PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "2015-04-29 Creation; 2016-08-02 SBN:T.Barnes Edits reflecting V6.0;" RECORD_TYPE = STREAM OBJECT = DATA_SET DATA_SET_ID = "RO-SS-RPCMAG-2-PRL-RAW-V5.0" OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "GLASSMEIERETAL2007B" END_OBJECT = DATA_SET_REFERENCE_INFORMATION OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "ROSETTA-ORBITER SW RPCMAG 2 PRL RAW V5.0" DETAILED_CATALOG_FLAG = "N" DATA_OBJECT_TYPE = TABLE START_TIME = 2014-03-23T22:02:19 STOP_TIME = 2014-11-21T23:58:47 DATA_SET_RELEASE_DATE = 2015-05-20 PRODUCER_FULL_NAME = "INGO RICHTER" ABSTRACT_DESC = "This dataset contains EDITED RAW DATA of the PRELANDING Phase from March 23 until November 21, 2014 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). Version V5.0 is the first version being released." DATA_SET_DESC = " Archive Note ============ This data set, RO-SS-RPCMAG-2-PRL-RAW-V5.0, was in lien resolution and abandoned with the liens left unresolved. The next version of this data set, RO-SS-RPCMAG-2-PRL-RAW-V6.0, has all liens from the prior version V5.0 resolved. Data Set Overview ================= The data from the ROSETTA PLASMA CONSORTIUM (RPC) Fluxgate Magnetometer(MAG)was submitted by Ingo Richter (TM) for the RPCMAG team. The PI of the team is Karl-Heinz Glassmeier. The data have been measured during the PRELANDING Phase of ROSETTA. Included are the following sub-phases: -the Rendezvous Manoeuvre 2 (RVM2) between January and September 2014 -the Post Hibernation Commissioning in March/April 2014 -the Near Comet Drift Phase (NCD) between March and July 2014 -the Far Approach Trajectory (FAT)between July and August 2014 -the Comet Characterization Phase (CC) between August and September -the Global Mapping Phase/Close Observation Phase (GMP/COP) between September and October 2014 -the Landing and First Science Sequence (LD/FSS) between October and November 2014 The several Landings of PHILAE happened on November 12, 2014. All magnetic field data are edited raw data. That means the data represent the 3 components of the magnetic field measured in counts of the used 20 bit ADC. Data are given in instrument coordinates. Neither any filtering nor any calibration has been applied to the data. Any s/c generated noise and s/c caused residual magnetic fields are not eliminated. The data are sorted by the sensor (OB: outboard sensor, IB: inboard sensor)and the measurement mode (M1..M6). They can uniquely be identified by their file names. Normally the OB is the Primary (Pri) and the IB is the Secondary (Sec) sensor. However, this order can be toggled by TCs. This feature has been tested especially during the commissioning phases. In cases were the PRIMARY and SECONDARY sensor were toggled the individual data files (OB/IB) will contain data measured with different sampling rates according to the actual sampling rates of the PRIMARY and SECONDARY sensors. Refer to the MODE DESCRIPTION table below. The actual sampling rate is the only indicator showing which sensor is the primary and which is the secondary one. REMARK: ======= Due to strong magnetic disturbance by the ORBITER and by the LANDER Philae, the magnetic field data are influenced by s/c generated magnetic fields. The source of these disturbance is manifold: - transient currents flowing on the spacecraft - Heater pulses - Thruster related magnetic field - Reaction wheel signatures - etc. Due to the complexity of these circumstances a proper data cleaning is an ongoing task. Thus the data of the present dataset still contain the mentioned disturbance signatures. Therefore, any use of the data for scientific research has to be done under consideration of these disturbances. Mode description: ================= MODE SAMPLE RATE PACKET PERIOD PACKET LENGTH VECTOR RATE Minimum Mode M1 1/32 Hz 1024 s 32 Pri Vec 0.03125 vec/s 1 Sec Vec 0.000976 vec/s Normal Mode M2 1 Hz 32 s 32 Pri Vec 1 vec/s 1 Sec Vec 0.03125 vec/s Burst Mode M3 20 Hz 16 s 320 Pri Vec 20 vec/s 16 Sec Vec 1 vec/s Medium Mode M4 5 Hz 32 s 160 Pri Vec 5 vec/s 1 Sec Vec 0.03125 vec/s Low Mode M5 0.25 Hz 128 s 32 Pri Vec 0.25 vec/s 1 Sec Vec 0.007812 vec/s Test Mode M6 20 Hz 16 s 320 Pri Vec 20 vec/s 1 Sec Vec 0.0625 vec/s HK Mode 32 s 8 words 0.03125 vec/s FILENAME CONVENTION & Mode Coding =================================== Due to operational constraints it might happen that the instrument mode or the primary sensor has to be switched during a specific observation. The actual mode and the primary sensor of the instrument can easily be identified by analyzing the filename of the actual data files. The complete filename convention is listed in the EAICD, chapter 3.1.4. The filenames for EDITED and CALIBRATED data are coded as follows: ___. RPCMAG yymmddThhmm RAW IB M1..M6 LBL CLA OB TAB CLB CLC Example: RPCMAG040528T1230_RAW_OB_M3.LBL RPCMAG040528T1230_RAW_OB_M3.TAB The filenames for Housekeeping data are coded as follows: _. RPCMAG yymmddThhmm HK LBL TAB Example: RPCMAG040528T1230_HK.LBL RPCMAG040528T1230_HK.TAB Geometry Information - Coordinate System ======================================== The geometry items SC_SUN_POSITION_VECTOR SC_TARGET_POSITION_VECTOR SC_TARGET_VELOCITY_VECTOR provided in the label of the data product are relative to the ECLIPJ2000 frame. This reference frame is built up by Ecliptic Coordinates related to Equinox of Epoch J2000. Orientation: X: Pointing from SUN to Vernal Equinoxe, Y: perpendicular to X in Ecliptic Plane, Z: Perpendicular to Ecliptic plane, pointing up The items SUB_SPACECRAFT_LATITUDE SUB_SPACECRAFT_LONGITUDE are given in the PLANETOCENTRIC coordinate system. All these geometry parameters are computed at time t=START_TIME. Distances are given in km, angles in degrees. " CONFIDENCE_LEVEL_NOTE = "This data set has the same structure as the former RPCMAG datasets obtained between 2004 and 2011. Those datasets have been reviewed by two independent teams in Spring 2012. After these reviews the datasets had been accepted by the Planetary Science Archive(PSA)of the ESA and by the Planetary Data System(PDS) of NASA for long-term archiving. The data have been processed on best effort basis according to the procedures described in RO-IGEP-TR0028: Step by Step Calibration Procedure. Quality flags are attached for CALIBRATED and RESAMPLED data as described in the EAICD RO-IGEP-TR0009. Both of these are available in the DOCUMENT directory." ARCHIVE_STATUS = "SAFED" CITATION_DESC = "Glassmeier K.-H., Richter I., Koenders C., Goetz C., Eichelberger. H, Cupido E., ROSETTA RPCMAG PRELANDING PHASE (PRL) EDITED RAW DATA RECORD V5.0, RO-SS-RPCMAG-2-PRL-EDITED-V5.0, ESA Planetary Science Archive and NASA Planetary Data System, 2015" DATA_SET_COLLECTION_MEMBER_FLG = "N" DATA_SET_TERSE_DESC = "This dataset contains RPCMAG EDITED RAW DATA of the PRELANDING Phase. Included are data 23.3.2014 - 21.11.2014." END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = "CHECKOUT" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_TARGET TARGET_NAME = "SOLAR WIND" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_TARGET TARGET_NAME = "67P/CHURYUMOV-GERASIMENKO 1 (1969 R1)" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_MISSION MISSION_NAME = "INTERNATIONAL ROSETTA MISSION" END_OBJECT = DATA_SET_MISSION OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = RO INSTRUMENT_ID = RPCMAG END_OBJECT = DATA_SET_HOST END_OBJECT = DATA_SET END