the detached label file INDEX.LBL in the same directory.
PDS label files (.LBL suffix) are located in many directories. They are descriptive labels (see reference 4) and may be either attached to or detached from their associated files.
The PDS label file is an object-oriented file; the object to which the label refers (e.g. IMAGE, TABLE, etc.) is denoted by a statement of the form:
^object = locationin which the carat character (^, also called a pointer in this context) indicates that the object starts at the given location. The location denotes the name of the file containing the object, if the label is detached, or the starting record or byte number, if the label is attached. For example:
^INDEX_TABLE = "INDEX.TAB"indicates that the INDEX_TABLE object described by the INDEX.LBL file is in the file named "INDEX.TAB".
^IMAGE = 3indicates that the IMAGE object begins at record 3 of the same file that the label is attached to. Below is a list of the possible formats for the ^object definition.
^object = nwhere
^object = n <BYTES>
^object = ("filename.ext")
^object = ("filename.ext",n)
^object = ("filename.ext",n <BYTES>)
n is the starting record or byte number of the object, counting from the beginning of the file (unless specified as bytes, this is assumed to be records), <BYTES> indicates that the number given is in units of bytes, filename is the upper-case file name, ext is the upper-case file extension, dirlist is a UNIX style, forward slash-delimited path-list of parent directories, in upper case, that specifies the object file directory (used only when the object is not in the same directory as the label file). The list begins at directory level below the root directory of the CD-ROM. 'dirlist/' may be omitted when the object being described is located either in the same directory as the detached label, or in a subdirectory named 'label' that is located in a higher level of the directory tree, typically the CD-ROM root itself.
All labels contain 80-byte fixed-length records, with a carriage return character (ASCII 13) in the 79th byte and a line feed character (ASCII 10) in the 80th byte. This allows the files to be read by the HFS, DOS, Unix, and VMS operating systems.
The detailed specifications for the formats of the image files are described in a Software Interface Specification published by MIPS (reference 5) and in the DATASET.CAT file, both of which are included on the CDs. The image files are all uncompressed 16-bit PDS formatted files with attached PDS labels.
The following paragraphs describe the content of the CD-ROMs.
The IMP EDR CD-ROM volume set is numbered MPIM_0001 through MPIM_0003. Each CD in the set will contain the same directory structure, with the exception of the data subdirectories, which will vary from one CD to another, as they are named on the basis of time.
The IMP EDR CD-ROM directory structure consists of one ROOT directory, a BROWSE subdirectory, a CATALOG subdirectory, a DOCUMENT subdirectory, a GAZETTER subdirectory, an INDEX subdirectory, and multiple data subdirectories. The data subdirectories are divided first on the basis of target, then on the basis of command sequence number, and finally on the basis of planet day number or "sol".
The root directory contains files describing the content and format of the CD-ROMs. The catalog subdirectory contains the completed catalog templates for the instrument and data set included on the volume. Any other templates (mission, instrument host, reference, and personnel) that are available at the time the CDs are created will also be included. The gazetteer directory includes a gazetteer of the informal names of the rocks and other features at the MPF landing site, in tabular format. Files in the index directory include tables of label items describing the observation of each EDR frame, and PDS labels which in turn describe the index tables. Each index table entry is generated after the corresponding EDR file is processed in the CD generation procedure. The INDEX tables on each CD-ROM shall only reflect those files contained on that CD-ROM. Separate, cumulative index files which contain a complete listing of all EDRs on the set, will also be included on the volumes.
Files in each of the data subdirectories consist of an EDR data file with an associated attached PDS label, organized in sub-directories first by target, sequence number, and sol. The following tables describe the content and source of files in the CD-ROM directories. (Source indicates the group providing the current version of a file.)
The following table lists the files in the root directory. The ERRATA.TXT file may not be present on all CDs, as it will document errors discovered on previous CDs in the set.
File | Contents | Source |
---|---|---|
AAREADME.HTM, LBL, TXT | Textual information describing CD-ROM content and format. | MIPS |
ERRATA.HTM, LBL, TXT | Textual information describing errors and/or anomalies found on the current or previous CDs. | MIPS |
VOLDESC.CAT | A description of the contents of this CD-ROM volume in a human and machine readable format. | MIPS |
The files in this directory contain textual information about many aspects of the mission and data, and are written in a format that may be loaded into the PDS Central Node's Data Set Catalog. The following table lists the files in the catalog subdirectory.
File | Contents | Source |
---|---|---|
CATINFO.TXT | A textual description of the contents of the CATALOG subdirectory. | MIPS |
DATASET.CAT | A description of the IMP EDR data set, including such things as processing history, data format, and ancillary data necessary to use the data. | MIPS |
INST.CAT | A detailed textual description of the Imager for Mars Pathfinder. | IMP team |
INSTHOST.CAT | A textual description providing an overview of the Mars Pathfinder Lander. | IMP team |
MISSION.CAT | A detailed description of the Mars Pathfinder mission. | IMP team |
PERSON.CAT | Contact information for people responsible for producing the Mars Pathfinder data sets. | IMP team |
REF.CAT | A list of references of papers providing further information about the data set. | IMP team |
This directory contains textual files describing the data sets and instruments, plus any other supplementary information available at the time the CDs are ready to be published.
File | Contents | Source |
---|---|---|
DOCINFO.TXT | Textual description of the files included in the document directory. | MIPS |
CONTACTS.ASC, LBL | Contact information for Mars Pathfinder personnel. | Project |
DATASET.HTM, LBL | A description of the IMP data set, including such things as processing history, data format, and ancillary data necessary to use the data. | IMP team |
EDRSIS.HTM, LBL, PDF | Imager for Mars Pathfinder Experiment Data Record | MIPS |
IMPUG.HTM, PDF, LBL | Imager for Mars Pathfinder User's Guide | IMP team |
INST.HTM, LBL | A detailed textual description of the Imager for Mars Pathfinder. | IMP team |
INSTHOST.HTM, LBL | A textual description providing an overview of the Mars Pathfinder Lander | IMP team |
MISSION.HTM, LBL | A detailed description of the Mars Pathfinder mission. | Project |
REF.HTM, LBL | A list of references of papers providing further information about the data set. | IMP team |
VOLSIS.HTM, LBL, PDF | MPF Imager for Mars Pathfinder Experiment Data Record CD-ROM SIS | MIPS |
3.2.2.4 Gazetteer Subdirectory
The files in this directory contain textual and tabular information about the named features at the Mars Pathfinder landing site. Please note that this information is provided as a convenience to researchers, and that the names assigned to features here have not been approved by the International Astronomical Union. Also note, that only those files which are available at the time the data is ready for CD mastering will be included. Thus, no guarantee is made that all the described files will be included.
File | Contents | Source |
---|---|---|
GAZINFO.TXT | A textual description of the contents of the GAZETTER subdirectory. | MIPS |
GAZETTER.TXT | A textual description of the structure and contents of the gazetteer table. | Bob Kanefsky |
GAZETTER.LBL | The PDS label describing the structure of the gazetteer table. | Bob Kanefsky |
GAZETTER.TAB | A table of the MPF landing site named features, along with some descriptive information. | Bob Kanefsky |
The following table lists the files in the index subdirectory.
File | Contents | Source |
---|---|---|
INDXINFO.TXT | Textual description of the contents of the INDEX directory. | MIPS |
INDEX.LBL | A PDS formatted label describing the format of the INDEX.TAB file. | MIPS |
INDEX.TAB | A tabular index of selected label items describing the IMP image files on the CD. This table alone is sufficient for doing simple searches for data on the CDs. | MIPS |
CUMINDEX.LBL | A PDS formatted label describing the format of the CUMINDEX.TAB file. | MIPS |
CUMINDEX.TAB | A cumulative tabular index containing the contents of the INDEX.TAB files from all of the IMP EDR CD-ROMs. | MIPS |
COMMAND.LBL | A PDS formatted label describing the format of the COMMAND.TAB file. | MIPS |
COMMAND.TAB | A table containing information about the commands sent to the IMP camera. Along with the EDRINDEX table, forms a relational database describing most of the available parameters for the images on the CDs. | MIPS |
EDRINDEX.LBL | A PDS formatted label describing the format of the EDRINDEX.TAB file. | MIPS |
EDRINDEX.TAB | A detailed tabular index of parameters describing the IMP image files. Along with the COMMAND table, forms a relational database describing most of the available parameters for the images on the CDs. | MIPS |
The data directories that contain the image EDRs are first subdivided on the basis of target, then on the basis of command sequence number, and finally by spacecraft clock start count. Thus the pathname for any image will be constructed as follows:
The division of images by target is done primarily on the basis of the observational intent of an image, as indicated by the OBSERVATION_NAME and IMAGE_OBSERVATION_TYPE. The targets include both planetary bodies such as Mars, Phobos, the Sun, and generic "Star", as well as specific objects like calibration targets, and the Rover and Lander. One of the reasons this was done is so that IMP images that were taken primarily for the support of other instrument experiments will all be collected in a single location. However, users of the data should be aware that useful "Mars" images will be scattered throughout the directory heirarchy. For example, an image taken specifically to study the windsocks, and therefore included in the WINDSOCK directory, may also be useful for studying the geological features visible in the background. The targets do not include specific features on Mars like "Barnacle Bill" or "Yogi". Most of the images containing these features will be classified under the general target "MARS". To find images containing specific features, please consult the gazetteer. (See section 3.2.2.4.)
The list of the target directory names and their meanings is shown in the table below. Also included is a list of the command sequences that will be included in each target directory.
Directory Name | Description | Command Sequences |
---|---|---|
APXSSITE | This directory contains images taken of sites where the APXS instrument was deployed. Their purpose is to support that instrument. | 71, 72 |
CALIMG | The images in this directory were taken for calibration purposes. This includes images of the radiometric and fiducial targets on the lander, flat field and dark current images, and readouts of the dark strip and null strip on the CCD. | 0 - 2, 7, 8, 15, 17, 25, 30 - 33, 46, 49, 51, 52, 54, 55, 62, 64 - 67, 69, 70, 72 - 74, 161, 164, 171, 172, 190, 191, 194 - 196, 250, 267, 283, 466 |
DEIMOS | These images were targeted at Deimos. | 154 |
LANDER | These are images targeted at parts of the lander to assess its status. This includes things like the airbag assessment pan and ramp deployment images. | 9, 10, 22, 23, 53, 180 |
MAG | These images were aimed at the various magnetic targets on the lander to study the magnetic properties of airborne particles. | 7, 62, 64, 65, 252, 257, 266, 267 |
MARS | This category consists of the vast majority of the images, those which were taken primarily to view the Martian landscape. It includes most of the major panoramas, the super resolution images, and the change monitoring images. | 1, 2, 8, 24, 30 - 33, 44, 69, 70, 73, 74, 161, 162, 164 - 167, 171, 172, 178, 179, 181 - 188, 190, 194, 195, 199, 265, 275 - 277, 279, 288, 290, 294 - 298 |
PHOBOS | These images were targeted at Phobos. | 155, 158, 258, 259 |
ROVER | These sequences of images were taken to support Rover operations and investigations. This includes things like end of day sequences, movie sequences, navigation images, and soil experiment images. | 13, 50, 53 - 56, 350, 353, 354 |
SKY | This directory includes a variety of images including those taken looking at both high elevations and at the horizon, and at a variety of times of day. (Some images may include the Sun.) Many were taken for the purpose of studying the atmosphere and the particles suspended in it. | 35, 36, 39, 46, 151, 152, 156, 280, 283, (1520) |
STAR
(ARCTURUS, |
These images were targeted at the stars Altair, Arcturus, and Vega. These are the one exception to the rule that target = directory name, since they are all grouped together in the "STAR" directory. | 154, 158, 258 |
SUN | These images were targeted at the Sun, usually for the purpose of studying the atmosphere. In cases where a sequence of images, usually around sunset or sunrise, included some images with the sun and some without, the sequence has been included in the SKY directory. | 59, 60, 260 - 263 |
WINDSOCK | The images in this directory were targeted at the windsocks on the ASI/MET mast. | 68, 173 - 175 |
The next level of subdirectories are divided by command sequence number. The command sequence number usually represents a set of commands designed to carry out a particular task. These command sequences were often repeated regularly, and resulted in the production of varying numbers of images. A list of the command sequence numbers and their corresponding observation names is provided in the following table. The "Target" column shows which top-level directory each sequence is stored in on the CDs.
In cases where two targets are listed, the images have been placed in a target directory based on the IMAGE_OBSERVATION_TYPE, pointing angle, or visual inspection. (The target for observations which include either Phobos or Deimos and a star were determined by Nicolas Thomas of the Max Planch Institut fur Aeronomie in Germany.)
Seq Num | Observation Name | Target |
---|---|---|
0 | IMP_HEALTH_CHECK_#1_(CRUISE) | CALIMG |
1 | PRE_DEPLOY_RED_PANORAMA | MARS or CALIMG |
2 | MISSION_SUCCESS_FIRST_LOOK_PART_ONE | MARS or CALIMG |
7 | MAG_TARGETS_IMP_DEPLOYED_12_FILTERS | MAG |
7 | MAG_TARGETS_IMP_DEPLOYED_12_FILTERS+RAD_CAL | MAG or CALIMG |
7 | MAG_TARG_DEPLOYED_15_FILTERS+RAD_CAL_15_FILTERS | MAG or CALIMG |
8 | IMP_HEALTH_CHECK_#2_(CRUISE) | CALIMG |
8 | MISSION_SUCCESS_FIRST_LOOK_PART_TWO | MARS |
9 | FORWARD_RAMP_DEPLOYMENT_IMAGES | LANDER |
10 | REAR_RAMP_DEPLOYMENT_IMAGES | LANDER |
13 | ROVER_MOVIE_REAR_RAMP | ROVER |
15 | UPPER_RAD_CAL_DEPLOYED_15_COLOR | CALIMG |
15 | UPPER_RAD_CAL_IMAGES_DEPLOYED_12_COLOR | CALIMG |
17 | COMPRESSED_RAD_CAL2_STOWED_1_COLOR | CALIMG |
22 | PREDEPLOY_AIRBAG_ASSESS_PAN | LANDER |
23 | DEPLOYED_AIRBAG_ASSESS_PAN | LANDER |
24 | SUN_EARTH_HORIZON_PANORAMA1 | MARS |
25 | RAD_CAL2_IMP_STOWED_7_COLOR | CALIMG |
30 | INSURANCE_PAN_FILTER_0_QUADRANT_1 | MARS or CALIMG |
30 | INSURANCE_PAN_FILTER_6_QUADRANT_1 | MARS |
30 | INSURANCE_PAN_FILTER_8_QUADRANT_1 | MARS |
30 | INSURANCE_PAN_FILTER_9_QUADRANT_1 | MARS |
31 | INSURANCE_PAN_FILTER_0_QUADRANT_2 | MARS or CALIMG |
31 | INSURANCE_PAN_FILTER_6_QUADRANT_2 | MARS |
31 | INSURANCE_PAN_FILTER_8_QUADRANT_2 | MARS |
31 | INSURANCE_PAN_FILTER_9_QUADRANT_2 | MARS or CALIMG |
32 | INSURANCE_PAN_FILTER_0_QUADRANT_3 | MARS or CALIMG |
32 | INSURANCE_PAN_FILTER_6_QUADRANT_3 | MARS |
32 | INSURANCE_PAN_FILTER_8_QUADRANT_3 | MARS |
32 | INSURANCE_PAN_FILTER_9_QUADRANT_3 | MARS or CALIMG |
33 | INSURANCE_PAN_FILTER_0_QUADRANT_4 | MARS or CALIMG |
33 | INSURANCE_PAN_FILTER_6_QUADRANT_4 | MARS |
33 | INSURANCE_PAN_FILTER_8_QUADRANT_4 | MARS |
33 | INSURANCE_PAN_FILTER_9_QUADRANT_4 | MARS |
35 | NIGHTTIME_OPACITY | SKY |
36 | EVENING_AUREOLE_AEROSOL_MEASUREMENTS | SKY |
39 | MORNING_AUREOLE_AEROSOL_MEASUREMENTS | SKY |
44 | PREDEPLOY_13_COLOR_NEAR_FIELD_LOSSLESS_IMAGE | MARS |
46 | CLOUD_DETECTION | SKY or CALIMG |
49 | UPPER_RAD_CAL_IMAGES_DEPLOYED_12_COLOR | CALIMG |
50 | ROVER_MOVIE | ROVER |
51 | DARK_CURRENT_CALIBRATION | CALIMG |
52 | DARK_CURRENT_SUBFRAMES | CALIMG |
53 | ROVER_MOVIE | ROVER |
53 | ROVER_NAVIGATION_IMAGES | ROVER |
53 | LANDER_SOLAR_ARRAY_IMAGES | LANDER |
54 | ROVER_NAVIGATION_IMAGES | ROVER or CALIMG |
54 | CONCURRENT_REAR_WHEEL_DIG_IMG | ROVER |
55 | ROVER_NAVIGATION/ROVER_END_OF_DAY_IMAGES | ROVER or CALIMG |
56 | ROVER_TRACK_IMAGES | ROVER |
56 | ROVER_NAVIGATION_IMAGES | ROVER |
59 | COMPRESSED_AEROSOL_OPACITY_SUN | SUN |
60 | AEROSOL_OPACITY_SUN | SUN |
62 | MAG_UPPER_LOWER_STOWED_1 | MAG or CALIMG |
64 | MAG_UPPER_LOWER_STOWED_2 | MAG or CALIMG |
65 | LOWER_MAG_STOWED_2 | MAG or CALIMG |
66 | RAD_CAL2_IMP_STOWED_12_COLOR | CALIMG |
67 | RAD_CAL2_IMP_STOWED_5_COLOR | CALIMG |
68 | WINDSOCK_IMAGES | WINDSOCK |
69 | FILTER_0_IN_2_TIERS_FIRST_QUAD_MONSTER_PAN | MARS or CALIMG |
69 | FILTER_5_IN_4_TIERS_FIRST_QUAD_MONSTER_PAN | MARS |
69 | FILTER_6_IN_2_TIERS_FIRST_QUAD_MONSTER_PAN | MARS |
69 | FILTER_9_IN_2_TIERS_FIRST_QUAD_MONSTER_PAN | MARS |
69 | FILTER_11_IN_2_TIERS_FIRST_QUAD_MONSTER_PAN | MARS |
70 | FILTER_0_IN_2_TIERS_SECOND_QUAD_MONSTER_PAN | MARS or CALIMG |
70 | FILTER_5_IN_4_TIERS_SECOND_QUAD_MONSTER_PAN | MARS |
70 | FILTER_6_IN_2_TIERS_SECOND_QUAD_MONSTER_PAN | MARS |
70 | FILTER_9_IN_2_TIERS_SECOND_QUAD_MONSTER_PAN | MARS |
70 | FILTER_11_IN_2_TIERS_SECOND_QUAD_MONSTER_PAN | MARS |
71 | APXS_SITE_IMG | APXSSITE |
72 | APXS_SITE_IMG | APXSSITE or CALIMG |
73 | FILTER_0_IN_2_TIERS_THIRD_QUAD_MONSTER_PAN | MARS or CALIMG |
73 | FILTER_5_IN_4_TIERS_THIRD_QUAD_MONSTER_PAN | MARS |
73 | FILTER_6_IN_2_TIERS_THIRD_QUAD_MONSTER_PAN | MARS |
73 | FILTER_9_IN_2_TIERS_THIRD_QUAD_MONSTER_PAN | MARS |
73 | FILTER_11_IN_2_TIERS_THIRD_QUAD_MONSTER_PAN | MARS |
74 | FILTER_0_IN_2_TIERS_FOURTH_QUAD_MONSTER_PAN | MARS or CALIMG |
74 | FILTER_5_IN_4_TIERS_FOURTH_QUAD_MONSTER_PAN | MARS |
74 | FILTER_6_IN_2_TIERS_FOURTH_QUAD_MONSTER_PAN | MARS |
74 | FILTER_9_IN_2_TIERS_FOURTH_QUAD_MONSTER_PAN | MARS |
74 | FILTER_11_IN_2_TIERS_FOURTH_QUAD_MONSTER_PAN | MARS |
151 | SUNSET_EVENING_AEROSOL_MEASUREMENTS | SKY |
151 | MORNING_TWILIGHT_AEROSOL_MEASUREMENTS | SKY |
152 | SUNSET_EVENING_AEROSOL_MEASUREMENTS | SKY |
154 | DEIMOS_13_FILTERS+2_STARS | DEIMOS or STAR |
154 | STARS_2_+_DEIMOS_13_FILTERS | DEIMOS or STAR |
154 | ALTAIR_VEGA_+_DEIMOS_13_FILTERS | DEIMOS or STAR |
155 | FAST_PHOBOS_IMAGING | PHOBOS |
156 | NIGHTTIME_OPACITY_2 | SKY |
158 | STARS_2_+_PHOBOS_13_FILTERS | PHOBOS or STAR |
158 | ALTAIR_VEGA_+_PHOBOS_13_FILTERS | PHOBOS or STAR |
158 | ARCTURUS_VEGA_+_PHOBOS_13_FILTERS | PHOBOS or STAR |
161 | MULTISPECTRAL_SLICE | MARS or CALIMG |
162 | MISTY_MOUNTAIN | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN_TIER_1_RED | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_RED | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_RED | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_RED | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_RED | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_BLUE | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_BLUE | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_BLUE | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_BLUE | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_BLUE | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_GREEN | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_GREEN | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_GREEN | MARS |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_GREEN | MARS or CALIMG |
164 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_GREEN | MARS or CALIMG |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_RED | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_RED | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_RED | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_RED | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_RED | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_BLUE | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_BLUE | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_BLUE | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_BLUE | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_BLUE | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_GREEN | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_GREEN | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_GREEN | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_GREEN | MARS |
165 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_GREEN | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_RED | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_RED | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_RED | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_RED | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_RED | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_BLUE | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_BLUE | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_BLUE | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_BLUE | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_BLUE | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_1_GREEN | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_2_GREEN | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_3_GREEN | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_4_GREEN | MARS |
166 | GALLERY_PAN/PRESIDENTIAL_PAN _TIER_5_GREEN | MARS |
167 | GALLERY_PAN/PRESIDENTIAL_PAN _MISSING_IMAGES | MARS |
171 | MULTISPECTRAL_SPOTS_13_COLOR+LOWER_RAD_CAL | MARS or CALIMG |
172 | MULTISPECTRAL_SPOTS_13_COLOR+RAD_CAL | MARS or CALIMG |
173 | WINDSOCK_IMAGES | WINDSOCK |
174 | NO_PROFILE_WINDSOCK_IMAGES | WINDSOCK |
175 | WINDSOCK_IMAGES | WINDSOCK |
178 | DUST_DEVIL_SEARCH | MARS |
179 | CHANGE_MONITORING | MARS |
179 | CHANGE_MONITORING_I | MARS |
180 | AIRBAG_RECHECK/ROVER_PETAL_PANORAMA | LANDER |
181 | SUPERPAN_OCTANT_1_TIER_A | MARS |
182 | SUPERPAN_OCTANT_1_TIER_C | MARS |
182 | SUPERPAN_OCTANT_2_TIER_A | MARS |
182 | SUPERPAN_OCTANT_2_TIER_B | MARS |
182 | SUPERPAN_OCTANT_2_TIER_C | MARS |
182 | SUPERPAN_OCTANT_2_TIER_D | MARS |
182 | SUPERPAN_OCTANT_2_TIER_E | MARS |
183 | SUPERPAN_OCTANT_3 | MARS |
183 | SUPERPAN_OCTANT_3_TIER_A | MARS |
184 | SUPERPAN_OCTANT_4_TIER_A | MARS |
184 | SUPERPAN_OCTANT_4_TIER_B | MARS |
184 | SUPERPAN_OCTANT_4_TIER_C | MARS |
184 | SUPERPAN_OCTANT_4_TIER_D | MARS |
184 | SUPERPAN_OCTANT_4_TIER_E | MARS |
185 | SUPERPAN_OCTANT_5_TIER_A | MARS |
185 | SUPERPAN_OCTANT_5_TIER_B | MARS |
185 | SUPERPAN_OCTANT_5_TIER_C | MARS |
185 | SUPERPAN_OCTANT_5_TIER_D | MARS |
185 | SUPERPAN_OCTANT_5_TIER_E | MARS |
186 | SUPERPAN_OCTANT_6 | MARS |
187 | SUPERPAN_OCTANT_7_TIER_A | MARS |
188 | SUPERPAN_OCTANT_8_TIER_A | MARS |
188 | SUPERPAN_OCTANT_8_TIER_B | MARS |
188 | SUPERPAN_OCTANT_8_TIER_C | MARS |
188 | SUPERPAN_OCTANT_8_TIER_D | MARS |
188 | SUPERPAN_OCTANT_8_TIER_E | MARS |
188 | SUPERPAN_OCTANT_8_TIER_F | MARS |
190 | UPPER_RAD_CAL_6_COLORS_AND_PHOTOMETRIC_SPOTS | CALIMG or MARS |
191 | UPPER_RAD_CAL_4_COLOR | CALIMG |
194 | BOTH_RAD_CAL_6_COLORS_AND_PHOTOMETRIC_SPOTS | CALIMG or MARS |
195 | LOWER_RAD_CAL_5+1_AND_PHOTOMETRIC_SPOT | CALIMG or MARS |
195 | LOWER_RAD_CAL_6_COLORS_AND_PHOTOMETRIC_SPOTS | CALIMG or MARS |
196 | BOTH_RAD_CAL_1+1_POINTING_SUBFRAME_SCATTERED_LIGHT | CALIMG |
196 | UPPER_RAD_CAL_1+1_POINTING_SUBFRAME_SCATTERED_LIGHT | CALIMG |
199 | SUPER_RESOLUTION_0 | MARS |
199 | SUPER_RESOLUTION_1 | MARS |
199 | SUPER_RESOLUTION_2 | MARS |
199 | SUPER_RESOLUTION_3 | MARS |
199 | SUPER_RESOLUTION_4 | MARS |
250 | IMP_FIDUCIAL_CHECK | CALIMG |
252 | REAR_RAMP_MAGNET | MAG |
257 | TIP_PLATE_MAGNET_DIOPTER_LENS | MAG |
258 | ALTAIR_VEGA_+_PHOBOS_13_FILTERS | STAR or PHOBOS |
259 | PHOBOS_FOG | PHOBOS |
260 | AEROSOL_OPACITY_SUN | SUN |
260 | AEROSOL_OPACITY_SUN_LOW | SUN |
261 | AEROSOL_OPACITY_SUN | SUN |
261 | WATER_OPACITY_SUN_CAL | SUN |
262 | WATER_OPACITY_SUN_EVENING | SUN |
263 | WATER_OPACITY_SUN_EVENING | SUN |
265 | YOGI_PHOTOMETRY | MARS |
266 | MAG_TARG_DEPLOYED_ILLUM_HGA_CN_250_CLK_90 | MAG |
267 | MAG_TARGET_MONITORING_IMP_DEPLOYED_3_FILTERS | MAG or CALIMG |
267 | MAG_TARGET_DAILY_MONITORING_IMP_DEPLOYED_3_FILTERS | MAG or CALIMG |
275 | VERTICAL_STEREO_1 | MARS |
276 | VERTICAL_STEREO_2 | MARS |
277 | VERTICAL_STEREO_3 | MARS |
279 | CHANGE_MONITORING_II | MARS |
280 | HALF_SKY_SURVEY-NORTH_2_COLOR | SKY |
283 | CLOUD_DETECTION | SKY or CALIMG |
288 | DEEP_FIELD_TEST | MARS |
290 | PHOTOMETRIC-STRIP-PM | MARS |
290 | PHOTOMETRIC-STRIP-MORNING | CALIMG |
294 | SUPER_RESOLUTION | MARS |
295 | PHOTOMETRIC-STRIP-PM | MARS |
296 | SUPER_RESOLUTION | MARS |
297 | SUPER_RESOLUTION | MARS |
298 | SUPER_RESOLUTION | MARS |
350 | ROVER_MOVIE | ROVER |
353 | ROVER_CONCURRENT_WAE_IMG | ROVER |
354 | CONCURRENT_FRONT_WHEEL_PUSH_IMG | ROVER |
466 | LOWER_RAD_CAL_DEPLOYED_15_COLOR | CALIMG |
15202 | SUNSET_EVENING_AEROSOL_MEASUREMENTS | SKY |
The final level of directory subdivision is by spacecraft clock start count or "sclk". The first four digits of the ten-digit sclk are used in the directory name; the remaining six digits are used in the file names. The directory name begins with a "c", indicating that the number that follows is a clock count, and ends with "xxx", indicating a range of numbers in the directory. The following table shows the spacecraft clock count range and the command sequences of the images that were acquired each "sol" or planet day number. The planet day number is the Martian day since surface operations began, with the day of the Mars Pathfinder landing being "1" (July 4, 1997). Negative sols refer to data acquired before the spacecraft landed. The last day when science data was returned from the surface was sol 83 (September 27, 1997).
Sol | Spacecraft Clock Count | Command Sequences |
---|---|---|
-194 | 1229455934 - 1229455947 | 0 |
-13 | 1245530232 - 1245531137 | 8 |
1 | 1246747799 - 1246767518 | 1, 2, 8 - 10, 17, 22, 25, 59, 62, 180 |
2 | 1246830148 - 1246879404 | 9, 10, 13, 22, 24, 30 - 33, 35, 44, 51, 52, 55, 59, 60, 64 - 68, 161, 174, 180 |
3 | 1246922727 - 1246979484 | 7, 15, 23, 35, 49, 51, 53 - 55, 60, 69 - 74, 152, 173, 175, 250 |
4 | 1246984293 - 1247042575 | 36, 39, 50, 53 - 56, 59, 60, 151, 154, 156, 172, 261, 353, 354 |
5 | 1247103484 - 1247134363 | 7, 46, 50, 55, 59, 60, 172 |
6 | 1247166077 - 1247245173 | 35, 50, 55, 59, 60, 158, 172, 250, 261, 262, 267 |
7 | 1247249105 - 1247281767 | 59, 60, 155, 156 |
8 | 1247362822 - 1247381899 | 55, 164, 191 |
9 | 1247461885 - 1247465543 | 59, 166, 191 |
10 | 1247540474 - 1247558766 | 50, 55, 60, 164, 172, 175, 267 |
11 | 1247644526 - 1247667452 | 36, 55, 60, 165, 167, 175, 191 |
12 | 1247718030 - 1247777747 | 35, 36, 39, 46, 50, 55, 60, 158, 172, 175, 260, 267 |
13 | 1247780956 - 1247866489 | 35, 36, 39, 46, 50, 53 - 55, 60, 151, 156, 172, 173, 175, 185, 260, 267, 353 |
14 | 1247869697 - 1247955762 | 35, 39, 46, 50, 51, 55, 60, 151, 154, 156, 172, 173, 175, 196, 199, 260 - 262, 267 |
15 | 1247958470 - 1248043453 | 7, 35, 36, 39, 46, 50, 54, 55, 60, 151, 156, 158, 172, 173, 175, 260, 263 |
16 | 1248059512 - 1248070341 | 151, 162 |
18 | 1248261679 - 1248288282 | 50, 51, 53 - 55, 60, 172, 173, 175, 182, 261, 263, 267, 466 |
19 | 1248339450 - 1248377542 | 36, 39, 46, 55, 60, 173, 175, 179, 252, 260, 267 |
20 | 1248407687 - 1248488477 | 35, 46, 50, 54, 55, 60, 154, 156, 172, 173, 175, 188, 199, 258, 260, 261, 267, 466 |
21 | 1248491877 - 1248577248 | 35, 39, 46, 50, 55, 56, 60, 156, 158, 172, 173, 175, 190, 195, 260, 263, 266, 267, 280 |
22 | 1248580652 - 1248666028 | 15, 35, 36, 50, 55, 60, 152, 156, 172, 173, 175, 260, 267, 1520 |
23 | 1248669426 - 1248754802 | 7, 35, 36, 39, 46, 54, 55, 60, 156, 158, 162, 172, 173, 175, 199, 252, 257, 260, 350 |
24 | 1248758201 - 1248843578 | 35, 36, 39, 46, 50, 55, 60, 152, 162, 173, 175, 179, 259, 260, 1520 |
25 | 1248846980 - 1248932352 | 35, 36, 51, 55, 60, 151, 154 - 156, 158, 175, 191, 199, 260 - 262 |
26 | 1248935755 - 1248999060 | 35, 36, 39, 50, 55, 60, 156, 173, 175, 260, 267 |
27 | 1249053327 - 1249086979 | 50, 53 - 55, 60, 173, 175, 260, 267, 283, 290, 295 |
28 | 1249141978 - 1249176630 | 36, 53, 55, 60, 173, 175, 179, 260, 267 |
29 | 1249230714 - 1249234574 | 60, 175, 290 |
30 | 1249327087 - 1249339269 | 50, 54, 55, 60, 173, 175, 267 |
32 | 1249501633 - 1249553780 | 35, 36, 50, 55, 60, 173, 175, 184, 257, 260 - 262 |
33 | 1249557179 - 1249610784 | 7, 35, 39, 50, 53, 55, 60, 156, 162, 173, 175, 260 |
34 | 1249678267 - 1249700185 | 55, 60, 171, 173, 175, 186, 267 |
35 | 1249766743 - 1249788649 | 55, 60, 172, 173, 175, 179, 267, 294, 297 |
36 | 1249855505 - 1249877079 | 15, 55, 60, 173, 175, 186, 196, 267, 275 |
37 | 1249944280 - 1249965854 | 15, 53, 55, 60, 173, 175, 185, 186 |
38 | 1250033055 - 1250086206 | 15, 35, 36, 51, 60, 173, 175, 183, 188, 194, 195, 260, 261, 267, 276, 277, 466 |
39 | 1250089605 - 1250143589 | 35, 39, 53, 55, 60, 151, 156, 162, 173, 175, 190, 194, 260, 267 |
40 | 1250210604 - 1250227270 | 7, 60, 173, 175, 283, 297 |
41 | 1250304397 - 1250310442 | 15, 55, 60, 173, 186 |
42 | 1250388155 - 1250403239 | 15, 50, 55, 60, 173, 175, 187, 267 |
44 | 1250565703 - 1250574341 | 15, 50, 56, 60, 173, 175, 181, 267 |
47 | 1250839150 - 1250839174 | 56 |
49 | 1251009882 - 1251024647 | 50, 54, 60, 173, 175 |
50 | 1251098642 - 1251118168 | 54, 55, 60, 173, 175, 267 |
52 | 1251276247 - 1251295182 | 7, 15, 50, 54, 55, 60, 173, 175, 288 |
53 | 1251365020 - 1251372802 | 50, 54, 55, 60, 173, 175, 267 |
54 | 1251453602 - 1251470240 | 15, 54, 55, 60, 173, 175, 183, 267 |
55 | 1251542386 - 1251574951 | 7, 15, 36, 55, 60, 173, 175, 182, 187, 195, 260, 265, 466 |
56 | 1251604264 - 1251649732 | 15, 39, 55, 60, 155, 158, 162, 173, 175, 190, 260, 265, 267, 283 |
57 | 1251719965 - 1251721489 | 15, 60, 175, 183 |
58 | 1251808714 - 1251817460 | 60, 173, 175, 267, 298 |
59 | 1251897621 - 1251912101 | 50, 55, 60, 175 |
60 | 1251986403 - 1252001360 | 55, 60, 173, 175, 267 |
61 | 1252075187 - 1252090991 | 60, 173, 175, 267 |
62 | 1252163969 - 1252182364 | 7, 60, 173, 175 |
63 | 1252252751 - 1252262891 | 60, 173, 175, 267 |
64 | 1252341337 - 1252359834 | 50, 54, 60, 175, 179, 267 |
65 | 1252430692 - 1252448618 | 53, 60, 173, 175, 267, 279, 283, 296 |
66 | 1252518903 - 1252537564 | 15, 50, 55, 60, 173, 175, 178, 181, 184, 185, 199, 257, 267 |
67 | 1252607685 - 1252626161 | 50, 55, 60, 173, 175, 267, 298 |
68 | 1252696473 - 1252722326 | 15, 53, 55, 60, 173, 175, 181, 267, 283 |
69 | 1252757190 - 1252803749 | 15, 60, 154, 155, 158, 173, 175, 187, 267, 297 |
70 | 1252874105 - 1252892509 | 7, 15, 50, 55, 60, 173, 175, 183 |
71 | 1252971823 - 1252978716 | 55, 60, 175, 199, 267 |
72 | 1253051760 - 1253070156 | 50, 51, 55, 60, 173, 175, 267, 297, 298 |
73 | 1253140544 - 1253145585 | 60, 175 |
74 | 1253229326 - 1253245120 | 50, 55, 60, 175, 199, 267, 283, 296 |
75 | 1253318109 - 1253328272 | 15, 55, 60, 173, 183, 265 |
76 | 1253406891 - 1253417652 | 15, 56, 60, 175, 181, 267, 298 |
77 | 1253495656 - 1253502191 | 15, 56, 60, 173, 183, 186 |
78 | 1253584457 - 1253595729 | 50, 56, 60, 175, 179, 257 |
79 | 1253673212 - 1253678269 | 60, 175, 196 |
80 | 1253761994 - 1253769706 | 55, 60, 175, 267, 296 |
81 | 1253850777 - 1253855828 | 60, 175 |
82 | 1253939542 - 1253958186 | 51, 60, 173, 175, 199, 283 |
83 | 1254028324 - 1254046834 | 15, 60, 175, 183, 298 |
A sample data directory structure might look like this:
APXSSITE----SEQ0071-----C1246XXX SEQ0072-----C1246XXX CALIMG------SEQ0007-----C1246XXX |--------C1247XXX : : SEQ0015-----C1246XXX |--------C1248XXX : : PHOBOS------SEQ0155-----C1247XXX : :
The contents of the data subdirectories are image files with attached PDS labels, as shown in the following table.
File | Contents | Source |
---|---|---|
WXXXXXXY.ZZZ (e.g. I392384R.IMG) |
Experiment Data Record with attached PDS label. (Complete format descriptions provided in reference 5 and DATASET.CAT.) | MIPS / IMP team |
According to PDS and ISO-9660 level 1 standards, filenames on the CDs are limited to the "8.3" format, ie., eight characters, followed by a period ".", followed by a three character extension. Therefore, the names for the individual images will consist of an instrument identifier, followed by the six least significant digits of the spacecraft clock count, followed by a single character frame identifier, followed by a three character representation of the image observation type. The filenames will be of the form WXXXXXXY.ZZZ, where:
Possible Values | Meaning | ||
---|---|---|---|
W | instrument identifier | I | Imager for Mars Pathfinder |
XXXXXX | clock count | (any six digit integer) | six least significant digits of Spacecraft Clock Start count |
Y | frame identifier | L | left image |
R | right image | ||
S | dark strip | ||
N | null strip | ||
ZZZ | file extension | IMG | regular image |
STR | dark strip | ||
NUL | null strip | ||
FLT | flat field | ||
DRK | dark field | ||
HST | histogram | ||
SUM | summed |
Given the combination of directory name and filename, the complete spacecraft clock count can be determined for any image from the table above. The image filenames may not be unique; it is always best to use the product id when looking for a unique image identifier.
The browse directory contains HTML, GIF, and JPEG files designed to allow for the easy perusal of the data on the CD. This HTML "browser" begins at the top level with the INDEX.HTM file in the BROWSE directory. Beneath this, the browse directory contains a directory structure identical to that of the data subdirectories. Each of these browse subdirectories contains JPEG-formatted thumbnail-sized and GIF-formatted full-sized versions of the images in the equivalent data directory. They also contain HTML files describing both the individual images, and whole directories.
The GIF and JPEG files, and the HTML files describing individual images, all have identical names to the images they describe, except that the file extensions have been changed to ".GIF", ".JPG", and ".HTM" respectively. PDS labels with ".LBL" extensions are also present, describing the other files in each directory.
A PDS KEYWORDS AND THEIR DEFINITIONS
A.1 IMAGE AND TABLE LABEL KEYWORDS
The following table lists, in alphabetical order, the PDS keywords that are used in the IMP EDR image labels and the INDEX, COMMAND, and EDRINDEX tables that describe them. Any keywords that are shown in lower case characters are used solely as column names in the tables, and are therefore not necessarily formal PDS keywords. Please note that the definitions provided are often specific to the Mars Pathfinder mission. Formal PDS definitions are available in the Planetary Science Data Dictionary (reference 3).
Many of these definitions make reference to various MPF-specific coordinate systems. For details, please see the Mars Pathfinder AIM Phasing and Coordinate Frame Document (reference 7) or the DATASET.CAT file, which is included on the IMP EDR CDs.
There are also a variety of keywords and terms used below which are related to the various data compression methods used on-board the spacecraft. For details on these, please see the DATASET.CAT file.
PDS Keyword | Mars Pathfinder Definition | |||||||||||||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
APPLICATION PACKET ID | The id of the telemetry packet queue to which the image data was directed. For details see application packet name. | |||||||||||||||||||||||||||||||||||||||
APPLICATION PACKET NAME | The name associated with the telemetry packet queue to which the
image data was directed. The queues are distinguished on the basis of
type and priority of data. The ids and names that were used during
the mission are shown below:
|
|||||||||||||||||||||||||||||||||||||||
atmos flag | A flag that indicates that the given observation was directed at the sun. | |||||||||||||||||||||||||||||||||||||||
AUTO EXPOSURE DATA CUT | The DN value which a specified fraction of pixels is permitted to exceed. The fraction is specified using the auto exposure pixel fraction keyword. Valid range: 0 to 4095 | |||||||||||||||||||||||||||||||||||||||
AUTO EXPOSURE PIXEL FRACTION | The percentage of pixels whose value is higher than the number specified by the auto exposure data cut keyword. This field is only applicable if the exposure type is set to AUTO or INCREMENTAL. Valid range: 0 to 100 | |||||||||||||||||||||||||||||||||||||||
AZIMUTH FOV | The angular measure of the horizontal field of view of an imaged scene. For MPF, "horizontal" is measured in the x-y plane of the IMP coordinate system. | |||||||||||||||||||||||||||||||||||||||
AZIMUTH MOTOR CLICKS | The number of motor step counts the camera rotated in the horizontal direction from the low hard stop. Since each step count is 0.553 degrees, the approximate azimuthal position of the camera can be derived from this value. Valid range is 0 to 1023. | |||||||||||||||||||||||||||||||||||||||
BAD PIXEL REPLACEMENT FLAG | Indicates whether or not bad pixel replacement processing was completed. If set to TRUE, certain pixels in the image were replaced based on a bad pixel table. Valid values: TRUE, FALSE. | |||||||||||||||||||||||||||||||||||||||
BANDS | The number of spectral bands in the image. Value: 1 | |||||||||||||||||||||||||||||||||||||||
CHECKSUM | An unsigned 32-bit sum of every byte of data in the image data object. | |||||||||||||||||||||||||||||||||||||||
COMMAND DESC command description |
The textual description associated with a COMMAND NAME. The valid
values for the IMP EDRs are shown below.
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COMMAND NAME | The name of an uplinked command sent to a spacecraft or instrument. For the IMP EDRs, this indicates the method the IMP camera was instructed to use to determine its pointing direction. For details, see command desc. | |||||||||||||||||||||||||||||||||||||||
COMMAND SEQUENCE NUMBER | A numeric identifier for a sequence of commands sent to a spacecraft or instrument. For the IMP EDRs, these are specifically the commands sent to the IMP camera, ordering it to perform a particular task. Valid range is 1 to 9999. For a complete list of the command sequence numbers used during the mission and their descriptions, see Table 3.2.2.6.B of this document. | |||||||||||||||||||||||||||||||||||||||
command version number | The version number of the command. The commands (ie., IMAGE_IDs) were intended to be unique, but in a few cases they were re-used with different command parameters. This keyword was added to distinguish between differing versions of the commands. Valid range is 1 to 9, where the lowest version number reflects the oldest version of a command. | |||||||||||||||||||||||||||||||||||||||
DARK CURRENT CORRECTION FLAG | A flag indicating whether or not a dark current correction was applied to the image. For MPF, this correction was applied to the image on board the spacecraft, before the image was transmitted to Earth. Valid values: TRUE, FALSE | |||||||||||||||||||||||||||||||||||||||
DARK CURRENT DOWNLOAD FLAG | A flag indicating whether or not an image of the dark strip area of the CCD was downlinked along with the image data. Valid values: TRUE, FALSE | |||||||||||||||||||||||||||||||||||||||
DATA SET ID | A unique alphanumeric identifier for a data set. Value: MPFL-M-IMP-2-EDR-V1.0 | |||||||||||||||||||||||||||||||||||||||
DATA SET NAME | The full name given to a data set. Typically identifies the instrument that acquired the data, the target of that instrument, and the processing level of the data. Value: MPF LANDER MARS IMAGER FOR MARS PATHFINDER 2 EDR V1.0 | |||||||||||||||||||||||||||||||||||||||
DETECTOR PIXEL HEIGHT | The height of a pixel in the CCD sensor measured in microns. Value: 23.0 | |||||||||||||||||||||||||||||||||||||||
DETECTOR PIXEL WIDTH | The width of a pixel in the CCD sensor measured in microns. Value: 23.0 | |||||||||||||||||||||||||||||||||||||||
DOWNLOAD TYPE | Specifies which image data to download, any or all of: image data (IM), dark current strip (DS), and null pixel data (NS). Valid values: NONE, DS, IM, DSIM, NS, DSNS, IMNS, DSIMNS | |||||||||||||||||||||||||||||||||||||||
EARTH RECEIVED START TIME | Identifies the earliest time that a telemetry packet containing data for the image was received. Has the form "YYYY-MM-DDThh:mm:ss.fffZ". | |||||||||||||||||||||||||||||||||||||||
EARTH RECEIVED STOP TIME | Identifies the latest time that a telemetry packet containing data for the image was received. Has the form "YYYY-MM-DDThh:mm:ss.fffZ". | |||||||||||||||||||||||||||||||||||||||
ELEVATION FOV | The angular measure of the vertical field of view of an imaged scene. For MPF, "vertical" is measured along the ZIMP axis of the IMP coordinate system. | |||||||||||||||||||||||||||||||||||||||
ELEVATION MOTOR CLICKS | The number of motor step counts the camera rotated in the vertical direction from the low hard stop. Since each step count is 0.553 degrees, the approximate elevational position of the camera can be derived from this value. Valid range is 0 to 1023. | |||||||||||||||||||||||||||||||||||||||
ERROR PIXELS | After all decompression and post decompression processing has been completed, this is the number of pixels that are outside the valid DN range of 0 to 4095. | |||||||||||||||||||||||||||||||||||||||
EXPECTED PACKETS | The total number of telemetry packets which constitute a complete image, ie., an image without missing data. | |||||||||||||||||||||||||||||||||||||||
EXPOSURE COUNT | Maximum number of exposures taken. Value is dependant on exposure type. Valid range: 0 - 16 | |||||||||||||||||||||||||||||||||||||||
EXPOSURE DURATION | Provides the value of the time interval between the opening and closing of an instrument aperture. The IMP camera does not have a shutter in the traditional sense, so for MPF this value is the integration time for manual and auto exposure, measured in milliseconds. | |||||||||||||||||||||||||||||||||||||||
EXPOSURE TYPE | Exposure type for the image. Valid values: AUTO, INCREMENTAL, MANUAL, PRETIMED, NONE. The auto and incremental exposures iterate off a starting value to determine the exposure time. For auto exposures, the value is preset. Incremental exposures start with the exposure time of the previous exposure. Manual exposure is a single exposure with a set exposure time. Pre-timed exposure uses the very last exposure time used, regardless of the type of exposure that it was. No exposure indicates that the command moves only the camera and doesn't take an exposure. | |||||||||||||||||||||||||||||||||||||||
file name | This is the name of the PDS formatted file as it is stored on the CD-ROM archive media. For the IMP EDRs, it consists of the instrument identifier "I", followed by the six least significant digits of the spacecraft clock start count, followed by a frame identifier (L=left, R=right, S=dark strip, N=null strip), followed by a 3 character extension. The extension indicates the image observation type as follows: IMG=regular, STR=dark strip, NUL=null strip, FLT=flat field, DRK=dark current, HST=histogram, and SUM=summation. (Note that the latter two values were never used.) | |||||||||||||||||||||||||||||||||||||||
FILE RECORDS | The number of physical file records, including both label records and data records, in a file. | |||||||||||||||||||||||||||||||||||||||
FILTER NAME | The name of the instrument filter through which the image was
acquired. The numbers refer to the effective wavelength in nm of the
filter for the left (L) or right (R) eye.
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FILTER NUMBER | The number of the instrument filter through which the image was acquired. (See filter name for details.) | |||||||||||||||||||||||||||||||||||||||
FIRST LINE | The line within a source image that corresponds to the first line in the sub-image. For the IMP EDRs, the source image is the complete 256x256 image area within the CCD. | |||||||||||||||||||||||||||||||||||||||
FIRST LINE SAMPLE | The sample within a source image that corresponds to the first sample in the sub-image. For the IMP EDRs, the source image is the complete 256x256 image area within the CCD. | |||||||||||||||||||||||||||||||||||||||
FLAT FIELD CORRECTION FLAG | Indicates whether or not a flat field correction was applied to the image. For MPF, this correction was applied to the image on board the spacecraft, before the image was transmitted to Earth. Valid values: TRUE, FALSE | |||||||||||||||||||||||||||||||||||||||
FRAME ID | Provides an identification for a particular instrument frame. Valid values are LEFT, RIGHT, BOTH, and HALFL. The IMP camera nominally operates in a mode where both the left and right images are exposed and transferred into the frame buffer simultaneously. Then either the RIGHT, LEFT, or BOTH frames are transmitted. For even shorter shutter times, the left image only may be transferred into the frame buffer (HALFL). The presence of BOTH in this field indicates that the image should be part of a stereo pair. | |||||||||||||||||||||||||||||||||||||||
grid position x, grid position y, grid position z |
The x (north/south), y (east/west), and z (vertical) components of a position defining the IMP pointing, measured with respect to the Martian Local Level Coordinate Frame (M Frame). Positive x is north, positive y is east, and positive z is down. Units are measured in meters. For details, see [MELLSTROM&LAU1996]. | |||||||||||||||||||||||||||||||||||||||
histogram flag | A flag to indicate that the product returned was a histogram. | |||||||||||||||||||||||||||||||||||||||
^IMAGE | A pointer to the first record of the image data within a PDS image file. | |||||||||||||||||||||||||||||||||||||||
IMAGE ID | Uniquely identifies the observation parameters of an image. The
most significant four digits identify the command sequence that
contains the imaging command. The middle two digits indicate the
version of the command sequence, and the right four digits identify
the image within a single imaging sequence. If the image id is even and non-zero, it is a left frame image. If the image id is one greater than the left frame image id (and therefore odd), it is the right frame of a stereo image. NOTE: During operations, a small number of image ids were re-used with different command parameters. This eliminates the uniqueness of the image id for those images. The TLM CMD DISCREPANCY FLAG may be useful in identifying images that have this problem. |
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IMAGE OBSERVATION TYPE | Identifies the type or purpose of an observation. Valid values
are shown in the table below.
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IMAGE TIME | Date and time at which the image was acquired, recorded in UTC system format. Shown as: "YYYY-MM-DDThh:mm:ss.fffZ". | |||||||||||||||||||||||||||||||||||||||
INST CMPRS BLK SIZE | The dimensions of a block for on-board compression. In the PDS labels, the value is a two dimensional array, where the first value is the line dimension of the block, and the second value is the sample dimension of the block. In the EDRINDEX.TAB file, it is a single value, the product of the line dimension and the sample dimension. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS BLOCKS | The number of blocks used to spatially segment the image file prior to compression. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS MODE | The targetted image quality or compression factor for on-board compression. Compression is obtained with Huffman or arithmetic entropy encoding, with or without LCT. Odd modes specify a targetted image quality, whereas even modes specify a targetted compression factor. Modes 1,2,5,6 utilize Huffman encoding; modes 3,4,7,8 use arithmetic encoding. Modes 5,6,7,8 use LCT. Mode 9 specifies RICE compression. Valid values: 1 to 9. (See inst cmprs name.) | |||||||||||||||||||||||||||||||||||||||
INST CMPRS NAME | The type of on-board compression used for data storage and
transmission. Valid values are shown below:
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INST CMPRS PARAM | This is a JPEG specific variable. It selects the on-board compression rate by image quality or by compression factor, based on selected on-board compression mode. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS QUALITY | A JPEG specific variable. If an odd IMP compression mode is used for on-board compression, this is the desired image quality index. If an even IMP compression mode is used, this is the resultant image quality used to reach a desired on-board compression factor. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS QUANTZ TBL ID | The identifier for the reference table used for quantization in the frequency domain for on-board transform compression. This name or code should be specific enough to allow the user of the data to have sufficient information to reference the quantization table used to compress the data. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS QUANTZ TYPE | The method of quantization used for the output of transform coders. Valid value: TABULAR | |||||||||||||||||||||||||||||||||||||||
INST CMPRS RATE | The average number of bits needed to represent a pixel for an on-board compressed image. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS RATIO | The ratio of the size, in bytes, of the original uncompressed data file to its compressed form. | |||||||||||||||||||||||||||||||||||||||
INST CMPRS SYNC BLKS | RICE specific variable. Number of compressed blocks between sync markers. | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT AZIMUTH | One of two angular measurements of the pointing direction of the instrument. The azimuth is measured positively in the clockwise direction (as viewed from above) from a fixed reference direction. The angle is measured in the x-y plane of the instrument's coordinate system, which is not necessarily co-linear with the surface fixed coordinate system. Note that for the MPF IMP, the reference direction is the YIMP axis of the IMP coordinate frame, and is co-linear with the YL axis of the lander coordinate frame. Valid values: 0 to 360 degrees | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT AZIMUTH METHOD | Identifies the method used to calculate the instrument azimuth from the azimuth motor clicks. Valid values: TELEMETRY, MPFNAV-MIPS, BACKLASH-UOFA | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT DEPLOYMENT STATE | Indicates whether or not the IMP camera had been deployed to the end of its 62 cm mast at the time the image was acquired. Valid values are STOWED and DEPLOYED. | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT ELEVATION | One of two angular measurements of the pointing direction of the instrument. The positive direction of the elevation is set by the positive elevation direction data element, which for MPF is UP. The elevation is measured with respect to the plane which is co-planar with the x-y plane of the instrument's coordinate system and which intersects the elevation axis around which the camera rotates. This is not necessarily co-linear with the surface fixed coordinate system. Valid values: -90 degrees (nadir) to +90 degrees (zenith) | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT ELEVATION METHOD | Identifies the method used to calculate the instrument elevation from the elevation motor clicks. Valid values: TELEMETRY, MPFNAV-MIPS, BACKLASH-UOFA | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT HOST NAME | The full name of the host on which an instrument is based. Value: MARS PATHFINDER LANDER | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT ID | An abbreviated name or acronym which identifies an instrument. Value: IMP | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT NAME | The full name of an instrument. Value: IMAGER FOR MARS PATHFINDER | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT TEMPERATURE instrument ccd temperature, instrument head temperature |
The temperature, in degrees Celcius, of the CCD sensor array and the camera head when the image was acquired. This is an array of two elements. (The values in the index tables are stored in two separate columns named instrument ccd temperature and instrument head temperature, respectively.) | |||||||||||||||||||||||||||||||||||||||
INSTRUMENT TEMPERATURE COUNT | The raw temperature counts of the CCD and camera head when the image was acquired. This is an array of two elements. | |||||||||||||||||||||||||||||||||||||||
INTERCHANGE FORMAT | The manner in which the data elements are stored. Value: BINARY | |||||||||||||||||||||||||||||||||||||||
ivp target name | Identifies the image vector pointing object at which the IMP camera was aimed. Valid values include SUN, EARTH, and PHOBOS. Note that the camera was "tricked" into pointing at other objects (like Deimos or stars) by directing it to point at Phobos, but re-defining the position of Phobos in the sky. | |||||||||||||||||||||||||||||||||||||||
LABEL RECORDS | The number of physical file records that contain only label information. The number of data records in a file is determined by subtracting the number of label records from the number of file records. | |||||||||||||||||||||||||||||||||||||||
LANDER SURFACE QUATERNION lander surface quaternion x, lander surface quaternion y, lander surface quaternion z, lander surface quaternion a |
An array of four values that define the relationship between the lander coordinate frame and the local level coordinate frame. These values are listed in the NAIF defined order of "cosine, x, y, z". (In the index tables, these values are split out into four separate columns.) | |||||||||||||||||||||||||||||||||||||||
LINE SAMPLES | The total number of pixels along the horizontal axis of an image. | |||||||||||||||||||||||||||||||||||||||
LINES | The total number of pixels along the vertical axis of an image. | |||||||||||||||||||||||||||||||||||||||
MAXIMUM | The maximum DN value in the image file. For the IMP, this range is 0 - 4095. | |||||||||||||||||||||||||||||||||||||||
MEAN | The average of the DN values in the image array. For MPF, this is the average of only those pixels within the valid DN range of 0 to 4095. | |||||||||||||||||||||||||||||||||||||||
MEDIAN | The median of the DN values in the image array. For MPF, this is the median value of only those pixels within the valid DN range of 0 to 4095. This value will be at most 8 DN greater than or equal to the true median value. | |||||||||||||||||||||||||||||||||||||||
MINIMUM | The minimum DN value in the image file. For the IMP, this range is 0 - 4095. | |||||||||||||||||||||||||||||||||||||||
MISSION NAME | A major planetary mission or project. Value: MARS PATHFINDER. | |||||||||||||||||||||||||||||||||||||||
MPF LOCAL TIME | Local time at the lander site on the surface of Mars, measured in local hours, minutes, and seconds, from midnight. Local hours are defined as one twenty-fourth of a local solar day. Local minutes are one sixtieth of a local hour, and local seconds are one sixtieth of a local minute. Format is hh:mm:ss. Based on the IAU standard for the Martian prime meridian. See [DAVIESETAL1994] for more details. | |||||||||||||||||||||||||||||||||||||||
OBSERVATION NAME | The purpose of an observation or sequence of commands. See Table 3.2.2.6.B in this document for a complete listing of the values. | |||||||||||||||||||||||||||||||||||||||
packet map mask | A series of binary digits identifying which of the expected packets were actually received. The bits are to be read left to right. Ie., the first packet is represented by the leftmost bit. | |||||||||||||||||||||||||||||||||||||||
path name | Path to directory containing file. This path is shown in UNIX format. It begins at the root level of the CD. It has a trailing slash, but no leading slash. | |||||||||||||||||||||||||||||||||||||||
PDS VERSION ID | The version number of the PDS standards documents that is valid when a data product label is created. For the Mars Pathfinder IMP EDRs, the version is 'PDS3'. | |||||||||||||||||||||||||||||||||||||||
PIXEL AVERAGING HEIGHT | The vertical dimension, in pixels, of the area over which pixels were averaged prior to image compression. | |||||||||||||||||||||||||||||||||||||||
PIXEL AVERAGING WIDTH | The horizontal dimension, in pixels, of the area over which pixels were averaged prior to image compression. | |||||||||||||||||||||||||||||||||||||||
PLANET DAY NUMBER | The Martian day (ie., sidereal day, equal to a rotation of 360 degrees) on which the image was taken. Starts with 1 as the first day of surface operations, the day the spacecraft landed. Negative values refer to pre-surface images. | |||||||||||||||||||||||||||||||||||||||
POSITIVE ELEVATION DIRECTION | The direction in which elevation is measured in positive degrees for an observer on the surface of a body. The elevation is measured with respect to the azimuthal reference plane. A value of UP indicates that elevation is measured positively upwards, ie., the zenith point would be at +90 degrees and the nadir point at -90 degrees. DOWN indicates that the elevation is measured positively downwards; the zenith point would be at -90 degrees and the nadir point at +90 degrees. | |||||||||||||||||||||||||||||||||||||||
PROCESSING HISTORY TEXT | A textual summary of the processing used to produce the image file. | |||||||||||||||||||||||||||||||||||||||
PRODUCER FULL NAME | The full name of the individual mainly responsible for the production of a data set. Value: ALLAN J. RUNKLE | |||||||||||||||||||||||||||||||||||||||
PRODUCER ID | A short name or acronym for the producer or producing team/group of a dataset. Value: MIPL OF JPL | |||||||||||||||||||||||||||||||||||||||
PRODUCER INSTITUTION NAME | A university, research center, NASA center, or other institution associated with the production of a data set. This would generally be an institution associated with the producer full name. Value: MULTIMISSION IMAGE PROCESSING LABORATORY, JET PROPULSION LAB | |||||||||||||||||||||||||||||||||||||||
PRODUCT CREATION TIME | Defines the UTC time when a product was created or last modified. Has the form "YYYY-MM-DDThh:mm:ss.fffZ". | |||||||||||||||||||||||||||||||||||||||
PRODUCT ID | A permanent, unique identifier assigned to each data product. For the IMP EDRs, this is constructed from the words "IMP_EDR" followed by the spacecraft clock start count, followed by the image observation type, followed by the image id. | |||||||||||||||||||||||||||||||||||||||
RECEIVED PACKETS | The total number of telemetry packets which constitute a reconstructed image. | |||||||||||||||||||||||||||||||||||||||
RECORD BYTES | The number of bytes in a physical file record, including record terminators and separators. | |||||||||||||||||||||||||||||||||||||||
RECORD TYPE | The record format of a file. Value: FIXED_LENGTH | |||||||||||||||||||||||||||||||||||||||
RICE OPTION VALUE | RICE compressor specific variable. | |||||||||||||||||||||||||||||||||||||||
RICE START OPTION | RICE compressor specific variable. | |||||||||||||||||||||||||||||||||||||||
SAMPLE BIT MASK | A mask identifying the active bits in a sample. | |||||||||||||||||||||||||||||||||||||||
SAMPLE BITS | The number of bits, or units of binary information contained in a line sample value. | |||||||||||||||||||||||||||||||||||||||
SAMPLE TYPE | The data storage representation of a sample value. Value: MSB_UNSIGNED_INTEGER | |||||||||||||||||||||||||||||||||||||||
SHUTTER EFFECT CORRECTION FLAG | Indicates whether or not a shutter effect correction was applied to the image. The shutter effect correction involves the removal from the image of the shutter, or fixed-pattern. For MPF, this correction was applied to the image on board the spacecraft, before the image was transmitted to Earth. Valid values: TRUE, FALSE | |||||||||||||||||||||||||||||||||||||||
SOFTWARE NAME | The name of the telemetry processing software used to generate the image data. | |||||||||||||||||||||||||||||||||||||||
SOFTWARE VERSION ID | Indicates the version or development level of a program or a program library used to generate the data. | |||||||||||||||||||||||||||||||||||||||
SOLAR AZIMUTH | One of two angular measurements indicating the position of the Sun as measured from a specific point on the surface of a planet (ex., from a lander or rover). The azimuth is measured positively in the clockwise direction (as viewed from above) with the meridian passing through the positive spin axis of the planet (ie., the north pole) defining the zero reference. | |||||||||||||||||||||||||||||||||||||||
SOLAR ELEVATION | One of two angular measurements indicating the position of the Sun as measured from a specific point on the surface of a planet (ex., from a lander or rover). The positive direction of the elevation is set by the positive elevation direction data element. It is measured from the plane which is perpendicular to the line passing between the observer and the planet's center and which intersects the observer. | |||||||||||||||||||||||||||||||||||||||
SOURCE PRODUCT ID | Identifies a product used as input to create a new product. For MPF, this refers to the filenames of the SPICE kernels used to produce the image and its ancillary data. | |||||||||||||||||||||||||||||||||||||||
SPACECRAFT CLOCK START COUNT | The value of the lander clock (in seconds) at which the image was acquired. | |||||||||||||||||||||||||||||||||||||||
SQRT COMPRESSION FLAG | Indicates whether or not square root compression was applied to the image. For MPF, this compression was performed onboard the lander, prior to transmission of the data to Earth. It involved the compression of the pixels from 12 bits down to 8 bits. | |||||||||||||||||||||||||||||||||||||||
SQRT MAXIMUM PIXEL | The maximum pixel value in a 12-bit image prior to square root compression. | |||||||||||||||||||||||||||||||||||||||
SQRT MINIMUM PIXEL | The minimum pixel value in a 12-bit image prior to square root compression. | |||||||||||||||||||||||||||||||||||||||
STANDARD DEVIATION | The standard deviation of the DN values in the image array. For MPF, this is calculated on only those pixels within the valid DN range of 0 to 4095. | |||||||||||||||||||||||||||||||||||||||
subframe flag | A flag to indicate that the image is not full size. Valid values: TRUE, FALSE | |||||||||||||||||||||||||||||||||||||||
sum flag | A flag to indicate that the product returned is a "summation" file. For the IMP EDRs, this means that it contains two records, the first a list of the sums of the image columns, and the second a list of the sums of the image rows. Valid values: TRUE, FALSE | |||||||||||||||||||||||||||||||||||||||
SURFACE BASED INST AZIMUTH | One of two angular measurements of the pointing direction of the
instrument. The azimuth is measured positively in the clockwise
direction (as viewed from above) with the meridian passing through the
positive spin axis ("north pole") defining the zero reference. The
surface based inst azimuth is derived from the instrument pointing and
spacecraft orientation. It is co-linear with the surface fixed
coordinate system, but the origin of the observation may not be
co-incident with the origin of the surface fixed frame. Note that the surface based inst azimuth describes the pointing direction of the instrument rather than the angular coordinates of the target of the observation. If there has been any significant change over time in the position of the observing instrument, this data element cannot be used to uniquely describe the vector to a viewed object. See surface based inst elevation. |
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SURFACE BASED INST ELEVATION | One of two angular measurements of the pointing direction of the
instrument. The positive direction of the elevation is set by the
positive elevation direction data element. It is measured from the
plane which is perpendicular to the local gravity vector and which
intersects the elevation axis around which the instrument rotates.
The surface based inst elevation is derived from the instrument
pointing and spacecraft orientation. It is co-linear with the surface
fixed coordinate system, but the origin of the observation may not be
co-incident with the origin of the surface fixed frame. Note that the surface based inst elevation describes the pointing direction of the instrument rather than the angular coordinates of the target of the observation. If there has been any change over time in the position of the observing instrument, this data element can not be used to uniquely describe the vector to a viewed object. Assuming a flat surface, and combined with the height of the instrument above the surface, it can be used to determine the position of an object; however, given realistic non-flat surfaces, observations from another point of origin are required to determine an object's distance. |
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SURFACE BASED INST METHOD | Identifies the method used to calculate the surface based instrument pointing. Valid values: NULL, L_FRAME-QUATERNION | |||||||||||||||||||||||||||||||||||||||
TARGET NAME | Identifies the intended target of an observation. Can be either a planetary body or a physical object. For the IMP, this is the intended target of the observation, and may not accurately represent what is actually in an image frame. Valid values: ALTAIR, APXS SITE, ARCTURUS, CALIMG, DEIMOS, LANDER, MAG(NETIC TARGET), MARS, PHOBOS, ROVER, SKY, SUN, VEGA, and WINDSOCK. Note that this list does not include specific feature names like "Barnacle Bill" and "Yogi". For details on feature names, please consult the gazetteer on the IMP CDs. | |||||||||||||||||||||||||||||||||||||||
TLM CMD DISCREPANCY FLAG | Indicates whether or not discrepancies were found between the IMP
uplinked commands and the downlinked telemetry. The fields checked
when determining this flag are:
APPLICATION_PACKET_ID Valid values: TRUE, FALSE |
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vector component x, vector component y, vector component z |
The x, y, and z components of a unit vector which defines the commanded IMP pointing. The vector is defined with respect to one of two possible coordinate frames, indicated by the command name. If the command name is IMP_IMAGE_VECTOR, the coordinate system is the IMP camera frame (IMP Frame); if the command name is IMP_IMAGE_LCLVEC, the coordinate system is the Martian Local Level Frame (M Frame). Valid range: -1.0 to 1.0 | |||||||||||||||||||||||||||||||||||||||
volume id | Identifies the CD volume containing the named file. For the IMP EDRs, this consists of the identifier "MPIM_" followed by the four digit volume number. |
B AAREADME FILE
The AAREADME.TXT file contains general information about the contents and format of the CD-ROM.
PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 1998-07-01 INTERCHANGE_FORMAT = ASCII NOTE = "AAREADME.TXT for Mars Pathfinder IMP EDR Archive CD-ROMs." END_OBJECT = TEXT END MARS PATHFINDER IMP EDR ARCHIVE CD-ROM 1. Introduction This CD-ROM is one of three CD-ROMs that contain Mars Pathfinder IMP (Imager for Mars Pathfinder) EDR (Experiment Data Record) images and ancillary files. The spacecraft clock start count ranges of the images contained on the three volumes are shown below. Each volume also contains a complete set of documentation files that describe the archive EDR images. Each EDR image has an attached PDS label that describes the file structure and instrument parameters used for that image. Volume ID SCLK Range --------- ----------------------- MPIM_0001 1229455934 - 1247913223 MPIM_0002 1247913268 - 1249772261 MPIM_0003 1249772268 - 1254046834 The MPF IMP EDR products archived on this volume are the original products released by the Mars Pathfinder project. They have been converted from the VICAR format used during mission operations to a PDS format. Supporting documentation and label files conform to the Planetary Data System (PDS) Standards, Version 3.2, Jet Propulsion Laboratory (JPL) document number D-7669. 2. CD-ROM Format This CD-ROM has been formatted so that a variety of computer systems (e.g., PC, Macintosh, and Sun) may access the data. Specifically, it is formatted according to the ISO-9660 level 1 Interchange Standard. For further information, refer to the ISO-9660 Standard Document: RF# ISO 9660-1988, April 15, 1988. This CD-ROM does not contain any Extended Attribute Records (XARs). Thus, VAX/VMS users on older platforms may have some problems accessing files on this volume. 3. File Formats The Mars Pathfinder IMP EDR images on this set of CD-ROMs are uncompressed, 16-bit files, labelled in conformance with PDS standards. Each image file is stored with a fixed length record format. There is an attached PDS label at the beginning of each image file that describes the content and format of the image. If the PDS label size is not an exact multiple of the file record length, padding is added after the end of the PDS label. Thus, the image object always starts on a record boundary. A more detailed specification of the image file format is given in the EDRSIS and VOLSIS files in the DOCUMENT directory. All detached label and document files (with the exception of PDF formatted files) are stream format files, with a carriage return (ASCII 13) and a line feed character (ASCII 10) at the end of each record. This allows the files to be read by the MacOS, DOS, Unix, and VMS operating systems. The PDF documentation files are in the binary Adobe Portable Document Format. These files can be read with the Adobe Acrobat Reader, available from "http://www.adobe.com/". (If this URL has expired, contact the PDS Operator for more information. Contact information for the PDS is shown in section 8.) All tabular files are described by detached PDS labels, which are label files having the same name as the data files they describe, with the extension .LBL. For example, the file CUMINDEX.TAB is accompanied by the detached label file CUMINDEX.LBL in the same directory. Tabular files are formatted so that they may be read directly into many database management systems (DBMS) or spreadsheet programs on various computers. All fields are separated by commas, and character fields are enclosed in double quotation marks ("). Character fields are left justified, and numeric fields are right justified. The "start byte" and "bytes" values listed in a PDS label do not include the commas between fields or the quotation marks surrounding character fields. The records are of fixed length, and the last two bytes of each record contain the ASCII carriage return and line feed characters. This allows a table to be treated as a fixed length record file on computers that support this file type and as a normal text file on other computers. PDS labels are object-oriented. The object to which the label refers (e.g., IMAGE, TABLE, etc.) is denoted by a statement of the form: ^object = location in which the carat character ('^', also called a pointer in this context) indicates that the object starts at the given location. For an object in the same file as the label, the location is an integer representing the starting record number of the object (the first record in the file is record 1). For an object located outside the label file, the location denotes the name of the file containing the object, along with the starting record or byte number. For example: ^IMAGE = ("C102.IMG",3) indicates that the IMAGE object begins at record 3 of the file C102.IMG, in the same directory as the detached label file. Below is a list of the possible formats that use the ^object keyword. ^object = n ^object = n <BYTES> ^object = "filename.ext" ^object = ("filename.ext",n) ^object = ("filename.ext",n <BYTES>) where: n starting record or byte number of the object, counting from beginning of the file (record 1, byte 1); default is record number. <BYTES> indicates that number given is in units of bytes. filename upper-case file name. ext upper-case file extension. 4. Data Calibration Formal calibration files and software could not be prepared in time to be included on this set of CD volumes. These files will be made available on the CD archive of the IMP derived products. However, some information has already been written about the calibration of the IMP camera, the magnets mounted on the lander, and the windsocks mounted on the ASI/MET mast. This documentation is referenced in the REF.CAT file in the CATALOG directory. See in particular [CROWEETAL1997], [SMITHETAL1997A], and [REIDETAL1998]. 5. Image Display The PDS provides software for displaying PDS formatted images on a variety of computer platforms. The application program for image display is called NASAView, which has versions for SUN, Macintosh, and PC platforms. For some computer platforms, there is a NASAView version that will work as a Web Browser helper application. Since the IMP data is 16-bit, some earlier versions of NASAView may not be able to display it. Versions 1.1.2 and later have been tested and are able to display this data. It is the intention of PDS to distribute NASAView through its World Wide Web and FTP sites. Consult the PDS WWW site for the status of NASAView in terms of its capabilities and availability. The address for the PDS NASAView web site is: http://pds.jpl.nasa.gov/license.html (Complete contact information for the PDS is available below in section 8.) 6. CD-ROM Contents Files on this CD-ROM are organized into a series of subdirectories below the top-level directory. The following table shows the structure and content of these directories. In the table, directory names are enclosed in square brackets ([]). (More details on the contents and structure of the CDs can be found in section 3.2 of the VOLSIS located in the DOCUMENT directory.) FILE CONTENTS Top-level directory | |- AAREADME.TXT The file you are now reading. |- AAREADME.HTM Hypertext version of the AAREADME.TXT file. |- AAREADME.LBL PDS label describing the AAREADME.HTM file. |- ERRATA.TXT List of comments and errors for this | volume set. |- ERRATA.HTM Hypertext version of the ERRATA.TXT file. |- ERRATA.LBL PDS label describing the ERRATA.HTM file. |- VOLDESC.CAT Description of the contents of this CD-ROM | volume in PDS label format. | |- [CATALOG] Directory containing PDS catalog information | | about the Mars Pathfinder IMP EDR data set. | |- CATINFO.TXT Description of files in the CATALOG directory. | |- DATASET.CAT IMP EDR dataset descripton catalog object. | |- INST.CAT IMP instrument description catalog object. | |- INSTHOST.CAT MPF Lander description catalog object. | |- MISSION.CAT MPF mission description catalog object. | |- PERSON.CAT MPF personnel objects. | |- REF.CAT MPF reference objects. | |- [DOCUMENT] Directory containing document files. | |- DOCINFO.TXT Description of files in DOCUMENT directory. | |- CONTACTS.* Contact information for MPF project personnel. | |- DATASET.* MPF IMP EDR dataset description. | |- EDRSIS.* IMP Experiment Data Record SIS. | |- IMPUG.* IMP User's Guide. | |- INST.* Instrument description. | |- INSTHOST.* MPF Lander description. | |- MISSION.* Mars Pathfinder mission description. | |- REF.* References related to MPF. | |- VOLSIS.* MPF IMP EDR CD-ROM specification. | |- [GAZETTER] Directory containing a gazetteer of informal | | feature names at the MPF landing site. | |- GAZINFO.TXT Description of files in the GAZETTER directory. | |- GAZETTER.LBL PDS label for GAZETTER.TAB. | |- GAZETTER.TAB Gazetteer in tabular format. | |- GAZETTER.TXT Description of the gazetteer. | |- [INDEX] Directory containing index files. | |- INDXINFO.TXT Description of files in the INDEX directory. | |- INDEX.TAB Abbreviated volume index in tabular format. | |- INDEX.LBL PDS label for INDEX.TAB. | |- CUMINDEX.TAB Cumulative version of INDEX.TAB. | |- CUMINDEX.LBL PDS label for CUMINDEX.TAB. | |- EDRINDEX.TAB Detailed volume index in tabular format. | |- EDRINDEX.LBL PDS label for EDRINDEX.TAB. | |- COMMAND.TAB List of command parameters in tabular format. | |- COMMAND.LBL PDS label for COMMAND.TAB. | |- [BROWSE] Directory containing the image browser. | |- BROWSER.LBL PDS label for HTML files at top level of | | browser. | |- BRWSINFO.TXT Description of files in the BROWSE directory. | |- DD.HTM Definitions of PDS keywords used in browser. | |- HELP.HTM Help file for browser. | |- INDEX.HTM Top page of the browser. (Start here | | to use the browser.) | |- [ICONS] Directory containing icons used in HTML pages. | |- [UUUUUUUU] Target directories containing HTML pages, GIF | | |- [SEQVVVV] browse images and JPEG thumbnails. Directories | | | |- [CWWWWXXX] beneath this have an identical structure to the | | | | | data directories. | |- [UUUUUUUU] Data directories containing PDS formatted | |- [SEQVVVV] image files. These directories are subdivided | | |- [CWWWWXXX] first by target (UUUUUUUU), then by command | | | |- IYYYYYYZ.IMG sequence number (where VVVV is the four digit | | | | number and finally by spacecraft clock start | | | | count (WWWW represents the four most | | | | significant digits of the clock count). Each | | | | of the bottom level directories contains PDS | | | | formatted data files where YYYYYY represents | | | | the six least significant digits of the SCLK | | | | and Z indicates the frame id, L=left, R=right. | | The top-level data directories are: | |- [APXSSITE] Directory containing images of sites where | the APXS instrument was deployed. | |- [CALIMG] Directory containing images taken for | calibration purposes. This includes images of | the radiometric and fiducial targets on the | lander, flat field and dark current images, | and readouts of the dark strip and null strip | on the CCD. | |- [DEIMOS] Directory containing images targeted at | Deimos. | |- [LANDER] Directory containing images targeted at parts | of the lander to assess its status. This | includes things like the airbag assessment | pan and ramp deployment images. | |- [MAG] Directory containing images aimed at the | various magnetic targets on the lander to | study the magnetic properties of airborne | particles. | |- [MARS] Directory containing the vast majority of the | images, those which were taken primarily to | view the Martian landscape. It includes most | of the major panoramas, the super resolution | images, and the change monitoring images. | |- [PHOBOS] Directory containing images targeted at | Phobos. | |- [ROVER] Directory containing images taken to support | Rover operations and investigations. This | includes things like end of day sequences, | movie sequences, navigation images, and soil | experiment images. | |- [SKY] Directory containing a variety of images | including those taken looking at both high | elevations and at the horizon, and at a | variety of times of day. (Some images may | include the Sun.) Many were taken for the | purpose of studying the atmosphere and the | particles suspended in it. | |- [STAR] Directory containing images targeted at the | stars Altair, Arcturus, and Vega. These are | the one exception to the rule that target = | directory name, since they are all grouped | together in the "STAR" directory. | |- [SUN] Directory containing images targeted at the | Sun, usually for the purpose of studying the | atmosphere. In cases where a sequence of | images, usually around sunset or sunrise, | included some images with the sun and some | without, the sequence has been included in the | SKY directory. | |- [WINDSOCK] Directory containing images targeted at the | windsocks on the ASI/MET mast. More specific details on the file naming conventions used for the image files are available in section 2.2.2 of the EDRSIS or Table 3.2.2.6.E of the VOLSIS, both of which are in the DOCUMENT directory. 7. Image Browser The image browser contained on this volume is a HyperText Markup Language based system that provides a simple search and quick-look capability. The browser is organized on a different basis than the CD volume. The CD image directories are sorted by target, command sequence number, and spacecraft clock start count, while the browser pages are sorted by target and observation name. This was done because the observation name is more descriptive than the command sequence number and should help people unfamiliar with the data find an image they are interested in. However, there is some loose correspondence between observation names and command sequence numbers, so the command sequence numbers have been included alongside observation names in the browser. For details of the relationship between these two values, please see Table 3.2.2.6.B in the VOLSIS, located in the DOCUMENT directory. The system consists of an HTML page for each image that displays a GIF version of the image and a limited portion of its respective label data. Each full resolution data file may be accessed directly from its corresponding HTML page. To use the image browser, open up the BROWSE/INDEX.HTM file in your web browser. For a more comprehensive search engine and browser for the data, please used the Planetary Image Atlas, available from the WWW page of the PDS Imaging Node: "http://www-pdsimage.jpl.nasa.gov/PDS/". 8. Whom to Contact for Information For questions concerning this volume set, contact: PDS Imaging Node Susan K. LaVoie M/S 168-527 Jet Propulsion Laboratory 4800 Oak Grove Drive Pasadena, CA 91109-8099 (818) 354-5677 WWW Site: http://www-pdsimage.jpl.nasa.gov/PDS/ E-mail: pds_imaging@www-pdsimage.jpl.nasa.gov For general information related to the PDS, contact: Planetary Data System, PDS Operator M/S 202-101 Jet Propulsion Laboratory 4800 Oak Grove Drive Pasadena, CA 91109-8099 (818) 354-4321 WWW Site: http://pds.jpl.nasa.gov/ E-mail: pds_operator@jpl.nasa.gov 9. Cognizant Persons & Acknowledgments The IMP camera was supplied by Principal Investigator Peter Smith at the University of Arizona Lunar and Planetary Laboratory. This volume set was designed and produced at the Jet Propulsion Laboratory, Pasadena, California by Elizabeth Duxbury. The following people provided assistance in various capacities: PDS Standards, Keywords, etc: Betty Sword, Steve Hughes, Karen Law, and Jean Mortellaro (PDS-CN JPL), Eric Eliason and Janet Barrett (PDS-IMG, U.S. Geological Survey, Flagstaff, Arizona), Charles Acton (PDS-NAIF, JPL), and Joe Mafi (PDS-PPI UCLA, Los Angeles, California) Data Preparation and Documentation: Doug Alexander, Sue LaVoie, Jean Lorre, Justin Maki, Allan Runkle, and Pamela Woncik (Multimission Image Processing Laboratory, JPL) Geometry Information: Boris Semenov (PDS-NAIF, JPL), Nicolas Thomas (Max Plank Institut fur Aeronomie, Katlenburg-Lindau, Germany), and John Wellman (JPL) MPF Project Support: Kathleen Spellman, Susan Merrill, and Susan Roberts (JPL) Calibration Information: Haraldur Gunnlaugsson (Niels Bohr Institute for Astronomy, Copenhagen, Denmark), Devon Crowe and Bob Reid (Lunar & Planetary Laboratory, University of Arizona, Tucson, Arizona), Robert Sullivan (Cornell Univeristy, Ithaca, New York) MPF Landing Site Gazetteer: Bob Kanefsky, Ted Blackmon, Carol Stoker, and Eric Zbinden (NASA Ames, Moffett Field, California) and Nathan Bridges and Albert Haldemann (JPL) Mars Pathfinder IMP Image Browser: The image browser used on this CD was based largely on the HTML browser developed for the Viking Lander EDR archive CD-ROMs, which were produced by Edward A. Guinness, Thomas C. Stein, and Jennifer Herron of Washington University, St. Louis, MO. CD Reviewers: Thanks to Ed Guinness (PDS-GEO, Washington University, St. Louis, Missouri), Bob Reid (Lunar & Planetary Laboratory, University of Arizona, Tucson, Arizona), and Betty Sword (PDS-CN, JPL) for their helpful comments on this set of CDs.
C TABLE LABELS
The INDEX.LBL file describes the structure of the INDEX.TAB file, which contains a selected set of parameters describing each EDR image file on the CD volume. The CUMINDEX.LBL and CUMINDEX.TAB files are very similar to these, except that they contain all the IMP images from all three volumes.
PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 409 FILE_RECORDS = 4661 DESCRIPTION = "INDEX.TAB lists all the IMP EDR image files on this volume, along with a selected set of parameters describing them." ^INDEX_TABLE = "INDEX.TAB" DATA_SET_ID = "MPFL-M-IMP-2-EDR-V1.0" MISSION_NAME = "MARS PATHFINDER" INSTRUMENT_HOST_NAME = "MARS PATHFINDER LANDER" INSTRUMENT_NAME = "IMAGER FOR MARS PATHFINDER" OBJECT = INDEX_TABLE INTERCHANGE_FORMAT = ASCII ROW_BYTES = 409 ROWS = 4661 COLUMNS = 24 INDEX_TYPE = SINGLE INDEXED_FILE_NAME = {"*.DRK","*.FLT","*.HST","*.IMG", "*.NUL","*.STR","*.SUM"} OBJECT = COLUMN NAME = PRODUCT_ID DATA_TYPE = CHARACTER START_BYTE = 2 BYTES = 42 DESCRIPTION = "A permanent, unique identifier assigned to each data product. For the IMP EDRs, this is constructed from the words 'IMP_EDR' followed by the spacecraft clock start count, followed by the image observation type, followed by the image id." END_OBJECT = COLUMN OBJECT = COLUMN NAME = VOLUME_ID DATA_TYPE = CHARACTER START_BYTE = 47 BYTES = 9 DESCRIPTION = "Identifies the CD volume containing the named file. For the IMP EDRs, this consists of the identifier 'MPIM_' followed by the four digit volume number." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PATH_NAME DATA_TYPE = CHARACTER START_BYTE = 59 BYTES = 26 DESCRIPTION = "Path to directory containing file. This path is shown in UNIX format. It begins at the root level of the CD. It has a trailing slah, but no leading slash." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILE_NAME DATA_TYPE = CHARACTER START_BYTE = 88 BYTES = 12 DESCRIPTION = "This is the name of the PDS formatted file as it is stored on the CD-ROM archive media. For the IMP EDRs, it consists of the instrument identifier 'I', followed by the six least significant digits of the spacecraft clock start count, followed by a frame identifier (L=left, R=right, S=dark strip, N=null strip), followed by a 3 character extension. The extension indicates the image observation type as follows: IMG=regular, STR=dark strip, NUL=null strip, FLT=flat field, DRK=dark current, HST=histogram, and SUM=summation. (Note that the latter two values were never used.)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SPACECRAFT_CLOCK_START_COUNT DATA_TYPE = ASCII_INTEGER START_BYTE = 102 BYTES = 10 DESCRIPTION = "The value of the lander clock (in seconds) at which the image was acquired." END_OBJECT = COLUMN OBJECT = COLUMN NAME = IMAGE_OBSERVATION_TYPE DATA_TYPE = CHARACTER START_BYTE = 114 BYTES = 12 DESCRIPTION = "Identifies the type or purpose of an observation. Valid values are REGULAR, DARK_CURRENT, FLAT_FIELD, HISTOGRAM, SUMMATION, DARK_STRIP, and NULL_STRIP. For the meanings of these values, please see appendix A of the IMP EDR CD-ROM SIS." END_OBJECT = COLUMN OBJECT = COLUMN NAME = COMMAND_SEQUENCE_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 128 BYTES = 4 DESCRIPTION = "Identifies a set of commands sent to the IMP camera, ordering it to perform a particular task. Valid range is 1 to 9999. For a complete list of the command sequence numbers used during the mission and their descriptions, see section 3.2.2.7 of the IMP EDR CD-ROM SIS." END_OBJECT = COLUMN OBJECT = COLUMN NAME = IMAGE_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 133 BYTES = 10 DESCRIPTION = "Uniquely identifies the observation parameters of an image. The most significant four digits identify the command sequence that contains the imaging command. The middle two digits indicate the version of the command sequence, and the right four digits identify the image within a single imaging sequence." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FRAME_ID DATA_TYPE = CHARACTER START_BYTE = 145 BYTES = 9 DESCRIPTION = "Provides an identification for a particular instrument frame. Valid values are LEFT, RIGHT, BOTH, and HALFL. The IMP camera nominally operates in a mode where both the left and right images are exposed and transferred into the frame buffer simultaneously. Then either the RIGHT, LEFT, or BOTH frames are transmitted. For even shorter shutter times, the left image only may be transferred into the frame buffer (HALFL). The presence of BOTH in this field indicates that the image should be part of a stereo pair." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_DEPLOYMENT_STATE DATA_TYPE = CHARACTER START_BYTE = 157 BYTES = 8 DESCRIPTION = "Indicates whether or not the IMP camera had been deployed to the end of its mast. Valid values are STOWED and DEPLOYED." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILTER_NAME DATA_TYPE = CHARACTER START_BYTE = 168 BYTES = 14 DESCRIPTION = "The name of the instrument filter through which the image was acquired. The numbers refer to the effective wavelength in nm of the filter for the left (L) or right (R) image. FILTER FILTER NUMBER NAME APPLICATION ----------------------------------------------- 0 L440_R440 Stereo, Geology 1 L450_R670 Solar 2 L885_R947 Solar 3 L925_R935 Solar 4 L935_R990 Solar 5 L670_R670 Stereo, Geology 6 L800_R750 Geology 7 L860_R-DIOPTER Geology 8 L900_R600 Geology 9 L930_R530 Stereo, Ranging, Geology 10 L1000_R480 Geology 11 L965_R965 Stereo, Ranging, Geology " END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILTER_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 184 BYTES = 2 DESCRIPTION = "The number of the instrument filter through which the image was acquired. (See FILTER_NAME for details.)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = IMAGE_TIME DATA_TYPE = TIME START_BYTE = 187 BYTES = 24 DESCRIPTION = "Date and time at which the image was acquired, recorded in UTC system format. Shown as YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = PRODUCT_CREATION_TIME DATA_TYPE = TIME START_BYTE = 212 BYTES = 24 DESCRIPTION = "Defines the UTC time a product was created or last modified. Has the form YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = EARTH_RECEIVED_START_TIME DATA_TYPE = TIME START_BYTE = 237 BYTES = 24 DESCRIPTION = "Identifies the earliest time that a telemetry packet containing data for the image was received. Has the form YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = EARTH_RECEIVED_STOP_TIME DATA_TYPE = TIME START_BYTE = 262 BYTES = 24 DESCRIPTION = "Identifies the latest time that a telemetry packet containing data for the image was received. Has the form YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = PLANET_DAY_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 287 BYTES = 4 DESCRIPTION = "The Martian day (ie., sidereal day, equal to a rotation of 360 degrees) on which the image was taken. Starts with 1 as the first day of surface operations, the day the spacecraft landed. Negative values refer to pre-surface images." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MPF_LOCAL_TIME DATA_TYPE = CHARACTER START_BYTE = 293 BYTES = 8 DESCRIPTION = "Local time at the lander site on the surface of Mars, measured in local hours, minutes, and seconds, from midnight. Local hours are defined as one twenty-fourth of a local solar day. Local minutes are one sixtieth of a local hour, and local seconds are one sixtieth of a local minute. Format is hh:mm:ss. Based on the IAU standard for the Martian prime meridian. See [DAVIESETAL1994] for more details." END_OBJECT = COLUMN OBJECT = COLUMN NAME = TARGET_NAME DATA_TYPE = CHARACTER START_BYTE = 304 BYTES = 8 DESCRIPTION = "Identifies the intended target of an observation. Can be either a planetary body or a physical object. The following is the list of targets imaged by the IMP: APXSSITE, ALTAIR, ARCTURUS, CALIMG, DEIMOS, LANDER, MAG, MARS, PHOBOS, ROVER, SKY, SUN, VEGA, WINDSOCKS " END_OBJECT = COLUMN OBJECT = COLUMN NAME = AZIMUTH_MOTOR_CLICKS DATA_TYPE = ASCII_INTEGER START_BYTE = 314 BYTES = 4 DESCRIPTION = "The number of motor step counts the camera rotated in the horizontal direction from the low hard stop. Since each step count is 0.553 degrees, the azimuthal position of the camera can be derived from this value. Valid range is 0 to 1023." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ELEVATION_MOTOR_CLICKS DATA_TYPE = ASCII_INTEGER START_BYTE = 319 BYTES = 4 DESCRIPTION = "The number of motor step counts the camera rotated in the vertical direction from the low hard stop. Since each step count is 0.553 degrees, the elevational position of the camera can be derived from this value. Valid range is 0 to 1023." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SURFACE_BASED_INST_AZIMUTH DATA_TYPE = ASCII_REAL START_BYTE = 324 BYTES = 8 DESCRIPTION = "One of two angular measurements of the pointing direction of the instrument. The azimuth is measured positively in the clockwise direction (as viewed from above) with the meridian passing through the positive spin axis ('north pole') defining the zero reference. The angle is measured in the local gravity horizontal plane, ie., a plane perpendicular to the local gravity vector." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SURFACE_BASED_INST_ELEVATION DATA_TYPE = ASCII_REAL START_BYTE = 333 BYTES = 8 DESCRIPTION = "One of two angular measurements of the pointing direction of the instrument. For the Mars Pathfinder IMP EDRs, elevation is measured positively upwards from the plane which is perpendicular to the local gravity vector and which intersects the elevation axis around with the camera rotates. Valid values: -90 degrees (nadir) to +90 degrees (zenith)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = OBSERVATION_NAME DATA_TYPE = CHARACTER START_BYTE = 343 BYTES = 64 DESCRIPTION = "The intended purpose of an observation or sequence of commands. See table 3.2.2.7.B in the IMP EDR CD-ROM SIS for a complete listing of the values." END_OBJECT = COLUMN END_OBJECT = INDEX_TABLE END
C.2 COMMAND.LBL
The COMMAND.LBL file describes the structure of the COMMAND.TAB file, which contains descriptive parameters describing each command, or IMAGE_ID, used to command the IMP camera. The IMAGE_IDs can be used as a common key with the EDRINDEX.TAB file to create a relational database.
PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 469 FILE_RECORDS = 7223 DESCRIPTION = "COMMAND.TAB provides a detailed description of the commands used on the Mars Pathfinder mission. Note that these are the values that were commanded, and may in some instances differ from the values that were actually used, which are shown in the EDRINDEX.TAB file. The records in this table are keyed on the IMAGE_ID, which represents an individual command with a set of unique command parameters. Each command usually produced multiple images." ^TABLE = "COMMAND.TAB" DATA_SET_ID = "MPFL-M-IMP-2-EDR-V1.0" MISSION_NAME = "MARS PATHFINDER" INSTRUMENT_HOST_NAME = "MARS PATHFINDER LANDER" INSTRUMENT_NAME = "IMAGER FOR MARS PATHFINDER" OBJECT = TABLE INTERCHANGE_FORMAT = ASCII ROW_BYTES = 469 ROWS = 7223 COLUMNS = 43 OBJECT = COLUMN NAME = IMAGE_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 1 BYTES = 10 FORMAT = "I10" DESCRIPTION = "Uniquely identifies the observation parameters of an image. The most significant four digits identify the command sequence that contains the imaging command. The middle two digits indicate the version of the command sequence, and the right four digits identify the image within a single imaging sequence." END_OBJECT = COLUMN OBJECT = COLUMN NAME = COMMAND_VERSION_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 12 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The version number of the command. The commands (ie., IMAGE_IDs) were intended to be unique, but in a few cases they were re-used with different command parameters. This keyword was added to distinguish between differing versions of the commands. Valid range is 1 to 9, where the lowest version number reflects the oldest version of a command." END_OBJECT = COLUMN OBJECT = COLUMN NAME = APPLICATION_PACKET_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 14 BYTES = 2 FORMAT = "I2" DESCRIPTION = "The id of the telemetry packet queue to which the image data was directed." END_OBJECT = COLUMN OBJECT = COLUMN NAME = AUTO_EXPOSURE_DATA_CUT DATA_TYPE = ASCII_INTEGER START_BYTE = 17 BYTES = 4 FORMAT = "I4" DESCRIPTION = "The DN value which a specified fraction of pixels is permitted to exceed. Valid range: 0 to 4095." END_OBJECT = COLUMN OBJECT = COLUMN NAME = AUTO_EXPOSURE_PIXEL_FRACTION DATA_TYPE = ASCII_REAL START_BYTE = 22 BYTES = 6 FORMAT = "F6.2" DESCRIPTION = "The percentage of pixels whose value is higher than the auto exposure data cut. This field isonly applicable if the exposure type is set to AUTO or INCREMENTAL. Valid range: 0 to 100." END_OBJECT = COLUMN OBJECT = COLUMN NAME = AZIMUTH_MOTOR_CLICKS DATA_TYPE = ASCII_INTEGER START_BYTE = 29 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The number of motor step counts the camera rotated in the horizontal direction from the low hard stop. Since each step count is 0.553 degrees, the azimuthal position of the camera can be derived from this value. Valid range is 0 to 1023." END_OBJECT = COLUMN OBJECT = COLUMN NAME = BAD_PIXEL_REPLACEMENT_FLAG DATA_TYPE = CHARACTER START_BYTE = 34 BYTES = 1 FORMAT = "A1" DESCRIPTION = "Indicates whether or not bad pixel replacement processing was completed. If set to 'T' (TRUE), certain pixels in the image were replaced based on a bad pixel table. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = COMMAND_DESCRIPTION DATA_TYPE = CHARACTER START_BYTE = 38 BYTES = 94 FORMAT = "A94" DESCRIPTION = "The textual description associated with a command name." END_OBJECT = COLUMN OBJECT = COLUMN NAME = COMMAND_NAME DATA_TYPE = CHARACTER START_BYTE = 135 BYTES = 16 FORMAT = "A16" DESCRIPTION = "The name of an uplinked command sent to a spacecraft or instrument. For the IMP EDRs, this indicates the method the IMP camera was instructed to use to determine its pointing direction. Valid values: IMP_IMAGE_AZ_EL, IMP_IMAGE_LCLGRD, IMP_IMAGE_LCLVEC, IMP_IMAGE_OBJECT, IMP_IMAGE_VECTOR." END_OBJECT = COLUMN OBJECT = COLUMN NAME = DARK_CURRENT_CORRECTION_FLAG DATA_TYPE = CHARACTER START_BYTE = 154 BYTES = 1 FORMAT = "A1" DESCRIPTION = "A flag indicating whether or not a dark current correction was applied to the image. For MPF, this correction was applied to the image on board the spacecraft, before the image was transmitted to Earth. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = DOWNLOAD_TYPE DATA_TYPE = CHARACTER START_BYTE = 158 BYTES = 6 FORMAT = "A6" DESCRIPTION = "Specifies which image data to download, any or all of: image data (IM), dark current strip (DS), and null pixel data (NS). Valid values: NONE, DS, IM, DSIM, NS, DSNS, IMNS, DSIMNS." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ELEVATION_MOTOR_CLICKS DATA_TYPE = ASCII_INTEGER START_BYTE = 166 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The number of motor step counts the camera rotated in the vertical direction from the low hard stop. Since each step count is 0.553 degrees, the elevational position of the camera can be derived from this value. Valid range is 0 to 1023." END_OBJECT = COLUMN OBJECT = COLUMN NAME = EXPOSURE_COUNT DATA_TYPE = ASCII_INTEGER START_BYTE = 170 BYTES = 1 FORMAT = "I1" DESCRIPTION = "Maximum number of exposures taken. Value is dependant on exposure type. Valid range: 0 - 16." END_OBJECT = COLUMN OBJECT = COLUMN NAME = EXPOSURE_DURATION DATA_TYPE = ASCII_REAL START_BYTE = 172 BYTES = 7 FORMAT = "F7.1" DESCRIPTION = "The commanded integration time for MANUAL and AUTO exposures, measured in milliseconds." END_OBJECT = COLUMN OBJECT = COLUMN NAME = EXPOSURE_TYPE DATA_TYPE = CHARACTER START_BYTE = 181 BYTES = 6 FORMAT = "A6" DESCRIPTION = "Exposure type for the image. Valid values: AUTO, INCR (incremental), MANUAL, PRETMD (pretimed), and NONE. AUTO exposure automatically adjusts the exposure time by iterating off of a pre-set exposure time. INCR exposure also automatically adjusts the exposure time, but iterates off of the exposure time from the previous image. MANUAL exposure is a single exposure with a set exposure time. PRETMD exposure uses the last exposure time used, regardless of the type of exposure it was. NONE indicates that the command moves only the camera and doesn't take an exposure." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILTER_NAME DATA_TYPE = CHARACTER START_BYTE = 190 BYTES = 14 FORMAT = "A14" DESCRIPTION = "The name of the instrument filter through which the image was acquired. The numbers refer to the effective wavelength in nm of the filter for the left (L) or right (R) image. FILTER FILTER NUMBER NAME APPLICATION ----------------------------------------------- 0 L440_R440 Stereo, Geology 1 L450_R670 Solar 2 L885_R947 Solar 3 L925_R935 Solar 4 L935_R990 Solar 5 L670_R670 Stereo, Geology 6 L800_R750 Geology 7 L860_R-DIOPTER Geology 8 L900_R600 Geology 9 L930_R530 Stereo, Ranging, Geology 10 L1000_R480 Geology 11 L965_R965 Stereo, Ranging, Geology " END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILTER_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 206 BYTES = 2 FORMAT = "I2" DESCRIPTION = "The number of the instrument filter through which the image was acquired. (See FILTER_NAME for details.)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = FIRST_LINE DATA_TYPE = ASCII_INTEGER START_BYTE = 209 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The line within a source image that corresponds to the first line in the sub-image. For the IMP EDRs, the source image is the complete 256x256 image area within the CCD." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FIRST_LINE_SAMPLE DATA_TYPE = ASCII_INTEGER START_BYTE = 213 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The sample within a source image that corresponds to the first sample in the sub-image. For the IMP EDRs, the source image is the complete 256x256 image area within the CCD." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FLAT_FIELD_CORRECTION_FLAG DATA_TYPE = CHARACTER START_BYTE = 218 BYTES = 1 FORMAT = "A1" DESCRIPTION = "Indicates whether or not a flat field correction was applied to the image. For MPF, this correction was applied to the image on board the spacecraft, before the image was transmitted to Earth. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FRAME_ID DATA_TYPE = CHARACTER START_BYTE = 222 BYTES = 5 FORMAT = "A5" DESCRIPTION = "Provides an identification for a particular instrument frame. Valid values are LEFT, RIGHT, BOTH, and HALFL. The IMP camera nominally operates in a mode where both the left and right images are exposed and transferred into the frame buffer simultaneously. Then either the RIGHT, LEFT, or BOTH frames are transmitted. For even shorter shutter times, the left image only may be transferred into the frame buffer (HALFL). The presence of BOTH in this field indicates that the image should be part of a stereo pair." END_OBJECT = COLUMN OBJECT = COLUMN NAME = GRID_POSITION_X DATA_TYPE = ASCII_REAL START_BYTE = 229 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "The north / south component of a positon defining the IMP pointing, measured with respect to the Martian Local Level Coordinate Frame (M Frame). A positive value indicates that the position was to the north of the lander; a negative value indicates it was to the south. The magnitude gives the distance, in meters, between the position and an east / west line drawn through the center of the lander base petal." END_OBJECT = COLUMN OBJECT = COLUMN NAME = GRID_POSITION_Y DATA_TYPE = ASCII_REAL START_BYTE = 238 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "The east / west component of a positon defining the IMP pointing, measured with respect to the Martian Local Level Coordinate Frame (M Frame). A positive value indicates that the position was to the east of the lander; a negative value indicates it was to the west. The magnitude gives the distance, in meters, between the position and an north / south line drawn through the center of the lander base petal." END_OBJECT = COLUMN OBJECT = COLUMN NAME = GRID_POSITION_Z DATA_TYPE = ASCII_REAL START_BYTE = 247 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "The vertical component of a position defining the IMP pointing, measured with respect to the Martian Local Level Coordinate Frame (M Frame). A positive value indicates that the position was below the lander base petal; a negative value indicates that it was above the base petal." END_OBJECT = COLUMN OBJECT = COLUMN NAME = HISTOGRAM_FLAG DATA_TYPE = CHARACTER START_BYTE = 256 BYTES = 1 FORMAT = "A1" DESCRIPTION = "A flag to indicate that the product returned was a histogram. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_MODE DATA_TYPE = ASCII_INTEGER START_BYTE = 259 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The targetted image quality or compression factor for on-board compression. Compression is obtained with Huffman or arithmetic entropy encoding, with or without LCT. Odd modes specify a targetted image quality, whereas even modes specify a targetted compression factor. Modes 1,2,5,6 utilize Huffman encoding; modes 3,4,7,8 use arithmetic encoding. Modes 5,6,7,8 use LCT. Mode 9 specifies RICE compression. Valid values: 1 to 9." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_NAME DATA_TYPE = CHARACTER START_BYTE = 262 BYTES = 60 FORMAT = "A60" DESCRIPTION = "The type of on-board compression used for data storage and transmission." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_PARAM DATA_TYPE = ASCII_INTEGER START_BYTE = 324 BYTES = 2 FORMAT = "I2" DESCRIPTION = "This is a JPEG compression specific variable. It specifies the on-board compression rate as image quality or compression factor, based on the selected instrument compression mode." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_QUANTZ_TBL_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 327 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The identifier for the reference table used for quantization in the frequency domain for on-board transform compression. This name or code should be specific enough to allow the user of the data to have sufficient information to reference the quantization table used to compress the data." END_OBJECT = COLUMN OBJECT = COLUMN NAME = IVP_TARGET_NAME DATA_TYPE = CHARACTER START_BYTE = 330 BYTES = 6 FORMAT = "A6" DESCRIPTION = "Specifies the image vector pointing object at which the IMP camera was aimed. Valid values include SUN, EARTH, PHOBOS, and NULL. Note that the camera was 'tricked' into pointing at other objects (like Deimos or stars) by directing it to point to Phobos, but redefining the position of Phobos in the sky." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LINES DATA_TYPE = ASCII_INTEGER START_BYTE = 338 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The total number of pixels along the vertical axis of an image." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LINE_SAMPLES DATA_TYPE = ASCII_INTEGER START_BYTE = 342 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The total number of pixels along the horizontal axis of an image." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PIXEL_AVERAGING_HEIGHT DATA_TYPE = ASCII_INTEGER START_BYTE = 346 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The vertical dimension, in pixels, of the area over which pixels were averaged prior to image compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PIXEL_AVERAGING_WIDTH DATA_TYPE = ASCII_INTEGER START_BYTE = 348 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The horizontal dimension, in pixels, of the area over which pixels were averaged prior to image compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SHUTTER_EFFECT_CORRECTION_FLAG DATA_TYPE = CHARACTER START_BYTE = 351 BYTES = 1 FORMAT = "A1" DESCRIPTION = "Indicates whether or not a shutter effect correction was applied to the image. The shutter effect correction involves the removal from the image of the shutter or fixed-pattern. For MPF, this correction was applied to the image on board the spacecraft, before the image was transmitted to Earth. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SOURCE_PRODUCT_ID DATA_TYPE = CHARACTER START_BYTE = 355 BYTES = 16 FORMAT = "A16" DESCRIPTION = "Identifies a product used as input to create a new product. For MPF, this refers to the filenames of the SPICE kernels used to produce the image and its ancillary data." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SQRT_COMPRESSION_FLAG DATA_TYPE = CHARACTER START_BYTE = 374 BYTES = 1 FORMAT = "A1" DESCRIPTION = "Indicates whether or not square root compression was applied to the image. For MPF, this compression was performed on-board the lander, prior to transmission of the data to Earth. It involved the compression of the pixels from 12 bits down to 8 bits. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SUBFRAME_FLAG DATA_TYPE = CHARACTER START_BYTE = 378 BYTES = 1 FORMAT = "A1" DESCRIPTION = "A flag to indicate that the image is not full size. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SUM_FLAG DATA_TYPE = CHARACTER START_BYTE = 382 BYTES = 1 FORMAT = "A1" DESCRIPTION = "A flag to indicate that the product returned is a 'summation' file. For the IMP EDRs, this means that it contains two records, the first a list of the sums of the image columns, and the second a list of the sums of the image rows. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ATMOS_FLAG DATA_TYPE = CHARACTER START_BYTE = 386 BYTES = 1 FORMAT = "A1" DESCRIPTION = "A flag that indicates that the given observation was directed at the sun. Valid values: T, F." END_OBJECT = COLUMN OBJECT = COLUMN NAME = OBSERVATION_NAME DATA_TYPE = CHARACTER START_BYTE = 390 BYTES = 56 FORMAT = "A56" DESCRIPTION = "The intended purpose of an observation or sequence of commands. See table 3.2.2.7.B in the IMP EDR CD-ROM SIS for a complete listing of the values." END_OBJECT = COLUMN OBJECT = COLUMN NAME = VECTOR_COMPONENT_X DATA_TYPE = ASCII_REAL START_BYTE = 448 BYTES = 6 FORMAT = "F6.3" DESCRIPTION = "The x component of a unit vector which defines the IMP pointing. The vector is defined with respect to one of two possible coordinate frames, indicated by the command name. If the command name is IMP_IMAGE_VECTOR, the coordinate system is the IMP camera frame (IMP Frmae); if the command name is IMP_IMAGE_LCLVEC, the coordinate system is the Martian Local Level Frame (M Frame). Valid range: -1.0 to 1.0." END_OBJECT = COLUMN OBJECT = COLUMN NAME = VECTOR_COMPONENT_Y DATA_TYPE = ASCII_REAL START_BYTE = 455 BYTES = 6 FORMAT = "F6.3" DESCRIPTION = "The y component of a unit vector which defines the IMP pointing. The vector is defined with respect to one of two possible coordinate frames, indicated by the command name. If the command name is IMP_IMAGE_VECTOR, the coordinate system is the IMP camera frame (IMP Frmae); if the command name is IMP_IMAGE_LCLVEC, the coordinate system is the Martian Local Level Frame (M Frame). Valid range: -1.0 to 1.0." END_OBJECT = COLUMN OBJECT = COLUMN NAME = VECTOR_COMPONENT_Z DATA_TYPE = ASCII_REAL START_BYTE = 462 BYTES = 6 FORMAT = "F6.3" DESCRIPTION = "The z component of a unit vector which defines the IMP pointing. The vector is defined with respect to one of two possible coordinate frames, indicated by the command name. If the command name is IMP_IMAGE_VECTOR, the coordinate system is the IMP camera frame (IMP Frmae); if the command name is IMP_IMAGE_LCLVEC, the coordinate system is the Martian Local Level Frame (M Frame). Valid range: -1.0 to 1.0." END_OBJECT = COLUMN END_OBJECT = TABLE END
C.3 EDRINDEX.LBL
The EDRINDEX.LBL file describes the structure of the EDRINDEX.TAB file, which contains a detailed listing of many parameters describing each EDR image. The only parameters which were used during the mission which have not been included here are those specifically pertaining to active mission operations.
PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 777 FILE_RECORDS = 16661 DESCRIPTION = "EDRINDEX.TAB lists all IMP EDR image files on this set of 3 CD volumes. It includes most of the parameters from the project database except those that were applicable only to mission operations." ^INDEX_TABLE = "EDRINDEX.TAB" DATA_SET_ID = "MPFL-M-IMP-2-EDR-V1.0" MISSION_NAME = "MARS PATHFINDER" INSTRUMENT_HOST_NAME = "MARS PATHFINDER LANDER" INSTRUMENT_NAME = "IMAGER FOR MARS PATHFINDER" OBJECT = INDEX_TABLE INTERCHANGE_FORMAT = ASCII ROW_BYTES = 777 ROWS = 16661 COLUMNS = 63 INDEX_TYPE = CUMULATIVE INDEXED_FILE_NAME = {"*.DRK","*.FLT","*.HST","*.IMG", "*.NUL","*.STR","*.SUM"} OBJECT = COLUMN NAME = SPACECRAFT_CLOCK_START_COUNT DATA_TYPE = ASCII_INTEGER START_BYTE = 1 BYTES = 10 FORMAT = "I10" DESCRIPTION = "The value of the lander clock (in seconds) at which the image was acquired." END_OBJECT = COLUMN OBJECT = COLUMN NAME = IMAGE_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 12 BYTES = 10 FORMAT = "I10" DESCRIPTION = "Uniquely identifies the observation parameters of an image. The most significant four digits identify the command sequence that contains the imaging command. The middle two digits indicate the version of the command sequence, and the right four digits identify the image within a single imaging sequence." END_OBJECT = COLUMN OBJECT = COLUMN NAME = IMAGE_OBSERVATION_TYPE DATA_TYPE = CHARACTER START_BYTE = 24 BYTES = 12 FORMAT = "A12" DESCRIPTION = "Identifies the type or purpose of an observation. Valid values are REGULAR, DARK_CURRENT, FLAT_FIELD, HISTOGRAM, SUMMATION, DARK_STRIP, and NULL_STRIP. For the meanings of these values, please see appendix A of the IMP EDR CD-ROM SIS." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PRODUCT_ID DATA_TYPE = CHARACTER START_BYTE = 39 BYTES = 42 FORMAT = "A42" DESCRIPTION = "A permanent, unique identifier assigned to each data product. For the IMP EDRs, this is constructed from the words 'IMP_EDR' followed by the spacecraft clock start count, followed by the image observation type, followed by the image id." END_OBJECT = COLUMN OBJECT = COLUMN NAME = VOLUME_ID DATA_TYPE = CHARACTER START_BYTE = 84 BYTES = 9 FORMAT = "A9" DESCRIPTION = "Identifies the CD volume containing the named file. For the IMP EDRs, this consists of the identifier 'MPIM_' followed by the four digit volume number." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PATH_NAME DATA_TYPE = CHARACTER START_BYTE = 96 BYTES = 26 FORMAT = "A26" DESCRIPTION = "Path to directory containing file. This path is shown in UNIX format. It begins at the root level of the CD. It has a trailing slah, but no leading slash." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILE_NAME DATA_TYPE = CHARACTER START_BYTE = 125 BYTES = 12 FORMAT = "A12" DESCRIPTION = "This is the name of the PDS formatted file as it is stored on the CD-ROM archive media. For the IMP EDRs, it consists of the instrument identifier 'I', followed by the six least significant digits of the spacecraft clock start count, followed by a frame identifier (L=left, R=right, S=dark strip, N=null strip), followed by a 3 character extension. The extension indicates the image observation type as follows: IMG=regular, STR=dark strip, NUL=null strip, FLT=flat field, DRK=dark current, HST=histogram, and SUM=summation. (Note that the latter two values were never used.)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = APPLICATION_PACKET_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 139 BYTES = 2 FORMAT = "I2" DESCRIPTION = "The id of the telemetry packet queue to which the image data was directed." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_AZIMUTH DATA_TYPE = ASCII_REAL START_BYTE = 142 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "One of two angular measurements of the pointing direction of the instrument. The azimuth is measured positively in the clockwise direction (as viewed from above) from a fixed reference direction. The angle is measured in the x-y plane of the instrument's coordinate system, which is not necessarily co-linear with the surface fixed coordinate system." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_AZIMUTH_METHOD DATA_TYPE = CHARACTER START_BYTE = 152 BYTES = 9 FORMAT = "A9" DESCRIPTION = "Identifies the method used to calculate the instrument azimuth from the azimuth motor clicks. Valid values: TELEMETRY, MPFNAV-MIPS, BACKLASH-UOFA." END_OBJECT = COLUMN OBJECT = COLUMN NAME = AZIMUTH_FOV DATA_TYPE = ASCII_REAL START_BYTE = 163 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "The angular measure of the horizontal field of view of an imaged scene. For MPF, 'horizontal' is measured in the x-y plane of the IMP coordinate system." END_OBJECT = COLUMN OBJECT = COLUMN NAME = AZIMUTH_MOTOR_CLICKS DATA_TYPE = ASCII_INTEGER START_BYTE = 171 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The number of motor step counts the camera rotated in the horizontal direction from the low hard stop. Since each step count is 0.553 degrees, the azimuthal position of the camera can be derived from this value. Valid range is 0 to 1023." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_ELEVATION DATA_TYPE = ASCII_REAL START_BYTE = 175 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "One of two angular measurements of the pointing direction of the instrument. The elevation is measured with respect to the plane which is co-planar with the x-y plane of the instrument's coordinate system (in this case the IMP Frame) and which intersects the elevation axis around which the instrument rotates. For the Mars Pathfinder IMP EDRs, the elevation is measured positive upwards. Valid values: -90 degrees (nadir) to +90 degrees (zenith)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_ELEVATION_METHOD DATA_TYPE = CHARACTER START_BYTE = 185 BYTES = 9 FORMAT = "A9" DESCRIPTION = "Identifies the method used to calculate the instrument elevation from the elevation motor clicks. Valid values: TELEMETRY, MPFNAV-MIPS, BACKLASH-UOFA." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ELEVATION_FOV DATA_TYPE = ASCII_REAL START_BYTE = 196 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "The angular measure of the vertical field of view of an imaged scene. For MPF, 'vertical' is measured along the Z-IMP axis of the IMP coordinate system." END_OBJECT = COLUMN OBJECT = COLUMN NAME = ELEVATION_MOTOR_CLICKS DATA_TYPE = ASCII_INTEGER START_BYTE = 204 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The number of motor step counts the camera rotated in the vertical direction from the low hard stop. Since each step count is 0.553 degrees, the elevational position of the camera can be derived from this value. Valid range is 0 to 1023." END_OBJECT = COLUMN OBJECT = COLUMN NAME = EXPECTED_PACKETS DATA_TYPE = ASCII_INTEGER START_BYTE = 208 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The total number of telemetry packets which constitute a complete image, ie., an image without missing data." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RECEIVED_PACKETS DATA_TYPE = ASCII_INTEGER START_BYTE = 212 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The total number of telemetry packets which constitute a reconstructed image." END_OBJECT = COLUMN OBJECT = COLUMN NAME = EXPOSURE_DURATION DATA_TYPE = ASCII_REAL START_BYTE = 216 BYTES = 7 FORMAT = "F7.1" DESCRIPTION = "The integration time for MANUAL and AUTO exposures, measured in milliseconds." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILTER_NAME DATA_TYPE = CHARACTER START_BYTE = 225 BYTES = 14 FORMAT = "A14" DESCRIPTION = "The name of the instrument filter through which the image was acquired. The numbers refer to the effective wavelength in nm of the filter for the left (L) or right (R) image. FILTER FILTER NUMBER NAME APPLICATION ----------------------------------------------- 0 L440_R440 Stereo, Geology 1 L450_R670 Solar 2 L885_R947 Solar 3 L925_R935 Solar 4 L935_R990 Solar 5 L670_R670 Stereo, Geology 6 L800_R750 Geology 7 L860_R-DIOPTER Geology 8 L900_R600 Geology 9 L930_R530 Stereo, Ranging, Geology 10 L1000_R480 Geology 11 L965_R965 Stereo, Ranging, Geology " END_OBJECT = COLUMN OBJECT = COLUMN NAME = FILTER_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 241 BYTES = 2 FORMAT = "I2" DESCRIPTION = "The number of the instrument filter through which the image was acquired. (See FILTER_NAME for details.)" END_OBJECT = COLUMN OBJECT = COLUMN NAME = COMMAND_SEQUENCE_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 244 BYTES = 4 FORMAT = "I4" DESCRIPTION = "Identifies a set of commands sent to the IMP camera, ordering it to perform a particular task. Valid range is 1 to 9999. For a complete list of the command sequence numbers used during the mission and their descriptions, see section 3.2.2.7 of the IMP EDR CD-ROM SIS." END_OBJECT = COLUMN OBJECT = COLUMN NAME = IMAGE_TIME DATA_TYPE = TIME START_BYTE = 249 BYTES = 24 FORMAT = "A24" DESCRIPTION = "Date and time at which the image was acquired, recorded in UTC system format. Shown as YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_BLK_SIZE DATA_TYPE = ASCII_INTEGER START_BYTE = 274 BYTES = 3 FORMAT = "I3" DESCRIPTION = "Dimension of a block for on-board compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_BLOCKS DATA_TYPE = ASCII_INTEGER START_BYTE = 278 BYTES = 4 FORMAT = "I4" DESCRIPTION = "Number of blocks used to spatially segment the image file prior to compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_MODE DATA_TYPE = ASCII_INTEGER START_BYTE = 283 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The targetted image quality or compression factor for on-board compression. Compression is obtained with Huffman or arithmetic entropy encoding, with or without LCT. Odd modes specify a targetted image quality, whereas even modes specify a targetted compression factor. Modes 1,2,5,6 utilize Huffman encoding; modes 3,4,7,8 use arithmetic encoding. Modes 5,6,7,8 use LCT. Mode 9 specifies RICE compression. Valid values: 1 to 9." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_NAME DATA_TYPE = CHARACTER START_BYTE = 286 BYTES = 60 FORMAT = "A60" DESCRIPTION = "The type of on-board compression used for data storage and transmission." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_PARAM DATA_TYPE = ASCII_INTEGER START_BYTE = 348 BYTES = 3 FORMAT = "I3" DESCRIPTION = "This is a JPEG compression specific variable. It specifies the on-board copmression rate as image quality or compression factor, based on the selected instrument compression mode." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_QUANTZ_TBL_ID DATA_TYPE = ASCII_INTEGER START_BYTE = 352 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The identifier for the reference table used for quantization in the frequency domain for on-board transform compression. This name or code should be specific enough to allow the user of the data to have sufficient information to reference the quantization table used to compress the data." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_QUALITY DATA_TYPE = ASCII_INTEGER START_BYTE = 356 BYTES = 3 FORMAT = "I3" DESCRIPTION = "A JPEG specific variable. If an odd IMP compression mode is used for on-board compression, this is the desired image quality index. If an even IMP compression mode is used, this is the resultant image quality used to reach a desired on-board compression factor." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_RATE DATA_TYPE = ASCII_REAL START_BYTE = 360 BYTES = 6 FORMAT = "F6.3" DESCRIPTION = "The average number of bits needed to represent a pixel for an ob-board compressed image." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_RATIO DATA_TYPE = ASCII_REAL START_BYTE = 367 BYTES = 8 FORMAT = "F8.2" DESCRIPTION = "The ratio of the size, in bytes, of the original uncompressed data file to its compressed form." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INST_CMPRS_SYNC_BLKS DATA_TYPE = ASCII_INTEGER START_BYTE = 376 BYTES = 4 FORMAT = "I4" DESCRIPTION = "A RICE specific variable. The number of compressed blocks between synchronization counters." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_DEPLOYMENT_STATE DATA_TYPE = CHARACTER START_BYTE = 382 BYTES = 8 FORMAT = "A8" DESCRIPTION = "Indicates whether or not the IMP camera had been deployed to the end of its mast. Valid values are STOWED and DEPLOYED." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_CCD_TEMPERATURE DATA_TYPE = ASCII_REAL START_BYTE = 392 BYTES = 5 FORMAT = "F5.1" DESCRIPTION = "The temperature, in degrees Celcius, of the CCD sensor array when the image was acquired." END_OBJECT = COLUMN OBJECT = COLUMN NAME = INSTRUMENT_HEAD_TEMPERATURE DATA_TYPE = ASCII_REAL START_BYTE = 398 BYTES = 5 FORMAT = "F5.1" DESCRIPTION = "The temperature, in degrees Celcius, of the camera head when the image was acquired." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LINES DATA_TYPE = ASCII_INTEGER START_BYTE = 404 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The total number of pixels along the vertical axis of an image." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LINE_SAMPLES DATA_TYPE = ASCII_INTEGER START_BYTE = 408 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The total number of pixels along the horizontal axis of an image." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LANDER_SURFACE_QUATERNION_X DATA_TYPE = ASCII_REAL START_BYTE = 412 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "One of four values that define the relationship between the lander coordinate frame and the local level coordinate frame." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LANDER_SURFACE_QUATERNION_Y DATA_TYPE = ASCII_REAL START_BYTE = 420 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "One of four values that define the relationship between the lander coordinate frame and the local level coordinate frame." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LANDER_SURFACE_QUATERNION_Z DATA_TYPE = ASCII_REAL START_BYTE = 428 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "One of four values that define the relationship between the lander coordinate frame and the local level coordinate frame." END_OBJECT = COLUMN OBJECT = COLUMN NAME = LANDER_SURFACE_QUATERNION_A DATA_TYPE = ASCII_REAL START_BYTE = 436 BYTES = 7 FORMAT = "F7.4" DESCRIPTION = "One of four values that define the relationship between the lander coordinate frame and the local level coordinate frame." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PLANET_DAY_NUMBER DATA_TYPE = ASCII_INTEGER START_BYTE = 444 BYTES = 4 FORMAT = "I4" DESCRIPTION = "The Martian day (ie., sidereal day, equal to a rotation of 360 degrees) on which the image was taken. Starts with 1 as the first day of surface operations, the day the spacecraft landed. Negative values refer to pre-surface images." END_OBJECT = COLUMN OBJECT = COLUMN NAME = MPF_LOCAL_TIME DATA_TYPE = CHARACTER START_BYTE = 450 BYTES = 8 FORMAT = "A8" DESCRIPTION = "Local time at the lander site on the surface of Mars, measured in local hours, minutes, and seconds, from midnight. Local hours are defined as one twenty-fourth of a local solar day. Local minutes are one sixtieth of a local hour, and local seconds are one sixtieth of a local minute. Format is hh:mm:ss. Based on the IAU standard for the Martian prime meridian. See [DAVIES1994] for more details." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PACKET_MAP_MASK DATA_TYPE = CHARACTER START_BYTE = 461 BYTES = 116 FORMAT = "A116" DESCRIPTION = "A series of binary digits identifying which of the expected packets were actually received. The bits are to be read left to right. Ie., the first packet is represented by the leftmost bit." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PIXEL_AVERAGING_HEIGHT DATA_TYPE = ASCII_INTEGER START_BYTE = 579 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The vertical dimension, in pixels, of the area over which pixels were averaged prior to image compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PIXEL_AVERAGING_WIDTH DATA_TYPE = ASCII_INTEGER START_BYTE = 581 BYTES = 1 FORMAT = "I1" DESCRIPTION = "The horizontal dimension, in pixels, of the area over which pixels were averaged prior to image compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = PRODUCT_CREATION_TIME DATA_TYPE = TIME START_BYTE = 583 BYTES = 24 FORMAT = "A24" DESCRIPTION = "Defines the UTC time was a product was created or last modified. Has the form YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = RICE_OPTION_VALUE DATA_TYPE = ASCII_INTEGER START_BYTE = 608 BYTES = 3 FORMAT = "I3" DESCRIPTION = "A RICE compressor specific variable." END_OBJECT = COLUMN OBJECT = COLUMN NAME = RICE_START_OPTION DATA_TYPE = ASCII_INTEGER START_BYTE = 612 BYTES = 3 FORMAT = "I3" DESCRIPTION = "A RICE compressor specific variable." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SOFTWARE_NAME DATA_TYPE = CHARACTER START_BYTE = 617 BYTES = 16 FORMAT = "A16" DESCRIPTION = "The name of the telemetry processing software used to generate the image data." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SOFTWARE_VERSION_ID DATA_TYPE = CHARACTER START_BYTE = 636 BYTES = 8 FORMAT = "A8" DESCRIPTION = "The version of the telemetry processing software used to generate the image data." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SOLAR_AZIMUTH DATA_TYPE = ASCII_REAL START_BYTE = 646 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "One of two angular measurements indicating the position of the Sun as measured from a specific point on the surface of a planet (ex., from a lander or rover). The azimuth is measured positively in the clockwise direction (as viewed from above) with the meridian passing through the positive spin axis of the planet (ie., the north pole) defining the zero reference." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SOLAR_ELEVATION DATA_TYPE = ASCII_REAL START_BYTE = 655 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "One of two angular measurements indicating the position of the Sun as measured from a specific point on the surface of a planet (ex., from a lander or rover). The positive direction of the elevation is set by the positive_elevation_direction data element. It is measured from the plane which is perpendicular to the line passing between the observer and the planet's center and which intersects the observer." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SQRT_MAXIMUM_PIXEL DATA_TYPE = ASCII_INTEGER START_BYTE = 664 BYTES = 4 FORMAT = "I4" DESCRIPTION = "The maximum pixel value in a 12-bit image prior to square root compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SQRT_MINIMUM_PIXEL DATA_TYPE = ASCII_INTEGER START_BYTE = 669 BYTES = 3 FORMAT = "I3" DESCRIPTION = "The minimum pixel value in a 12-bit image prior to square root compression." END_OBJECT = COLUMN OBJECT = COLUMN NAME = EARTH_RECEIVED_START_TIME DATA_TYPE = TIME START_BYTE = 673 BYTES = 24 FORMAT = "A24" DESCRIPTION = "Identifies the earliest time that a telemetry packet containing data for image was received. Has the form YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = EARTH_RECEIVED_STOP_TIME DATA_TYPE = TIME START_BYTE = 698 BYTES = 24 FORMAT = "A24" DESCRIPTION = "Identifies the latest time that a telemetry packet containing data for image was received. Has the form YYYY-MM-DDThh:mm:ss.fffZ" END_OBJECT = COLUMN OBJECT = COLUMN NAME = SURFACE_BASED_INST_AZIMUTH DATA_TYPE = ASCII_REAL START_BYTE = 723 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "One of two angular measurements of the pointing direction of the instrument. The azimuth is measured positively in the clockwise direction (as viewed from above) with the meridian passing through the positive spin axis ('north pole') defining the zero reference. The angle is measured in the local gravity horizontal plane, ie., a plane perpendicular to the local gravity vector." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SURFACE_BASED_INST_ELEVATION DATA_TYPE = ASCII_REAL START_BYTE = 732 BYTES = 8 FORMAT = "F8.4" DESCRIPTION = "One of two angular measurements of the pointing direction of the instrument. For the Mars Pathfinder IMP EDRs, elevation is measured positively upwards from the plane which is perpendicular to the local gravity vector and which intersects the elevation axis around with the camera rotates. Valid values: -90 degrees (nadir) to +90 degrees (zenith)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SURFACE_BASED_INST_METHOD DATA_TYPE = CHARACTER START_BYTE = 742 BYTES = 18 FORMAT = "A18" DESCRIPTION = "Identifies the method used to calculate the surface based instrument pointing. Valid values: NULL, L_FRAME-QUATERNION" END_OBJECT = COLUMN OBJECT = COLUMN NAME = TARGET_NAME DATA_TYPE = CHARACTER START_BYTE = 763 BYTES = 8 FORMAT = "A8" DESCRIPTION = "Identifies the intended target of an observation. Can be either a planetary body or a physical object. The following is the list of targets imaged by the IMP: APXSSITE, ALTAIR, ARCTURUS, CALIMG, DEIMOS, LANDER, MAG, MARS, PHOBOS, ROVER, SKY, SUN, VEGA, WINDSOCKS " END_OBJECT = COLUMN OBJECT = COLUMN NAME = TLM_CMD_DISCREPANCY_FLAG DATA_TYPE = CHARACTER START_BYTE = 774 BYTES = 1 FORMAT = "A1" DESCRIPTION = "Indicates whether or not discrepancies were found between the IMP uplinked commands and the downlinked telemetry. Valid values: 'T' and 'F'." END_OBJECT = COLUMN END_OBJECT = INDEX_TABLE END
C.4 GAZETTER.LBL
The GAZETTER.LBL file describes the structure of the GAZETTER.TAB file, which contains a listing of some of the informal feature names at the Mars Pathfinder landing site.
PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 104 FILE_RECORDS = 91 ^TABLE = "GAZETTER.TAB" OBJECT = TABLE NAME = "Mars Pathfinder Landing Site Gazetteer" INTERCHANGE_FORMAT = ASCII ROWS = 91 COLUMNS = 9 ROW_BYTES = 104 DESCRIPTION = "This table is a gazetteer of the names informally assigned to many of the rocks and other local small features visible near the Mars Pathfinder landing site." OBJECT = COLUMN NAME = TARGET_NAME DATA_TYPE = CHARACTER START_BYTE = 2 BYTES = 8 FORMAT = "A8" DESCRIPTION = "The planet or satellite on which the feature is located." END_OBJECT = COLUMN OBJECT = COLUMN NAME = SEARCH_FEATURE_NAME DATA_TYPE = CHARACTER START_BYTE = 13 BYTES = 20 FORMAT = "A20" DESCRIPTION = "The geographical feature name with all diacritical marks stripped off. This name is stored in upper case only so that it can be used for sorting and search purposes." END_OBJECT = COLUMN OBJECT = COLUMN NAME = DIACRITIC_FEATURE_NAME DATA_TYPE = CHARACTER START_BYTE = 36 BYTES = 20 FORMAT = "A20" DESCRIPTION = "The geographical feature name containing standard diacritical information. Only one feature in the Pathfinder table requires a diacritical mark, and that is Souffle, which has an acute accent on the 'e'." END_OBJECT = COLUMN OBJECT = COLUMN NAME = GRID_POSITION_X DATA_TYPE = ASCII_REAL START_BYTE = 58 BYTES = 6 FORMAT = "F6.2" UNIT = METER DESCRIPTION = "The north / south component of the object's position. A positive value indicates that the object was north of the lander; a negative value indicates it was to the south. The magnitude gives the distance between the object and an east / west line drawn through the center of the lander base petal (the origin of Mars Local Level coordinate frame)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = GRID_POSITION_Y DATA_TYPE = ASCII_REAL START_BYTE = 65 BYTES = 6 FORMAT = "F6.2" UNIT = METER DESCRIPTION = "The east / west component of the object's position. A positive value indicates that the object was east of the lander; a negative value indicates that it was to the west. The magnitude gives the distance between the object and a north / south line drawn through the center of the lander base petal (the origin of the Mars Local Level coordinate frame)." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FEATURE_DISTANCE DATA_TYPE = ASCII_REAL START_BYTE = 72 BYTES = 6 FORMAT = "F6.2" UNIT = METER DESCRIPTION = "The object's distance from the origin of the Mars Local Level coordinate frame." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FEATURE_WIDTH DATA_TYPE = ASCII_REAL START_BYTE = 79 BYTES = 5 FORMAT = "F5.2" UNIT = METER DESCRIPTION = "The horizontal size of the object: the width of its maximum intersection with any plane perpendicular to the IMP camera's line of sight. Estimated by virtual measurement." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FEATURE_HEIGHT DATA_TYPE = ASCII_REAL START_BYTE = 85 BYTES = 5 FORMAT = "F5.2" UNIT = METER DESCRIPTION = "The vertical size of the feature. Consider a diagonal line segment drawn from the highest point of a rock to a point where it touches the Mars surface or extends below it. Taking that line segment as the hypoteneus of a right triangle, the length of the vertical side is the height of the rock. The distance was determined by virtual measurement, using the following technique: (i) find the lowest point (maximum Z value) of the Martian surface in close proximity to a rock by moving the cursor around in MarsMap, (ii) finding the highest point on the rock (minimum Z value) by moving the cursor over the rock in Marsmap, and (iii) taking the difference of the Z values." END_OBJECT = COLUMN OBJECT = COLUMN NAME = FEATURE_TYPE DATA_TYPE = CHARACTER START_BYTE = 92 BYTES = 10 FORMAT = "A10" UNIT = "N/A" DESCRIPTION = "This is used to distinguish rock-like objects from a few other named surface features. The types used, which are not the usual list of IAU feature types visible from orbit, are: ROCK: Any object that superficially appears to be a rock, although many of them may later be interpreted to be crust, clods, conglomerates, etc. DUNE: Used for Mermaid Dune. AREA: An extended area that bears a name for easy reference. Used for Baker's Bench and Photometry Flats." END_OBJECT = COLUMN END_OBJECT = TABLE END
D SAMPLE PDS IMAGE LABEL
PDS_VERSION_ID = PDS3 /* FILE CHARACTERISTICS */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = number of bytes per record in the file FILE_RECORDS = total number of records in the file LABEL_RECORDS = number of records in the file containing only label information /* POINTERS TO DATA OBJECTS */ ^IMAGE = first record in file containing image data /* IDENTIFICATION DATA ELEMENTS */ DATA_SET_ID = "MPFL-M-IMP-2-EDR-V1.0" DATA_SET_NAME = "MPF LANDER MARS IMAGER FOR MARS PATHFINDER 2 EDR V1.0" PRODUCER_ID = "MIPL OF JPL" PRODUCER_FULL_NAME = "ALLAN J. RUNKLE" PRODUCER_INSTITUTION_NAME = "MULTIMISSION IMAGE PROCESSING LABORATORY, JET PROPULSION LAB" PRODUCT_ID = "IMP_EDR-<sclkstrtcnt>-<image_observation_ type>-<image_id>" IMAGE_ID = nnnnnnnnnn COMMAND_SEQUENCE_NUMBER = nnnn IMAGE_OBSERVATION_TYPE = <REGULAR, DARK_CURRENT, FLAT_FIELD, HISTOGRAM, SUMMATION, DARK_STRIP, NULL_STRIP> FRAME_ID = <LEFT, RIGHT, BOTH, LEFT_HALF> MISSION_NAME = "MARS PATHFINDER" INSTRUMENT_HOST_NAME = "MARS PATHFINDER LANDER" INSTRUMENT_NAME = "IMAGER FOR MARS PATHFINDER" INSTRUMENT_ID = "IMP" TARGET_NAME = planetary body, feature, or region OBSERVATION_NAME = purpose of observation IMAGE_TIME = yyyy-mm-ddThh:mm:ss.fffZ PLANET_DAY_NUMBER = nn MPF_LOCAL_TIME = hh:mm:ss SPACECRAFT_CLOCK_START_COUNT = nnnnnnnnnn EARTH_RECEIVED_START_TIME = yyyy-mm-ddThh:mm:ss.fffZ EARTH_RECEIVED_STOP_TIME = yyyy-mm-ddThh:mm:ss.fffZ PRODUCT_CREATION_TIME = yyyy-mm-ddThh:mm:ss.fffZ /* DESCRIPTIVE DATA ELEMENTS */ EXPECTED_PACKETS = n RECEIVED_PACKETS = n APPLICATION_PACKET_ID = n APPLICATION_PACKET_NAME = group name associated with APID EXPOSURE_DURATION = f.ffff EXPOSURE_TYPE = <AUTO, INCREMENTAL, MANUAL, PRETIMED, NONE> EXPOSURE_COUNT = n AUTO_EXPOSURE_DATA_CUT = n AUTO_EXPOSURE_PIXEL_FRACTION = f.ffff ERROR_PIXELS = n FILTER_NAME = <"L440_R440", "L450_R670", "L885_R947", "L925_R935", "L935_R990", "L670_R670", "L800_R750", "L860_R-DIOPTER", "L900_R600", "L930_R530", "L1000_R480", "L965_R965"> FILTER_NUMBER = n INSTRUMENT_TEMPERATURE = (f.ffff, f.ffff) INSTRUMENT_TEMPERATURE_COUNT = (n, n) INSTRUMENT_DEPLOYMENT_STATE = <"STOWED", "DEPLOYED", "UNKNOWN"> DETECTOR_PIXEL_HEIGHT = f.ffff DETECTOR_PIXEL_WIDTH = f.ffff SOURCE_PRODUCT_ID = standard SPICE kernel names for PCK, SPK, etc SOFTWARE_NAME = name of MPF telemetry processing software SOFTWARE_VERSION_ID = version of MPF telemetry processing software PROCESSING_HISTORY_TEXT = "CODMAC LEVEL 1 TO LEVEL 2 CONVERSION VIA JPL/MIPL MPFTELEMPROC" /* GEOMETRY DATA ELEMENTS */ INSTRUMENT_AZIMUTH = f.ffff AZIMUTH_FOV = f.ffff AZIMUTH_MOTOR_CLICKS = n INSTRUMENT_AZIMUTH_METHOD = <"TELEMETRY", "MPFNAV-MIPS", "BACKLASH-UOFA"> INSTRUMENT_ELEVATION = f.ffff ELEVATION_FOV = f.ffff ELEVATION_MOTOR_CLICKS = n INSTRUMENT_ELEVATION_METHOD = <"TELEMETRY", "MPFNAV-MIPS", "BACKLASH-UOFA"> SURFACE_BASED_INST_AZIMUTH = f.ffff SURFACE_BASED_INST_ELEVATION = f.ffff SURFACE_BASED_INST_METHOD = "L_FRAME-QUATERNION" POSITIVE_ELEVATION_DIRECTION = UP SOLAR_AZIMUTH = f.ffff SOLAR_ELEVATION = f.ffff LANDER_SURFACE_QUATERNION = (f.ffff, f.ffff, f.ffff, f.ffff) /* IMP FLIGHT SOFTWARE COMMAND DATA ELEMENTS */ COMMAND_NAME = name of the uplinked command COMMAND_DESC = text which describes the uplinked command TLM_CMD_DISCREPANCY_FLAG = <TRUE, FALSE> DOWNLOAD_TYPE = <NONE, DS, IM, DSIM, NS, DSNS, IMNS, DSIMNS> DARK_CURRENT_DOWNLOAD_FLAG = <TRUE, FALSE> DARK_CURRENT_CORRECTION_FLAG = <TRUE, FALSE> FLAT_FIELD_CORRECTION_FLAG = <TRUE, FALSE> BAD_PIXEL_REPLACEMENT_FLAG = <TRUE, FALSE> SHUTTER_EFFECT_CORRECTION_FLAG = <TRUE, FALSE> SQRT_COMPRESSION_FLAG = <TRUE, FALSE> /* COMPRESSION DATA ELEMENTS */ INST_CMPRS_BLK_SIZE = (n, n) INST_CMPRS_BLOCKS = n INST_CMPRS_MODE = n INST_CMPRS_PARAM = n INST_CMPRS_QUALITY = n INST_CMPRS_QUANTZ_TBL_ID = name or code identifying the reference table used for quantization in the frequency domain for on-board transform compression INST_CMPRS_QUANTZ_TYPE = TABULAR INST_CMPRS_SYNC_BLKS = n INST_CMPRS_NAME = <"RICE ADAPTIVE VARIABLE-LENGTH CODING (RICE)", "JPEG DIRECT COSINE TRANSFORM (DCT)"> INST_CMPRS_RATE = f.ffff INST_CMPRS_RATIO = f.ffff PIXEL_AVERAGING_HEIGHT = n PIXEL_AVERAGING_WIDTH = n RICE_START_OPTION = n RICE_OPTION_VALUE = n SQRT_MINIMUM_PIXEL = n SQRT_MAXIMUM_PIXEL = n /* IMAGE OBJECT DATA ELEMENTS */ OBJECT = IMAGE INTERCHANGE_FORMAT = BINARY LINES = n LINE_SAMPLES = n BANDS = 1 SAMPLE_TYPE = MSB_UNSIGNED_INTEGER SAMPLE_BITS = <8, 16, or 32> SAMPLE_BIT_MASK = <2#11111111#, 2#0000111111111111#, or 2#11111111111111111111111111111111#> MAXIMUM = n MEAN = f.ffff MEDIAN = n MINIMUM = n STANDARD_DEVIATION = f.ffff FIRST_LINE = n FIRST_LINE_SAMPLE = n CHECKSUM = <32 bit unsigned integer> END_OBJECT = IMAGE END
E VOLUME DESCRIPTION FILE
This file contains a description of the contents of the CD in a human and machine readable format.
PDS_VERSION_ID = PDS3 OBJECT = VOLUME VOLUME_SERIES_NAME = "MISSION TO MARS" VOLUME_SET_NAME = "MARS PATHFINDER: THE IMAGER FOR MARS PATHFINDER EDR" VOLUME_SET_ID = "USA_NASA_PDS_MPIM_00XX" VOLUMES = 3 VOLUME_NAME = "VOLUME 1: IMP EDRS 1229455934 - 1247913223" VOLUME_ID = "MPIM_0001" VOLUME_FORMAT = "ISO-9660" VOLUME_VERSION_ID = "VERSION 1" MEDIUM_TYPE = "CD-ROM" DATA_SET_ID = "MPFL-M-IMP-2-EDR-V1.0" PUBLICATION_DATE = 1998-07-01 DESCRIPTION = "This volume contains images taken by the Imager for Mars Pathfinder on July 4 through July 18, 1997 (plus a few pre-landing calibration images). The images are Experiment Data Records, which have been decoded and decompressed in single frame form, but not calibrated or radiometrically corrected. The volume also contains detailed documentation about the mission, spacecraft, instrument, and data set, as well as calibration information, a gazetteer, an HTML image browser, and index tables." OBJECT = DATA_PRODUCER INSTITUTION_NAME = "JET PROPULSION LABORATORY" FACILITY_NAME = "MULTIMISSION IMAGE PROCESSING LABORATORY" FULL_NAME = "ALLAN J. RUNKLE" ADDRESS_TEXT = "JET PROPULSION LABORATORY\n 4800 OAK GROVE DRIVE\n MAILSTOP 168-414\n PASADENA, CA 91109\n USA" TELEPHONE_NUMBER = "8183546006" ELECTRONIC_MAIL_TYPE = "INTERNET" ELECTRONIC_MAIL_ID = "allan.j.runkle@jpl.nasa.gov" END_OBJECT = DATA_PRODUCER OBJECT = DATA_SUPPLIER INSTITUTION_NAME = "JET PROPULSION LABORATORY" FACILITY_NAME = "MULTIMISSION IMAGE PROCESSING LABORATORY" FULL_NAME = "SUSAN K. LAVOIE" DISCIPLINE_NAME = "IMAGE PROCESSING" NODE_NAME = "IMAGING" ADDRESS_TEXT = "JET PROPULSION LABORATORY\n 4800 OAK GROVE DRIVE\n MAILSTOP 168-527\n PASADENA, CA 91109\n USA" TELEPHONE_NUMBER = "8183545677" ELECTRONIC_MAIL_TYPE = "INTERNET" ELECTRONIC_MAIL_ID = "susan.k.lavoie@jpl.nasa.gov" END_OBJECT = DATA_SUPPLIER OBJECT = CATALOG ^DATA_SET_CATALOG = "DATASET.CAT" ^INSTRUMENT_CATALOG = "INST.CAT" ^INSTRUMENT_HOST_CATALOG = "INSTHOST.CAT" ^MISSION_CATALOG = "MISSION.CAT" ^PERSONNEL_CATALOG = "PERSON.CAT" ^REFERENCE_CATALOG = "REF.CAT" END_OBJECT = CATALOG END_OBJECT = VOLUME END