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Wind Waves RAD1_L3A : Direction Finding Data (Unpolarized Source Assumption)

ResourceID
spase://CNES/NumericalData/CDPP-Archive/Wind/WAVES/WIND_WAVES_RAD1_L3A

Description
This data set contains Wind Waves RAD1 direction-finding data. Direction-finding inversion method has been applied on RAD1_L2 high resolution data to derive characteristics of radio emissions. The method is based on the work by Manning and Fainberg, Space Science Instrumentation, 1980. It returns the absolute flux density (in W/m^2/Hz) of the radio source, as well as the azimuth, and the elevation angles (in degrees) in a RTN reference frame centered on the Wind spacecraft. The method is only valid under the following criteria: * Radio source is unpolarized * Radio source has an uniform brightness * Radio source signal remains constant at a given frequency over a spacecraft rotation (~3sec) * Short antenna dipole assumption is valid * Z axial antenna is not tilted Absolute flux density is calibrated using radio galaxy method (see Zaslavsky et al., 2011. DOI 10.1029/2010RS004464). Caveat: Level 3 df data are computed with the following assumptions : (i) incoming wave properties do not change during a spacecraft rotation (~3 seconds)parameter set, (ii) radio sources are unpolarized (U=V=Q=0), (iii) galaxy radio emission is not subtracted, (iv) radio sources have an uniform brightness distribution, (v) Z antennas are not tilted

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Version:2.4.0

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-Archive/Wind/WAVES/WIND_WAVES_RAD1_L3A
ResourceHeader
ResourceName
Wind Waves RAD1_L3A : Direction Finding Data (Unpolarized Source Assumption)
DOI
https://doi.org/10.24400/802406/mbdb-0ep4
ReleaseDate
2022-09-01 16:55:14Z
Description
This data set contains Wind Waves RAD1 direction-finding data. Direction-finding inversion method has been applied on RAD1_L2 high resolution data to derive characteristics of radio emissions. The method is based on the work by Manning and Fainberg, Space Science Instrumentation, 1980. It returns the absolute flux density (in W/m^2/Hz) of the radio source, as well as the azimuth, and the elevation angles (in degrees) in a RTN reference frame centered on the Wind spacecraft. The method is only valid under the following criteria: * Radio source is unpolarized * Radio source has an uniform brightness * Radio source signal remains constant at a given frequency over a spacecraft rotation (~3sec) * Short antenna dipole assumption is valid * Z axial antenna is not tilted Absolute flux density is calibrated using radio galaxy method (see Zaslavsky et al., 2011. DOI 10.1029/2010RS004464). Caveat: Level 3 df data are computed with the following assumptions : (i) incoming wave properties do not change during a spacecraft rotation (~3 seconds)parameter set, (ii) radio sources are unpolarized (U=V=Q=0), (iii) galaxy radio emission is not subtracted, (iv) radio sources have an uniform brightness distribution, (v) Z antennas are not tilted
Acknowledgement
Data provided are publicly available. If used in presentations or publications, please acknowledge Wind/Waves Investigation (K. Issautier and K. Goetz). We recommend the data users to contact the Wind/Waves team early in their study. For reporting purposes, we request bibliography information for any publication, etc., using these data. Please send information on the use of this data to: K. Issautier (PI). We suggest to add the following lines into the acknowledgments: The authors acknowledge CNES (Centre National d'Etudes Spatiales), CNRS (Centre National de la Recherche Scientifique), and Observatoire de Paris for support to the Wind/Waves team and the CDPP (Centre de Données de la Physique des Plasmas) for the provision of the Wind/Waves data. The following paper should also be used to reference: Bougeret et al, Space Science Reviews, 1995, doi: 10.1007/BF00751331
Contacts

AccessInformation
RepositoryID
Availability
Online
AccessURL
Name
REGARDS
URL
Description
Access via CNES Data Archive for CDPP
Format
CDF
ProcessingLevel
Calibrated
ProviderProcessingLevel
3
InstrumentIDs
MeasurementType
Waves.Passive
MeasurementType
Spectrum
TemporalDescription
TimeSpan
StartDate
1994-11-10 00:00:00Z
StopDate
2022-02-28 00:00:00Z
ObservedRegion
Heliosphere.NearEarth
Parameter #1
Name
Sequential sweep number
Description
Sequential sweep number in the file, starting from the first sweep of the current day
Support
SupportQuantity
Other
Parameter #2
Name
Frequency
Description
Frequency of analysis
Units
kHz
UnitsConversion
1e3>Hz
Support
SupportQuantity
Other
Parameter #3
Name
Sequential number in parent L2 data file
Description
Sequential number in parent L2 data file
Support
SupportQuantity
Other
Parameter #4
Name
Flux density
Description
Absolute flux density measured at the antennas (receiver background removed) : Stokes parameter I
Units
W/m^2/Hz
Wave
WaveType
PlasmaWaves
WaveQuantity
StokesParameters
Parameter #5
Name
Wave vector elevation
Description
Elevation of the wave vector in the RTN reference frame centered on Wind spacecraft
Units
degree
UnitsConversion
0.0174532925>rad
Support
Qualifier
DirectionAngle.ElevationAngle
SupportQuantity
Orientation
Parameter #6
Name
Wave vector azimuth
Description
Azimuth of the wave vector in the RTN reference frame centered on Wind spacecraft
Units
degree
UnitsConversion
0.0174532925>rad
Support
Qualifier
DirectionAngle.AzimuthAngle
SupportQuantity
Orientation
Parameter #7
Name
Radio source angular radius
Description
Radio source angular radius, assuming an uniform brightness distribution.
Units
degree
UnitsConversion
0.0174532925>rad
Support
SupportQuantity
Other
Parameter #8
Name
Signal modulation rate
Description
Signal modulation rate
Support
SupportQuantity
Other