DATA_SET_DESCRIPTION |
Data Set Overview
=================
This dataset contains data generated by MIRO during the Earth
Swing-by 1 mission phase of Rosetta. These data cover the
following periods and activities:
(All are in 2005, so Year is omitted from dates.)
Start Time Stop Time Activity
(mm-ddThh:mm) (mm-ddThh:mm)
03-04T08:10 03-04T21:36 Observation of Moon
03-04T21:36 03-04T22:10 Close observation of Earth
(Asteroid mode used)
03-04T22:10 03-05T10:20 Observation of Moon
03-05T12:00 03-05T15:40 Observation of Earth
03-05T17:20 03-07T11:45 Observation of Earth
03-07T11:45 03-07T14:02 Observation of Moon
Modification History
====================
Version 1.1 (Nov. 2010):
- Added UTC to all data files, revised *.FMT files and other
documentation accordingly.
- Added GEOMETRY directory.
- Minor corrections and additions.
- Added OIOR and LOG files to DOCUMENT directory.
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:
ORHR_______________00028.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.
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