Data Set Information
DATA_SET_NAME PHOENIX MARS METEOROLOGICAL PRESSURE / TEMPERATURE EDR V1.0
DATA_SET_ID PHX-M-MET-2-PT-EDR-V1.0
NSSDC_DATA_SET_ID NULL
DATA_SET_TERSE_DESCRIPTION PHX MET pre-processed Pressure and Temperature Data.
DATA_SET_DESCRIPTION
Modification History
  ====================
    Version 1 data volumes include volumes MS000 through LS029, released
    Dec 2008.  These volumes contain MET data collected May 2008
    through June 2008, sols 0-29.
 
  Data Set Overview
  =================
 
    The Phoenix Mars Lander arrived at 68.2184N, 234.2487E on May 25, 2008.
 
    The PHX METEOROLOGICAL EDR DATA product contains unprocessed values of
    pressure and temperature data.  Each product is approximately 24 hours
    (LMST) in duration, and was collected continuously over the entire mission
    at a data rate of 2 sec.
 
    The Data are organized into 'High Resolution' (2 sec) and 'Low
    Resolution' (512 sec).  There are three temperature sensors
    along the vertical 1.0 m MET Mast (250, 500 and 1000mm), a
    reference Platinum Resistance Thermometer (PRT) at the base, and a
    pressure sensor on the Lander Deck on the Payload Electronic
    Box.  [TAYLOR2008]
 
    The collection of High Resolution Data is determined by the setting
    of P & T threshold values ranging from setting the thresholds to
    zero (constantly triggering, creating continuous 2 sec data) to
    essentially infinity (never triggering, creating no 2 sec data).
    Owing to favorable transmission bandwidth, the unit was operated over
    the entire mission in triggered (2 sec) mode.
 
    The Data is organized by a unique identifier (Token) is keeping with
    the other Phoenix instruments.  The token for the PT was nominally
    set each sol, when the PT instrument stopped recording to allow
    for transfer of data to the Lander (and hence telemetry to Earth).
    The token is provided as a 4 byte hex value.
 
 
  Parameters
  ==========
 
    Each EDR file contains time as the MET Frame count since instrument
    power on (1 count is 2 sec).
 
    The MET P&T threshold was commanded each sol, to trigger constantly,
    creating 2 sec data.  The calibration constants used internally onboard
    the unit were determined prior to launch, and outlined in the CCC report.
 
    The pre-processed EDR temperature data for each of the three
    thermocouples and the PRT were stored as a 16 bit value.  For the
    lower resolution 512 sec data the min, max and standard deviation
    were also stored at 16 bit.  All pressure values (avg, min, max, var)
    are given as 32 bit values.
 
    The temperature data is sent as a DN, which is converted in the MET
    Ground Data Segment into values of Kelvin (EDR -> RDR), while the
    pressure is send in units of PA.
 
    The MET PT instruments were nominally operated 24 hours of each Martian
    sol.  Once each sol, the instrument was transitioned out of RECORD
    to allow for transfer of data from MET flash to the Lander.  Thus
    there will nominally be a ~20 min gap each sol.
 
    During surface operations the MET PT was operated continuously, with a
    gap early in the mission (Sol 19/20) owing to a spacecraft event.
    Smaller data gaps exist, from dropouts in telemetry, but these were often
    recovered owing to use of the MET PT internal flash and data retransmits.
 
 
  Processing
  ==========
 
    The EDRs are essentially identical to the telemetry messages sent
    from the MET-PT instrument to the Lander computer, converted to ASCII
    and with the addition of a Lander timestamp (there is no onboard MET
    clock, so the instrument relies on an internal Frame Count.  Matching
    of this frame count and the Lander clock are made using the MET GDS)
    Commanded parameters, such as threshold values, are also added to the
    EDR products.
 
    Finally, the data were converted to PDS format, converting the
    tab-delimited fields to fixed-width fields, and exchanging the
    multiple packet headers for a single session header by the MET GDS.
 
    Address:     Cameron Dickinson
                 Dept. of Earth and Space Science Engineering
                 York University
                 4700 Keele St
                 Toronto, ON M3J 1P3
 
    Phone:       (416) 736-2100 X 23870
    Email:       cameron.dickinson@gmail.com
 
    For science related questions about the data, please contact the
    MET Instrument Science Team Lead:
 
    Address:     James Whiteway
                 Dept. of Earth and Space Science Engineering
                 York University
                 4700 Keele St
                 Toronto, ON M3J 1P3
 
    Phone:       (416) 736-2100 X 22310
    Email:       whiteway@yorku.ca
 
 
  Data
  ====
 
    All of the data in this data set are contained in ASCII tabular files
    with detached PDS labels.  Data is stored in a separate directory
    relating to the sol in which the recording of data commenced (i.e.
    data acquired from 003 10:00 local to 004 10:15 will be in the sol
    3 directory)
 
    Individual filenames are constructed as follows:
 
                             MS000EMH_00896227243_10CCM0.LBL
 
        1: The first character will always be an 'M', representing MET
           data.
        2: The second character will be an 'S', signifying surface
           data (versus 'C' for Cruise)
      3-5: The next three characters provide the sol number of the data
           file.
      6-8: The next three characters describe the type of MET data,
           EML - EDR MET LOW (Resolution)
           EMH - EDR MET HIGH (Resolution)
           RML - RDR MET LOW (Resolution)
           RMH - RDR MET HIGH (Resolution)
           RMC - RDR MET Corrected (Pressure Corrected Values)
           RMA - RDR MET Ancillary (Pressure Sensor Temperatures)
        9: Blank
    10-20: SCLK - Spacecraft clock
       21: Blank
    22-25: Operations Token
       26: Producer (M for MET Team)
       27: Version
       28: Period
    29-31: Extension, LBL or TAB
 
    The tabular files are formatted so that they may be read directly into
    many database management systems (DBMS) or spreadsheet programs on
    various computers.  Each of the files contains two tables.  The first
    is the header table, and is only a single record in length.  The
    second table contains all of the data records for a session and varies
    in length.
 
    All fields in the tables are stored in columns of fixed width and are
    right justified.  The records are of fixed length; since the header
    records are shorter than the data records, they have been padded with
    blank spaces at the end of the record.  The last two bytes of each
    record contain the ASCII carriage return and line feed characters.
    This allows the tables to be treated as fixed length record files on
    computers that support this file type and as normal text files on
    other computers.
 
    The PDS labels are object-oriented. The object to which the labels
    refer (the tables) 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 located outside the label file (as in this case), the
    location denotes the name of the file containing the object, along
    with the starting record.  For example:
 
        ^TABLE = 'MS013EML_00126907202_15C6M1.TAB'
 
    indicates that the TABLE object is in the same directory as the
    detached label file. (Records are counted starting at 1, not 0.)
 
    The detached label 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.
 
 
  Software
  ========
 
    The EDR/RDR tables can be displayed on UNIX, Macintosh,
    and PC platforms as simple ASCII files, or using the PDS developed
    program, NASAView.  This software is freely available from the PDS
    Central Node and may be obtained from their web site at
    http://pds.nasa.gov/.  For more information or help in obtaining
    the software, contact the PDS operator at the following address:
 
    Address:     Planetary Data System, PDS Operator
                 Jet Propulsion Laboratory
                 4800 Oak Grove Drive
                 Pasadena, CA 91109
 
    Phone:       (818) 354-4321
    Email:       pds_operator@jpl.nasa.gov
    WWW URL:     http://pds.nasa.gov/
DATA_SET_RELEASE_DATE 2008-12-23T00:00:00.000Z
START_TIME 2008-05-26T12:08:36.308Z
STOP_TIME 2008-06-25T06:14:37.816Z
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 METEOROLOGY SUITE, PRESSURE & TEMPERATURE
INSTRUMENT_ID MET
INSTRUMENT_TYPE METEOROLOGY
NODE_NAME Planetary Atmospheres
ARCHIVE_STATUS LOCALLY_ARCHIVED
CONFIDENCE_LEVEL_NOTE
Review
  ======
 
    The contents of this data have been peer reviewed by the following
    people:
 
    Lyle Huber        - PDS Atmospheres Node, New Mexico State University
    Jim Murphy        - PDS Atmospheres Node, New Mexico State University
    Cameron Dickinson - MET/Lidar Data Manager, York University
    Jim Whiteway      - MET/LIDAR Instrument Co-Investigator, York University
CITATION_DESCRIPTION Dickinson, C. D., PHX METEOROLOGICAL DATA V1.0, NASA Planetary Data System, 2008.
ABSTRACT_TEXT The PHX METEOROLOGICAL DATA product contains pre-processed (Digital Numbers) temperature and pressure data. The temperature data was collected at 250, 500 and 1000mm above the Phoenix Lander deck, and the pressure data was collected at (nearly) the height of the Lander deck. Nominally the data was collected at 2 sec resolution, but is also provided at 512 sec averages (with distribution statistics).
PRODUCER_FULL_NAME CAMERON S. DICKINSON
SEARCH/ACCESS DATA
  • Atmospheres Mars Archive
  • Phoenix Analyst Notebook
  • PHX MET EDR Volume PHMT_0XXX