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Venus Solar Wind Interactions Simulation Output Collection
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 ...

Citiation Information

Author	Brecht, S. H.; Ledvina, S. A.
Title	Venus 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.
Publisher	NASA Planetary Data System
Publication Year	2020

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collection_data_1.0.csv

collection_data_1.0

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This collection contains the simulation output presented in Brecht, S. H. and S. A. Ledvina, An explanation of the nightside

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