PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = " 2011-07-01, L.Kamp, Created. " RECORD_TYPE = "STREAM" OBJECT = DATA_SET DATA_SET_ID = "RO-A-MIRO-3-AST2-LUTETIA-V1.0" OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "ROSETTA-ORBITER LUTETIA MIRO 3 AST2 LUTETIA V1.0" DATA_SET_TERSE_DESC = "Data from MIRO during the Lutetia Fly-by of Rosetta" ABSTRACT_DESC = "This data set contains radiometrically calibrated Spectroscopic and Continuum data, in the form of table files, taken during the Lutetia Fly-by phase of the Rosetta mission by the MIRO instrument." CITATION_DESC = "Gulkis, S., Hofstadter, M.D., Janssen, M.A., Kamp, L.W., Lee, S. et al., ROSETTA MIRO INSTRUMENT CALIBRATED DATA FOR THE LUTETIA FLY-BY, RO-A-MIRO-3-AST2-LUTETIA-V1.0, ESA PLANETARY SCIENCE ARCHIVE AND NASA PLANETARY DATA SYSTEM, 2011" ARCHIVE_STATUS = "IN PEER REVIEW" DATA_SET_COLLECTION_MEMBER_FLG = "N" DETAILED_CATALOG_FLAG = "N" DATA_OBJECT_TYPE = "TABLE" DATA_SET_RELEASE_DATE = 2011-07-05 PRODUCER_FULL_NAME = "Dr. Samuel Gulkis" START_TIME = 2010-07-10T06:14:00 STOP_TIME = 2010-07-11T06:15:00 DATA_SET_DESC = " Data Set Overview ================= This dataset contains data generated by MIRO during the Lutetia Fly-by mission phase of Rosetta. 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) 07-10T05:45 07-10T15:45 Observations of Lutetia (MR02) 07-11T01:30 07-11T16:45 Observations of dark sky (MR05) The first observation (MR02) involved direct scientific observations of the asteroid itself. The second 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. No calibrated spectroscopic were generated for the MR05 observation, because only differenced data were taken during the actual Lutetia observation (MR02), making the determination of a dark level irrelevant. Therefore, there are only Continuum data for MR05 in the DATA directories of this archive. Note that no calibrated data were generated for the Active Payload Checkout #12, 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: 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., Lee, S., 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." 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%." END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = "21 LUTETIA" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_TARGET TARGET_NAME = "CALIBRATION" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = "RO" INSTRUMENT_ID = "MIRO" END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_MISSION MISSION_NAME = "INTERNATIONAL ROSETTA MISSION" END_OBJECT = DATA_SET_MISSION OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "GULKISETAL2007" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END