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Venus Solar Wind Interactions Data Order Volume Toggle viewing into brief mode
venus-solar-wind-interactions      UNCERTIFIED
This bundle contains the data presented in Brecht, S. H. and S. A. Ledvina, An explanation of the nightside ionospheric structure of Venus, JGR, 2020.
This bundle contains the data presented in Brecht, S. H. and S. A. Ledvina, An explanation of the nightside ionospheric structure of Venus, JGR, 2020.    less ...
Citiation Information
Author Brecht, S. H.; Ledvina, S. A.
TitleVenus Solar Wind Interactions Data
Description This bundle contains the data presented in Brecht, S. H. and S. A. Ledvina, An explanation of the nightside ionospheric structure of Venus, JGR, 2020.
PublisherNASA Planetary Data System
Publication Year 2020
doi https://doi.org/10.17189/1520598
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data
Venus Solar Wind Interactions Data
-
This collection contains the data presented in Brecht, S. H. and S. A. Ledvina, An explanation of the nightside ionospheric structure of Venus, JGR, 2020. The data is stored in ASCII (text) format for easy reading. Units for the results are in the cgs system, densities (cm^-3), magnetic field (Gauss) and lengths (cm). The magnetic field can be found in the B-GradPe.dat.gz. The O+ density is designated by 2s in the file name. The O2+ density is designated by 3s in the file name. There are 2 types of data files, *.dat.gz and *.sdat.gz. The *.dat files contain the data stored on the Cartesian grid, while the *.sdat contains the data stored on the spherical mesh.
document
Venus Solar Wind Interactions Document Collection
This document collection contains a User Guide file that describes the data in the Venus Solar Wind Interactions Data bundle, which contains the data presented in Brecht, S. H. and S. A. Ledvina, An explanation of the nightside ionospheric structure of Venus, JGR, 2020.
bundle_venus_solar_wind_interactions_v1.0
This bundle contains the data presented in
Brecht, S. H. and S. A. Ledvina, An explanation of the nightside
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