Search Results
1–7 of 7 results (0.000 seconds)
-
instrument host:
VENUS EXPRESS
Information about the VENUS EXPRESS instrument host -
investigation:
VENUS EXPRESS
Information about the VENUS EXPRESS investigation -
instrument host:
VENUS EXPRESS
Information about the VENUS EXPRESS instrument host -
investigation:
VENUS EXPRESS
Information about the VENUS EXPRESS investigation -
bundle:
Venus Solar Wind Interactions Data
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. -
collection:
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. -
collection:
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.
Data Sets and Information