Data Set Information
|
DATA_SET_NAME |
IRAS POSITION AND POINTING V1.0
|
DATA_SET_ID |
IRAS-6-SDR-SATELLITE-STATUS-V1.0
|
NSSDC_DATA_SET_ID |
GD-11F
|
DATA_SET_TERSE_DESCRIPTION |
Spacecraft position vectors and individual scan parameters for
the IRAS mission
|
DATA_SET_DESCRIPTION |
Data Set Overview
=================
This data presented with this data set include
IRASPOS.TAB - The IRAS Position File describes the position of the
satellite in its orbit about the Earth at 200 second intervals in
heliocentric ecliptic rectangular coordinates (B1950), where the
X axis points to the First Point of Ares. In addition an Earth
ephemeris is also included, which was generated by Miles Standish
at JPL using the information that was available in 1983 to best
approximate the knowledge of the Earth's position that was used
in the reduction of the IRAS data. Finally, the geocentric
position of the satellite is calculated using the above
information.
SCAN.TAB - The IRAS Scan History File describes the pointing
geometry and length of each survey-mode scan (by SOP OBS) over
the entire mission.
|
DATA_SET_RELEASE_DATE |
1997-03-24T00:00:00.000Z
|
START_TIME |
1983-02-08T12:00:00.000Z
|
STOP_TIME |
1983-11-21T12:00:00.000Z
|
MISSION_NAME |
INFRARED ASTRONOMICAL SATELLITE
|
MISSION_START_DATE |
1983-01-26T12:00:00.000Z
|
MISSION_STOP_DATE |
1983-11-23T12:00:00.000Z
|
TARGET_NAME |
|
TARGET_TYPE |
|
INSTRUMENT_HOST_ID |
IRAS
|
INSTRUMENT_NAME |
FOCAL PLANE ARRAY
|
INSTRUMENT_ID |
FPA
|
INSTRUMENT_TYPE |
CAMERA
|
NODE_NAME |
Small Bodies
|
ARCHIVE_STATUS |
SUPERSEDED
|
CONFIDENCE_LEVEL_NOTE |
Review
======
IRASPOS.TAB underwent peer review on March 24, 1997.
SCAN.TAB was peer reviewed on April 26, 1993, and updated on March
24, 1997.
|
CITATION_DESCRIPTION |
Citation TBD
|
ABSTRACT_TEXT |
This data presented with this data set includes: (a) The position
of the satellite in its orbit about the Earth at 200 second
intervals in heliocentric ecliptic rectangular coordinates
(B1950), where the X axis points to the First Point of Ares. In
addition an Earth ephemeris is also included, which was generated
by Miles Standish at JPL using the information that was available
in 1983 to best approximate the knowledge of the Earth's
position that was used in the reduction of the IRAS data.
Finally, the geocentric position of the satellite is calculated
using the above information. (b) The IRAS Scan History File
describes the pointing geometry and length of each survey-mode
scan (by SOP OBS) over the entire mission.
|
PRODUCER_FULL_NAME |
MARK SYKES
|
SEARCH/ACCESS DATA |
SBN PSI WEBSITE
|