Collection Information
|
IDENTIFIER |
urn:nasa:pds:venus-solar-wind-interactions:data::1.0
|
NAME |
Venus Solar Wind Interactions Data
|
TYPE |
Data
|
DESCRIPTION |
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.
|
SEARCH/ACCESS DATA |
Venus Solar Wind Interactions Online
|
|
|
Citation |
DIGITAL OBJECT IDENTIFIER (DOI) |
10.17189/1520598 (from parent bundle)
|
AUTHOR LIST |
Brecht, S. H.; Ledvina, S. A.
|
EDITOR LIST |
|
PUBLICATION YEAR |
2020
|
DESCRIPTION |
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.
|
|
|
Context |
START DATE TIME |
1965-01-01T12:00:00.000Z
|
STOP DATE TIME |
N/A (ongoing)
|
LOCAL MEAN SOLAR TIME |
|
LOCAL TRUE SOLAR TIME |
|
SOLAR LONGITUDE |
|
PRIMARY RESULT PURPOSE |
SCIENCE
|
PRIMARY RESULT PROCESSING LEVEL |
Derived
|
PRIMARY RESULT DESCRIPTION |
This is simulation data
|
PRIMARY RESULT WAVELENGTH RANGE |
|
PRIMARY RESULT DOMAIN |
|
PRIMARY RESULT DISCIPLINE NAME |
|
INVESTIGATION |
PIONEER VENUS
VENUS EXPRESS
|
OBSERVING SYSTEM |
Pioneer Venus
Venus Express
|
OBSERVING SYSTEM COMPONENT |
Pioneer Venus Orbiter
Venus Express
Computer Simulation
|
TARGET |
VENUS
SOLAR WIND
|
REFERENCES |
|