| Field | Description | Type | Null | Limits | Size | Key | Default | Authority | Source |
|---|---|---|---|---|---|---|---|---|---|
| ID | Numerical ID for each product entry in the table. | INT(11) | Not Null | unique index | Database Server | ||||
| VOLUME_ID | The PDS Volume ID | VARCHAR(9) | PDS cumindex.tab | ||||||
| FILE_SPECIFICATION_NAME | File path on the PDS Volume | VARCHAR(19) | PDS cumindex.tab | ||||||
| PRODUCT_ID | Product ID for image. | VARCHAR(12) | Not Null | unique index | PDS cumindex.tab | ||||
| IMAGE_TIME | SCET time at start of image | DATETIME | PDS cumindex.tab | ||||||
| INSTRUMENT_NAME | The name of the instrument that produced this image product. | VARCHAR(6) | PDS cumindex.tab | ||||||
| FILTER_NAME | Filter name (RED or BLUE, N/A for NA) | VARCHAR(4) | PDS cumindex.tab | ||||||
| LINE_SAMPLES | image width | SMALLINT(4) unsigned | PDS cumindex.tab | ||||||
| IMAGE_LINES | image height | MEDIUMINT(6) unsigned | PDS cumindex.tab | ||||||
| CROSSTRACK_SUMMING | Crosstrack summing. For global images the crosstrack summing is variable across the detector. Please refer to the mocsis.txt appendix F for a full description. | TINYINT(2) unsigned | PDS cumindex.tab | ||||||
| DOWNTRACK_SUMMING | downtrack summing | TINYINT(2) unsigned | PDS cumindex.tab | ||||||
| SCALED_PIXEL_WIDTH | image resolution in meters/pixel at center of image | FLOAT(8,2) | PDS cumindex.tab | ||||||
| PIXEL_ASPECT_RATIO | Pixel aspect ratio (pixel height/pixel width) at center of image. The image's center pixel is projected on the ground and its linear extents are ratioed, so any effects of emission angle and line time are modelled. To recover an image with 'square' pixels, the image should be resampled to a height of aspect_ratio * input height. | FLOAT(6,2) | PDS cumindex.tab | ||||||
| EMISSION_ANGLE | emission angle at center of image | FLOAT(6,2) | PDS cumindex.tab | ||||||
| INCIDENCE_ANGLE | incidence angle at center of image | FLOAT(6,2) | PDS cumindex.tab | ||||||
| PHASE_ANGLE | phase angle at center of image | FLOAT(6,2) | PDS cumindex.tab | ||||||
| CENTER | The image center coordinates stored as a GIS object. | POINT | Not Null | PDS cumindex.tab | |||||
| CENTER_LONGITUDE | center longitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| CENTER_LATITUDE | center areographic latitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| FOOTPRINT | The footprint coordinates stored as a GIS polygon object. | POLYGON | Not Null | PDS cumindex.tab | |||||
| UPPER_LEFT_LONGITUDE | upper left longitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| UPPER_LEFT_LATITUDE | upper left areographic latitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| UPPER_RIGHT_LONGITUDE | upper right longitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| UPPER_RIGHT_LATITUDE | upper right areographic latitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| LOWER_LEFT_LONGITUDE | lower left longitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| LOWER_LEFT_LATITUDE | lower left areographic latitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| LOWER_RIGHT_LONGITUDE | lower right longitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| LOWER_RIGHT_LATITUDE | lower right areographic latitude | FLOAT(6,2) | PDS cumindex.tab | ||||||
| MISSION_PHASE_NAME | mission phase name | VARCHAR(10) | PDS cumindex.tab | ||||||
| TARGET_NAME | target name (e.g., MARS, PHOBOS, STAR, SPACE) | VARCHAR(6) | PDS cumindex.tab | ||||||
| SPACECRAFT_CLOCK_START_COUNT | spacecraft clock value at start of image | VARCHAR(15) | PDS cumindex.tab | ||||||
| FOCAL_PLANE_TEMPERATURE | focal plane temp in Celsius | FLOAT(5,1) | PDS cumindex.tab | ||||||
| LINE_EXPOSURE_DURATION | line integration time in milliseconds | FLOAT(8,4) | PDS cumindex.tab | ||||||
| GAIN_MODE_ID | gain mode (see documentation) | VARCHAR(2) | PDS cumindex.tab | ||||||
| OFFSET_MODE_ID | offset mode (see documentation) | VARCHAR(3) | PDS cumindex.tab | ||||||
| EDIT_MODE_ID | first pixel stored from detector, zero-based | SMALLINT(4) unsigned | PDS cumindex.tab | ||||||
| ENCODING_TYPE | A description of the compression applied to this image, of the form string-parms, where <string> is taken from the set {MOC-NONE,MOC-PRED,MOC-DCT,MOC-WHT} and <parms> are additional parameters describing the algorithm-specific compression parameters. | VARCHAR(14) | PDS cumindex.tab | ||||||
| SCALED_IMAGE_WIDTH | image width from left to right image edge in km | FLOAT(7,2) | PDS cumindex.tab | ||||||
| SCALED_IMAGE_HEIGHT | image height from first line to last line in km | FLOAT(8,2) | PDS cumindex.tab | ||||||
| SPACECRAFT_ALTITUDE | distance from s/c to closest point on surface in km | FLOAT(7,2) | PDS cumindex.tab | ||||||
| TARGET_CENTER_DISTANCE | distance from s/c to target body center in km | FLOAT(7,2) | PDS cumindex.tab | ||||||
| SLANT_DISTANCE | range from s/c to intersection of view vector with target body in km | FLOAT(7,2) | PDS cumindex.tab | ||||||
| USAGE_NOTE | Because of the MOC's line-scan nature, depending on the orientation and sense of rotation of the spacecraft and the optical inversion properties of the camera system involved, MOC images can either be normal or flipped left-for-right (independent of whether the image is north up or south up.) This flag will be 'F' if the image should be flipped left-to-right, and 'N' if it is already in normal form. | VARCHAR(1) | PDS cumindex.tab | ||||||
| NORTH_AZIMUTH | The angle in degrees clockwise from the reference axis of the image (a line from the center to the right edge of the image) to the direction to the north pole of the target body. If the USAGE_NOTE described previously is 'F', the image should be flipped prior to applying this angle. | FLOAT(6,2) | PDS cumindex.tab | ||||||
| SUB_SOLAR_AZIMUTH | The angle in degrees clockwise from the reference axis of the image (a line from the center to the right edge of the image) to the direction to the subsolar point on the target body. If the USAGE_NOTE described previously is 'F', the image should be flipped prior to applying this angle. | FLOAT(6,2) | PDS cumindex.tab | ||||||
| SUB_SOLAR_LONGITUDE | west longitude of subsolar point in degrees | FLOAT(6,2) | PDS cumindex.tab | ||||||
| SUB_SOLAR_LATITUDE | planetographic latitude of subsolar point in degrees | FLOAT(6,2) | PDS cumindex.tab | ||||||
| SUB_SPACECRAFT_LONGITUDE | west longitude of subspacecraft point in degrees | FLOAT(6,2) | PDS cumindex.tab | ||||||
| SUB_SPACECRAFT_LATITUDE | planetographic latitude of subspacecraft point in degrees | FLOAT(6,2) | PDS cumindex.tab | ||||||
| SOLAR_DISTANCE | distance from the center of the image on the target body to the center of the sun in km | FLOAT(11,1) | PDS cumindex.tab | ||||||
| SOLAR_LONGITUDE | solar longitude ('L sub s') at time of image in degrees from martian vernal equinox, as computed by the method in 'Accurate analytic representations of solar time and seasons on Mars with applications to the Pathfinder/Surveyor missions', Michael Allison, Geophysical Reseach Letters 24, 16, pp 1967-1970 (August 15, 1997) | FLOAT(6,2) | PDS cumindex.tab | ||||||
| LOCAL_TIME | Local True Solar Time in decimal hours from midnight at the center of the image, as computed by the method in 'Accurate analytic representations of solar time and seasons on Mars with applications to the Pathfinder/Surveyor missions', Michael Allison, Geophysical Reseach Letters 24, 16, pp 1967-1970 (August 15, 1997). An 'hour' in this context is an angular measure of 15 degrees of solar motion. | FLOAT(5,2) | PDS cumindex.tab | ||||||
| IMAGE_SKEW_ANGLE | The image skew angle is the absolute value, in degrees, of the angle between the left edge (a line between the lower left and upper left corners) and the bottom edge (a line between the lower left and lower right corners) of the image, where the edges are projected on the target body. For images whose footprints are exactly rectangular, this angle will be 90 degrees. Departures from 90 degrees indicate a non-rectangular image footprint, caused by slews of the spacecraft during imaging outside the orbit plane or off-nadir pointing, or both. | FLOAT(5,1) | PDS cumindex.tab | ||||||
| RATIONALE_DESC | A text description of the scientific purpose for the acquisition of this image. For routine mapping operations, this will most likely be the goal of the image as targeted (which may not be met if the image missed its target significantly, the atmosphere was cloudy, gain parameters were set inappropriately, etc.) | VARCHAR(80) | PDS cumindex.tab | ||||||
| DATA_QUALITY_DESC | 'OK' if all fragments of the image are received without detected checksum or sequence errors, and 'ERRORS' otherwise. | VARCHAR(6) | PDS cumindex.tab | ||||||
| ORBIT_NUMBER | orbit number as defined by the MGS Project | MEDIUMINT(5) unsigned | PDS cumindex.tab | ||||||
| LAST_UPDATE | This column records the last time that a record was updated. | TIMESTAMP | db server |
Table Options:
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