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VEGA1 HALLEY FLYBY MAGNETOMETER DATA
On MARCH 6, 1986, AT 7:20:06 UT, the Vega spacecraft passed the nucleus of comet Halley at a distance of 8,890 km with a relative velocity of 78 km/s. The magnetic field experiments MISCHA carried four fluxgate sensors, with three sensors mounted on a boom at the end of the solar panels and the fourth sensor mounted one meter closer. During the cruise phase, the TRASSA-1 mode of the instrument (1 vector/2.5 min) was used. The sensors were switched to the TRASSA-2 mode (1 vector/min) during the flyby which started roughly two days before the encounter. From 3 h before closest approach (CA) until 1 hour after CA, the HS-mode (1 vector/6s) and the DT-mode (1 vector/100ms) was used [DELVAETAL1991].
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VEGA1 HALLEY FLYBY MAGNETOMETER DATA
공공데이터포털
On MARCH 6, 1986, AT 7:20:06 UT, the Vega spacecraft passed the nucleus of comet Halley at a distance of 8,890 km with a relative velocity of 78 km/s. The magnetic field experiments MISCHA carried four fluxgate sensors, with three sensors mounted on a boom at the end of the solar panels and the fourth sensor mounted one meter closer. During the cruise phase, the TRASSA-1 mode of the instrument (1 vector/2.5 min) was used. The sensors were switched to the TRASSA-2 mode (1 vector/min) during the flyby which started roughly two days before the encounter. From 3 h before closest approach (CA) until 1 hour after CA, the HS-mode (1 vector/6s) and the DT-mode (1 vector/100ms) was used [DELVAETAL1991].
VEGA1 CRUISE MAGNETOMETER DATA
공공데이터포털
On Dec 15, 1984, the Vega spacecraft was launched to first flyby Venus at which time landers were released and then continue to a flyby of Halley. The magnetic field experiments MISCHA carried four fluxgate sensors, with three sensors mounted on a boom at the end of the solar panels and the fourth sensor mounted one meter closer. During the cruise phase, the TRASSA-1 mode of the instrument (1 vector/2.5 min) was used. The sensors were switched to the TRASSA-2 mode (1 vector/min) during the flyby which started roughly two days before the encounter. From 3 h before closest approach (CA) until 1 hour after CA, the HS-mode 1 vector/6s) and the DT-mode (1 vector/100ms) was used [DELVAETAL1991].
ROSETTA-ORBITER 67P RPCMAG 2 ESC1 RAW V6.0
공공데이터포털
This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) of the COMET ESCORT1 Phase from November 22, 2014 until March 10, 2015 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). The current version of the dataset is V6.0
ROSETTA-ORBITER 67P RPCMAG 2 ESC2 RAW V6.0
공공데이터포털
This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) of the COMET ESCORT 2 Phase from March 11 until June 30, 2015 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). The current version of the dataset is V6.0
ROSETTA-ORBITER 67P RPCMAG 2 ESC2 RAW V9.0
공공데이터포털
This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) of the COMET ESCORT 2 Phase from March 11, 2015 until June 30, 2015 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). The current version of the dataset is V9.0. The difference to the datasets of earlier versions is mainly a significantly improved sensor temperature model, more detailed documentation about magnetic disturbance sources, more data handling information for the user and also an improved quality flagging system. This applies mainly to CALIBRATED and RESAMPLED datasets. The RAW dataset, however, has been updated as well in order provide all datasets at the same stage, although RAW data proper did not change.
ROSETTA-ORBITER 67P RPCMAG 2 ESC4 RAW V9.0
공공데이터포털
This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) of the COMET ESCORT 4 Phase from October 21, 2015 until January 12, 2016 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). The current version of the dataset is V9.0. The difference to the datasets of earlier versions is mainly a significantly improved sensor temperature model, more detailed documentation about magnetic disturbance sources, more data handling information for the user and also an improved quality flagging system. This applies mainly to CALIBRATED and RESAMPLED datasets. The RAW dataset, however, has been updated as well in order provide all datasets at the same stage, although RAW data proper did not change.
ROSETTA-ORBITER 67P RPCMAG 2 ESC4 RAW V6.0
공공데이터포털
This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) of the COMET ESCORT 4 Phase from October 21, 2015 until January 12, 2016 of the ROSETTA orbiter magnetometer RPCMAG. Observations are done in the vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). The current version of the dataset is V6.0, the first being archived.
VEGA1 DUST PARTICLE IMPACT PLASMA DETECTOR DATA V1.0
공공데이터포털
The SP-1 experiment on Vega spacecraft was intended for studying the spatial and mass distributions of dust particles in the cometary coma over the mass range 1.e-16 to 1.e-6 g. Covering such a broad mass range was made possible by using sensors of two types, namely, impact plasma and acoustic.
VEGA1 DUST PARTICLE IMPACT PLASMA DETECTOR DATA V1.0
공공데이터포털
The SP-1 experiment on Vega spacecraft was intended for studying the spatial and mass distributions of dust particles in the cometary coma over the mass range 1.e-16 to 1.e-6 g. Covering such a broad mass range was made possible by using sensors of two types, namely, impact plasma and acoustic.
ROSETTA-ORBITER 67P NAVCAM 3 COMET ESCORT 1 MTP010 V1.0
공공데이터포털
This dataset contains ROSETTA NAVCAM RADIOMETRICALLY CALIBRATED DATA of the COMET ESCORT 1 MTP010 Phase from 22 Nov. 2014, 04:19:32 to 19 Dec. 2014, 22:35:03 when at the vicinity of target 67P/CG.