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VENUS EXPRESS: ASPERA-4 IMA SWM Solar Wind Moments (CDF)

ResourceID
spase://CNES/NumericalData/CDPP-Archive/VEX/ASPERA4/VEX_ASPERA4_SWM

Description
This data set contains solar wind parameters derived from ion data from the Ion Mass Analyzer (IMA).

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Details

Version:2.4.0

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-Archive/VEX/ASPERA4/VEX_ASPERA4_SWM
ResourceHeader
ResourceName
VENUS EXPRESS: ASPERA-4 IMA SWM Solar Wind Moments (CDF)
DOI
https://doi.org/10.24400/802406/kh9f-bc8k
ReleaseDate
2022-06-06 17:35:00Z
Description
This data set contains solar wind parameters derived from ion data from the Ion Mass Analyzer (IMA).
Acknowledgement
Please acknowledge the Principal Investigator(s) as well as the ESA Planetary Science Archive and the CDPP (Centre des Données de la Physique des Plasmas) when making a publication using the data you are going to download. Principal Investigator(s): S. Barabash (IRF, Kiruna, Sweden)
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://CNES/Person/CDPP-Archive/Stas.Barabash
AccessInformation
RepositoryID
Availability
Online
AccessURL
Name
REGARDS
URL
Description
Access via CNES Data Archive for CDPP
Format
CDF
ProcessingLevel
Calibrated
InstrumentIDs
MeasurementType
EnergeticParticles
TemporalDescription
TimeSpan
StartDate
2006-07-12 00:00:00Z
StopDate
2014-11-27 00:00:00Z
ObservedRegion
Venus.Magnetosphere
Parameter #1
Name
Density
Description
The plasma density.
Units
cm^-3
UnitsConversion
1e6>m^-3
Particle
ParticleType
Ion
Qualifier
Moment
ParticleQuantity
NumberDensity
Parameter #2
Name
Velocity
Description
The plasma velocity.
Units
km/s
UnitsConversion
1e3>m/s
Particle
ParticleType
Ion
Qualifier
Moment
ParticleQuantity
Velocity
Parameter #3
Name
Temperature
Description
The plasma Temperature.
Units
K
Particle
ParticleType
Ion
Qualifier
Moment
ParticleQuantity
Temperature
Parameter #4
Name
Quality flag
Description
The flag parameter indicates: 0) No identified issues, 1) Bad fit, likely EUV or SEP contamination, 2) Too low temperature for the instrument to reliably resolve the Maxwellian 3) IMA was running in a badly suited Post-acceleration (PAC) level. 4) Solar wind observed in partially blocked FOV bin. 5) Solar wind density was smaller than 1 PART/CM**3. All entries are averaged from scan-wise moments with flag = 0, but the flag column is kept for possible future use.
Support
SupportQuantity
DataQuality