Data Set Information
|
DATA_SET_NAME |
PHOENIX MARS MECA OPTICAL MICROSCOPE 3
RADIOMETRIC SCI V1.0
|
DATA_SET_ID |
PHX-M-OM-3-RADIOMETRIC-SCI-V1.0
|
NSSDC_DATA_SET_ID |
|
DATA_SET_TERSE_DESCRIPTION |
PHX MECA Imaging RDR Science data
includes processed data products from the Optical Microscope (OM),
along with data from the MECA command electronics.
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
This data set contains data to help understand the morphology, reflectance
and texture of Martian soil and dust at the microscopic scale (typically in
the range 10 - 100 microns). In most cases full-frame images with full pixel
resolution will be acquired. In some cases, as e.g. for AFM context, the
images will be subframed. Onboard downsampling is available, but will not be
used during normal operations. Null strip (containing information on bias
and system noise) and dark strip (information on dark current) are returned
as a separate product if requested.
Parameters
==========
N/A
Processing
==========
This data set uses the Committee on Data Management and Computation (CODMAC)
data level numbering system. The Phoenix EDRs are considered CODMAC Level 2
(equivalent to NASA Level 0) or Edited Data (i.e. cleaned, time-ordered and
quality-flagged data). The EDRs are reconstructed from Level 1 or Raw Data,
which are the telemetry packets within the project specific Standard
Formatted Data Unit (SFDU) record. They are assembled into complete images,
but are not radiometrically or geometrically corrected. Phoenix EDR data
products were generated by the Multi-mission Image Processing Lab (MIPL) at
the Jet Propulsion Laboratory. The EDRs are raw uncalibrated data
reconstructed from telemetry packet SFDUs and formatted according to the
Camera EDR Software Interface Specification (SIS). Meta-data acquired from
the telemetry data headers and a meta-data database were used to populate
the PDS label. There will not be multiple versions of a Phoenix Camera EDR.
Missing packets will be identified and reported for retransmission to the
ground as partial datasets. Prior to retransmission, the missing EDR data
will be filled with zeros. The EDR data will be reprocessed only after all
partial datasets are retransmitted and received on the ground. In these
cases, the original EDR version will be overwritten. The EDR data product
will be placed into the File Exchange Interface (FEI) for distribution.
Data
====
The OM data files will be decoded, decompressed camera image data in single
frame form as an Experiment Data Record (EDR). The image data are acquired
as 12-bit data, but stored as 16-bit signed integers. There are three data
types:
1) Full Frame EDRs
Each Full Frame EDR contains a 512 columns * 256 rows image array. The size
of a Full Frame EDR data product is therefore approximately 2.1 Mb (260 kB).
2) Subframe EDRs
Subframe EDRs are intended to provide context for the AFM data.
3) Null & Dark Strip EDRs
Each Null & Dark Strip EDR contains a 16 columns * 256 rows array. The pixel
values are stored as 16-bit signed integers. The first and last 4 columns
are pre-pixels (obtained by reading out 'virtual pixels' without vertical
shift) and contain information on the bias value and system noise. The
central 8 columns are masked pixels that contain information on the dark
current. Null & Dark Strip EDRs are not available for each and every Full
Frame EDR, but will only be generated and downlinked occasionally upon
request.
Ancillary Data
==============
No ancillary data are needed to understand OM EDRs. Rotation and translation
positions of the sample wheel are specified in units of motor step numbers
in the EDR label. The Phoenix Project Software Interface Specification (SIS)
for Camera Data Products provides the necessary information to convert
rotation position step numbers into substrate IDs.
Coordinate System
=================
N/A
Software
========
PDS-labeled images and tables can be viewed with the program NASAView,
developed by the PDS and available for a variety of computer platforms from
the PDS web site http://pdsproto.jpl.nasa.gov/Distribution/license.html.
There is no charge for NASAView.
Media/Format
============
The data set will initially be delivered and kept online. Upon Mission
completion, the OM EDRs will be delivered to PDS on DVD as part of the
complete Phoenix EDR data set.
|
DATA_SET_RELEASE_DATE |
2008-12-23T00:00:00.000Z
|
START_TIME |
2008-05-25T12:00:00.000Z
|
STOP_TIME |
N/A (ongoing)
|
MISSION_NAME |
PHOENIX
|
MISSION_START_DATE |
2008-05-25T12:00:00.000Z
|
MISSION_STOP_DATE |
2008-11-02T12:00:00.000Z
|
TARGET_NAME |
MARS
|
TARGET_TYPE |
PLANET
|
INSTRUMENT_HOST_ID |
PHX
|
INSTRUMENT_NAME |
MECA OPTICAL MICROSCOPE
|
INSTRUMENT_ID |
OM
|
INSTRUMENT_TYPE |
IMAGING CAMERA
|
NODE_NAME |
Imaging
|
ARCHIVE_STATUS |
ARCHIVED
|
CONFIDENCE_LEVEL_NOTE |
Confidence Level Overview
=========================
N/A
Review
======
The data have not undergone any review process, such as PDS Peer review.
Data Coverage and Quality
=========================
No data gaps expected. Any data packets lost during downlink shall be
retransmitted (cf. section on Processing).
Limitations
===========
None.
|
CITATION_DESCRIPTION |
Hecht, Michael, Phoenix Mars MECA
Imaging Science RDR V1.0, NASA Planetary
Data System, PHX-M-OM-3-RADIOMETRIC-SCI-V1.0,
2008.
|
ABSTRACT_TEXT |
The Microscopy, Electrochemistry, and
Conductivity Analyzer (MECA) experiment on the Mars Phoenix Lander
consists of four instrument components plus command electronics. This
MECA Imaging Science RDR data set contains data from one of the four
MECA components, the Optical Microscope (OM).
|
PRODUCER_FULL_NAME |
MICHAEL H. HECHT
|
SEARCH/ACCESS DATA |
Imaging Planetary Image Atlas
Phoenix Analyst Notebook
Imaging Online Data Volumes
|
|