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Found 21 dataset(s) matching "vega-2".
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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...
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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...
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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...
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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...
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The longest-lived in-situ measurement platforms at Venus have been the Soviet VEGA balloons in 1985 and the only high-quality pressure/temperature profile in the lowest 10km of the atmosphere is...
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This data set contains Philip Stooke shape models for 243 Ida, 253 Mathilde, 951 Gaspra, comet Halley, J5 Amalthea, J14 Thebe, N7 Larissa, N8 Proteus, S10 Janus, S11 Epimetheus, S16 Prometheus,...
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This data set contains Philip Stooke shape models for 243 Ida, 253 Mathilde, 951 Gaspra, comet Halley, J5 Amalthea, J14 Thebe, N7 Larissa, N8 Proteus, S10 Janus, S11 Epimetheus, S16 Prometheus,...
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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...
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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...
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For the TV SYSTEM, 39 images were sent as a 7-d FITS file with little information in the FITS headers. In addition, to the size of the image (NAXIS1 and NAXIS2), the values for NAXIS3 and NAXIS4...
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For the TV SYSTEM, 39 images were sent as a 7-d FITS file with little information in the FITS headers. In addition, to the size of the image (NAXIS1 and NAXIS2), the values for NAXIS3 and NAXIS4...
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The TVS data from KFKI came in various stages. The initial submission from KFKI was completely replaced in the fall 1992. At that time, additional processed data with aspect and range corrections...
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The TVS data from KFKI came in various stages. The initial submission from KFKI was completely replaced in the fall 1992. At that time, additional processed data with aspect and range corrections...
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The TVS data from Institute Kosmosforschung (IKF) is in various stages. The submission is a single image which was smoothed or transformed by image processing techniques.
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The TVS data from Institute Kosmosforschung (IKF) is in various stages. The submission is a single image which was smoothed or transformed by image processing techniques.
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The PLASMAG-1 instument package included six different sensors: A0 plasma impact detector for measuring neutral particle flux, (manufactured by R. Grard, ESA/ESTEC, Noordwijk, The Netherlands) A1...
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The PLASMAG-1 instument package included six different sensors: A0 plasma impact detector for measuring neutral particle flux, (manufactured by R. Grard, ESA/ESTEC, Noordwijk, The Netherlands) A1...
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The data from IKI for this dataset were received as two binary files containing data taken in all instrument modes. These files were split into separate files for each mode, preserving the...
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The data from IKI for this dataset were received as two binary files containing data taken in all instrument modes. These files were split into separate files for each mode, preserving the...
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The data from MPI for this dataset were received as text files each containing spectra of a single instrument mode (there were several files for most modes). These spectra were reformatted into...
