Data Set Information
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| DATA_SET_NAME |
ROSETTA-ORBITER LUTETIA MIRO 2 AST2 LUTETIA V1.0
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| DATA_SET_ID |
RO-A-MIRO-2-AST2-LUTETIA-V1.0
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| NSSDC_DATA_SET_ID |
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| DATA_SET_TERSE_DESCRIPTION |
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| DATA_SET_DESCRIPTION |
Data Set Overview : This dataset contains data generated by MIRO during the Lutetia Flyby mission phase of Rosetta and also data obtained during the IFP Noise Figure Test of Active Payload Checkout 12, which fell in the same Mission Phase. These data cover the following periods and activities: (All are in 2010, so Year is omitted from dates.) Start Time Stop Time Activity (mm-ddThh:mm) (mm-ddThh:mm) 04-30T16:30 04-30T18:17 PC12 IFP Noise Figure Test 07-10T05:45 07-10T15:45 Approach observations of Lutetia 07-10T15:45 Closest Approach to Lutetia 07-10T15:45 07-10T16:45 Recession observations of Lutetia 07-11T03:45 07-11T06:15 Observations of dark sky 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 value s 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: ROS_LUTETIA_RSOC_V01.TPC ORHR_______________00109.BSP ORHS_______________00109.BSP de405.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.
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| DATA_SET_RELEASE_DATE |
2011-06-30T00:00:00.000Z
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| START_TIME |
2010-04-30T04:30:00.000Z
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| STOP_TIME |
2010-07-11T06:15:00.000Z
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| MISSION_NAME |
INTERNATIONAL ROSETTA MISSION
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| MISSION_START_DATE |
1995-03-01T12:00:00.000Z
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| MISSION_STOP_DATE |
N/A (ongoing)
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| TARGET_NAME |
21 LUTETIA
CALIBRATION
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| TARGET_TYPE |
ASTEROID
CALIBRATION
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| INSTRUMENT_HOST_ID |
RO
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| INSTRUMENT_NAME |
MICROWAVE INSTRUMENT FOR THE ROSETTA ORBITER
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| INSTRUMENT_ID |
MIRO
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| INSTRUMENT_TYPE |
RADIOMETER
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| NODE_NAME |
Small Bodies
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| ARCHIVE_STATUS |
IN_LIEN_RESOLUTION
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| 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.
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| CITATION_DESCRIPTION |
Gulkis, S., Hofstadter, M.D., Kamp, L.W., Lee, S. et al., ROSETTA MIRO INSTRUMENT RAW DATA FOR THE LUTETIA SWING-BY, RO-A-MIRO-2-AST2-LUTETIA-V1.0, ESA PLANETARY SCIENCE ARCHIVE AND NASA PLANETARY DATA SYSTEM, 2011
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| ABSTRACT_TEXT |
This data set contains Spectroscopic, Continuum and Engineering data, in the form of table files, taken during the LUTETIA flyby phase of the Rosetta mission by the MIRO instrument.
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| PRODUCER_FULL_NAME |
Dr. Samuel Gulkis
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| SEARCH/ACCESS DATA |
SBN Comet Website
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