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Venus Solar Wind Interactions Simulation Output Collection Order Volume Toggle viewing into brief mode
venus-solar-wind-interactions      UNCERTIFIED
This collection contains the simulation output 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     more ...
This bundle contains the simulation output 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 Simulation Output Collection
Description This collection contains the simulation output 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.
PublisherNASA Planetary Data System
Publication Year 2020
Top/ data / click here to download folders and files
B-GradPe.dat
B-SGrid-GradPe.sdat
D-SGrid-GradPe.sdat
Den2s-GradPe.dat
Den2s-NoGradPe.dat
Den3s-GradPe.dat
Den3s-NoGradPe.dat
collection_data_1.0.csv
collection_data_1.0
Start Time: Stop Time:
This collection contains the simulation output presented in
Brecht, S. H. and S. A. Ledvina, An explanation of the nightside
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