Data Set Information
DATA_SET_NAME ROSETTA-ORBITER EARTH MIRO 2 EAR3 EARTH3 V1.0
DATA_SET_ID RO-E-MIRO-2-EAR3-EARTH3-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 Earth Swing-by 2 mission phase of Rosetta. These data cover the following periods and activities:  (All are in 2009, so Year is omitted from dates.)  Start Time Stop Time Activity (mm-ddThh:mm) (mm-ddThh:mm)  11-08T03:10 11-08T07:10 Raster scan of Moon while unresolved, in order to determine MIRO boresight position (MR04A). 11-13T05:20 11-13T14:30 Observations of Earth. 11-13T15:40 11-13T18:20 Observations of Moon. 11-18T03:10 11-18T07:10 Raster scan of Moon while unresolved, in order to determine MIRO boresight position (MR04A).  Operations on 2009-11-13 (DOY 317): The sequences dedicated to MIRO were (1) an Earth stare offset from nadir by about 11 degrees (to keep solar elongation < 140 deg.), from 07:20 to 08:20 (MR02), and (2) a dwell on the Moon's limb near the North Pole, from 17:20 to 18:20 (MR03), in order to search for H2O. However, outside these sequences, the MIRO instrument remained on during several maneuvers riding along with other instruments, gathering data, which are included in the files in the DATA subdirectory.  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_______________00089.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.
DATA_SET_RELEASE_DATE 2011-03-28T00:00:00.000Z
START_TIME 2009-11-07T09:00:00.000Z
STOP_TIME 2009-11-18T10:00:00.000Z
MISSION_NAME INTERNATIONAL ROSETTA MISSION
MISSION_START_DATE 1995-03-01T12:00:00.000Z
MISSION_STOP_DATE N/A (ongoing)
TARGET_NAME CALIBRATION
EARTH
MOON
TARGET_TYPE CALIBRATION
PLANET
SATELLITE
INSTRUMENT_HOST_ID RO
INSTRUMENT_NAME MICROWAVE INSTRUMENT FOR THE ROSETTA ORBITER
INSTRUMENT_ID MIRO
INSTRUMENT_TYPE RADIOMETER
NODE_NAME Small Bodies
ARCHIVE_STATUS IN_LIEN_RESOLUTION
CONFIDENCE_LEVEL_NOTE
These data were not processed in any way other than being decommutated from the raw telemetry stream, so no processing errors are expected. For a discussion of the reliability of the MIRO instrument itself, see the documentation included with this and subsequent mission archives.
CITATION_DESCRIPTION Gulkis, S., Backus, C.R., Janssen, M.A., Kamp, L.W. et al., ROSETTA MIRO INSTRUMENT RAW DATA FOR THE THIRD EARTH SWING-BY, RO-E-MIRO-2-EAR3-EARTH3-V1.0, ESA PLANETARY SCIENCE ARCHIVE AND NASA PLANETARY DATA SYSTEM, 2011
ABSTRACT_TEXT This data set contains Spectroscopic, Continuum and Engineering data, in the form of table files, taken during the third Earth swing-by phase of the Rosetta mission by the MIRO instrument.
PRODUCER_FULL_NAME Dr. Samuel Gulkis
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