Data Set Information
DATA_SET_NAME ROSETTA-ORBITER STEINS MIRO 3 AST1 STEINS V1.0
DATA_SET_ID RO-A-MIRO-3-AST1-STEINS-V1.0
NSSDC_DATA_SET_ID
DATA_SET_TERSE_DESCRIPTION
DATA_SET_DESCRIPTION
Data Set Overview :  This dataset contains data generated by MIRO during the Steins Fly-by mission phase of Rosetta. These data cover the following periods and activities:  (All are in 2008, so Year is omitted from dates.)  Start Time Stop Time Activity (mm-ddThh:mm) (mm-ddThh:mm)  09-05T13:30 09-05T18:20 Approach observations of Steins (MR02) 09-05T18:27 09-05T18:50 Asteroid mode obs. of Steins (MR03) 09-05T18:50 09-05T20:31 Recession observations of Steins (MR04) 09-06T01:30 09-06T01:44 Asteroid mode obs. of dark sky (MR05)  The three Steins observations have separate files in the DATA/SPECTROSCOPIC directory, but the CONTINUUM files are not separated since Asteroid Mode has no special effect on contimuum data.  The first three observations involved direct scientific observations of the asteroid itself. The fourth observation did not observe the asteroid, but had two goals: (a) to establish the dark level of the continuum channels by turning the LNA power off, and (b) to determine the dark level of the spectroscopic channels by staring at the dark sky for several hours.  Note that no calibrated data were generated for the Active Payload Checkout #8, in contrast to the corresponding level-2 archive, because calibrated data are not meaningful for that test.  Author List :  The author list in the CITATION_DESC includes only those persons who worked on preparing this archive dataset for delivery. The full list of all persons involved in the MIRO experiment is (taken from the GULKISETAL2007 reference): S. Gulkis, Frerking, M., Crovisier, J., Beaudin, G., Hartogh, P., Encrenaz, P., Koch, T., Kahn, C., Salinas, Y., Nowicki, R., Irigoyen, R., Janssen, M., Stek, P., Hofstadter, M., Allen, M., Backus, C., Kamp, L., Jarchow, C., Steinmetz, E., Deschamps, A., Krieg, J., Gheudin, M., Bockelee-Morvan, D., Biver, N., Encrenaz, T., Despois, D., Ip, W., Lellouch, E., Mann, I., Muhleman, D., Rauer, H., Schloerb, P., and Spilker, T.  Geometry Information :  The MIRO data file labels contain vectors specifying the position of the Sun and Target body relative to the spacecraft and the velocity of the Target body relative to the spacecraft. The values of the keywords SC_SUN_POSITION_VECTOR, SC_TARGET_POSITION_VECTOR and SC_TARGET_VELOCITY_VECTOR are related to the ECLIPJ2000 reference frame. The values of SUB_SPACECRAFT_LATITUDE and SUB_SPACECRAFT_LONGITUDE are northern latitude and eastern longitude in the standard planetocentric IAU  frame. All values are computed for the the midpoint of the observations. Distances are given in , velocities in , angles in .  This information was obtained using the following NAIF/SPICE kernel files:  ORHR_______________00061.BSP de405s.bsp  The vectors were retrieved using the NAIF call SPKEZ() with a correction for one-way light time and stellar aberration using a Newtonian formulation.  More geometry information is given in the GEOMETRY directory of this archive.
DATA_SET_RELEASE_DATE 2009-05-01T00:00:00.000Z
START_TIME 2008-09-05T01:08:00.000Z
STOP_TIME 2008-09-06T05:00:00.000Z
MISSION_NAME INTERNATIONAL ROSETTA MISSION
MISSION_START_DATE 1995-03-01T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME 2867 STEINS
CALIBRATION
TARGET_TYPE ASTEROID
CALIBRATION
INSTRUMENT_HOST_ID RO
INSTRUMENT_NAME MICROWAVE INSTRUMENT FOR THE ROSETTA ORBITER
INSTRUMENT_ID MIRO
INSTRUMENT_TYPE RADIOMETER
NODE_NAME Small Bodies
ARCHIVE_STATUS ARCHIVED
CONFIDENCE_LEVEL_NOTE
The calibration algorithms used to generate these data are still under development, so the current values must be regarded as preliminary, with uncertainties of order 10%.
CITATION_DESCRIPTION Gulkis, S., Backus, C.R., Janssen, M.A., Kamp, L.W. et al., ROSETTA MIRO INSTRUMENT CALIBRATED DATA FOR THE STEINS FLY-BY, RO-A-MIRO-3-AST1-STEINS-V1.0, ESA PLANETARY SCIENCE ARCHIVE AND NASA PLANETARY DATA SYSTEM, 2009
ABSTRACT_TEXT This data set contains radiometrically calibrated Spectroscopic and Continuum data, in the form of table files, taken during the Steins Fly-by phase of the Rosetta mission by the MIRO instrument.
PRODUCER_FULL_NAME Dr. Samuel Gulkis
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