VEGA2 DUST PARTICLE IMPACT DETECTOR DATA V1.0

공공데이터포털

The SP-2 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 DETECTOR DATA V1.0

공공데이터포털

The SP-2 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 DETECTOR DATA V1.0

공공데이터포털

The SP-2 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.

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.

VEGA2 DUST PARTICLE COUNTER MASS ANALYSER DATA V1.0

공공데이터포털

Encounter data for Vega-2 consisted of two files: DSFAST27 and Dvg2CLN1. The data were submitted by the Univ of Chicago group along with hard copy versions of the operating manual and a preprint of the results.

VEGA2 DUST PARTICLE COUNTER MASS ANALYSER DATA V1.0

공공데이터포털

Encounter data for Vega-2 consisted of two files: DSFAST27 and Dvg2CLN1. The data were submitted by the Univ of Chicago group along with hard copy versions of the operating manual and a preprint of the results.

ULYSSES DUST DETECTION SYSTEM V2.0

공공데이터포털

Dataset Overview ================ This data set contains information on dust the dust environment in interplanetary space within the inner solar system, between Jupiter and the Sun, and at high polar latitudes of the Sun. Both interplanetary and interstellar dust particles have been detected. This information is collected with a dust impact experiment, from which may be inferred direction of motion, mass, velocity and charge (see ULYDINST.CAT). The data presented in this dataset include instrumental readouts, inferred metadata, calibration information and a calendar of events. Specifically:

ULYSSES DUST DETECTION SYSTEM V2.0

공공데이터포털

Dataset Overview ================ This data set contains information on dust the dust environment in interplanetary space within the inner solar system, between Jupiter and the Sun, and at high polar latitudes of the Sun. Both interplanetary and interstellar dust particles have been detected. This information is collected with a dust impact experiment, from which may be inferred direction of motion, mass, velocity and charge (see ULYDINST.CAT). The data presented in this dataset include instrumental readouts, inferred metadata, calibration information and a calendar of events. Specifically:

VEGA2 DUST PARTICLE IMPACT PLASMA DETECTOR DATA V1.0

공공데이터포털

A number of datasets from the VEGA missions were submitted by Dyachkov at IKI as FITS files (binary data) using the GROUPS form or multidimensioned arrays. In addition, little information was provided except for the date, spacecraft, and experiment. Sometimes in the GROUPS parameters (Pvalues), there were experiment parameters such as 'time' indicated and by inference this could be determined to be exposure time versus a clock time. Since there was at least one extensive set of observations (TVS images), that were provided by IKI in this manner and a separate facility (KFKI) with the proper IHW keywords, it was possible to make estimates as to the meaning of 'time' with proper units (seconds).