PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 80 RELEASE_ID = 0001 REVISION_ID = 0000 OBJECT = TEXT PUBLICATION_DATE = 2010-05-18 NOTE = "Description of the GEOMETRY directory contents for the Venus Express SPICAV level 0B IR archive volume" END_OBJECT = TEXT END GEOMETRY Directory Contents ****************************************************************************** The time sampling period for the level 0B - IR DATA file is : time_spectrum = time_session * NUMBER_SESSIONS with : NUMBER_SESSIONS : Number of sessions by spectrum (one IR spectrum is divided into several communication sessions) time_session = ceil(MODE_TIME(COMMAND_MODE_TIME)*332/1000) = 0A level time sampling period MODE_TIME=[1.4,2.8,5.6,11.2] COMMAND_MODE_TIME :AOTF chopping period : 0- 1.4 ms, 1- 2.8 ms, 2- 5.6 ms, 3- 11.2 ms Values of NUMBER_SESSIONS and COMMAND_MODE_TIME are obtained by reading the IR data (see IR label file) WARNING: -------- For the present GEOMETRY files associated to the level 0B - IR data files, the sampling used is the 0A level time sampling period. (= time_session) REMINDER: --------- In level 0A IR data file, a record corresponds to one communication session (one part of a spectrum) from the two detectors. In level 0B IR data file contains all reconstructed spectra of an IR SPICAV observation collected by the two detectors of the infrared channel. All other relevant information (parameters of the command, frequency array, system monitor's values) are also included in the file. For more details on that topic please refeer the SA_VEX_ARCH_001_05.PDF/.ASC. ****************************************************************************** The GEOMETRY directory will contain geometry files associated to the level 0B IR data. The files listed below will be found in this directory. |- [GEOMETRY] A directory containing the data + associated label files | | | |- GEOMINFO.TXT Description of files in this directory | | | | | |-[VENUS] A directory containing VEX SPICAV level 0B IR geometry | | | files associated to data collected during the Venus | | | nominal phase | | | | | |-[VOCP_0001_0022] | | | | | | | |- [DOYxxxx] | | | | | | | | |-- {file(s) *TXT, *.LBL} | | | | | |-[MTP001_0023_0044] | | | | | | | |-[ORBITxxxx] | | | | | | | |-- {file(s) *TXT, *.LBL} | | | Geometry files provided by the SPICAV team will have the following name: SPIV_YYT_nnnnAnn_M_vv_GOXww.DAT where YY 2 letters describing the SPICAV data level (eg. 0A, 1A, 0B, ...) T 1 letter describing the type of data collected (U for UV and R for IR) nnnn 4 digits for the orbit number or Pmmm (P for VOI PHASE and mmm are the doy number) Ann sequence number indicating the order that data were collected for the nnnn orbit (A01, A02,...). M 1 letter describing the type operation mode (eg.H: EARTH, W: MERCURY, E:STAR,S:SUN,L:LIMB, N:NADIR) vv version number of the file X 1 letter describing the content of the file. The value of this letter can be L for a light version of the geometry file (only some main parameters) and F for a full version. ww version number of the software generating the geometry file