HDPWS

Ulysses - URAP - io torus QTN - electron density

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/ULYSSES/URAP/ulys-urap-dens

Description
The electron density measurements Ne are given in cm-3 and the given acquisition time for each value is dependant on three different measurement methods (flagged by 0,1 or 2). Ne_min and Ne_max stands for errors bars on the density measurements (which are also strongly depending on the measurements methods) The method #0 corresponds to densities deduced from the upper hybrid frequency peak detection, in the HF band of the URAP/RAR receiver (firstly published in Hoang et al., Planet. Space Sci.,Vol. 41, No. 11/12, pp. 1011-1020, 1993, and references therein). The given acquisition time is the elapsed time (UT) of the sweeping receiver at the f_uh peak acquisition. The method #1 corresponds to density obtained by the minimum chi-square fitting of theoritical dispersion curves of Bernstein modes to the experimental dispersion curves derived from the URAP/RAR spectra, Ne and Te being the two free fitted parameters (Moncuquet et al., J. Geophys. Res., 100, 21697-21708 , 1995 and references therein); The given acquisition time for each density measurement is the elapsed time (UT) at mid-time of the whole spectrum acquisition (the acquisition duration of a whole spectrum is 128s). In this case, the determination of Ne and Te are synchronized , but they are not independently determined. The method #2 corresponds to density obtained from detection of Bernstein "fQ" frequencies (Moncuquet et al.,J. Geophys. Res., 102, 2373-2379, 1997 and references therein). The given acquisition time is the elapsed time (UT) of the sweeping receiver at the lowest fQ acquisition.

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NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/ULYSSES/URAP/ulys-urap-dens
ResourceHeader
ResourceName
Ulysses - URAP - io torus QTN - electron density
ReleaseDate
2012-03-06 22:15:53Z
Description
The electron density measurements Ne are given in cm-3 and the given acquisition time for each value is dependant on three different measurement methods (flagged by 0,1 or 2). Ne_min and Ne_max stands for errors bars on the density measurements (which are also strongly depending on the measurements methods) The method #0 corresponds to densities deduced from the upper hybrid frequency peak detection, in the HF band of the URAP/RAR receiver (firstly published in Hoang et al., Planet. Space Sci.,Vol. 41, No. 11/12, pp. 1011-1020, 1993, and references therein). The given acquisition time is the elapsed time (UT) of the sweeping receiver at the f_uh peak acquisition. The method #1 corresponds to density obtained by the minimum chi-square fitting of theoritical dispersion curves of Bernstein modes to the experimental dispersion curves derived from the URAP/RAR spectra, Ne and Te being the two free fitted parameters (Moncuquet et al., J. Geophys. Res., 100, 21697-21708 , 1995 and references therein); The given acquisition time for each density measurement is the elapsed time (UT) at mid-time of the whole spectrum acquisition (the acquisition duration of a whole spectrum is 128s). In this case, the determination of Ne and Te are synchronized , but they are not independently determined. The method #2 corresponds to density obtained from detection of Bernstein "fQ" frequencies (Moncuquet et al.,J. Geophys. Res., 102, 2373-2379, 1997 and references therein). The given acquisition time is the elapsed time (UT) of the sweeping receiver at the lowest fQ acquisition.
Contacts
Role Person StartDate StopDate Note
1. GeneralContact spase://SMWG/Person/Elena.Budnik
Association
AssociationID
AssociationType
PartOf
Note
io torus QTN
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
ulys-urap-dens
Description
Web Service to this product using the HAPI interface.
Format
CSV
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
Description
Access to Data via CDPP/AMDA Web application.
Format
CSV
Format
VOTable
Format
CDF
Format
PNG
Acknowledgement
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
ProviderName
LESIA
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
1992-02-08 15:00:28Z
StopDate
1992-02-08 22:57:28Z
CadenceMin
PT38S
CadenceMax
PT576S
ObservedRegion
Jupiter
Parameter #1
Name
density e-
ParameterKey
ulys_urap_ne
UCD
phys.density;phys.electron
Units
cm-3
RenderingHints
DisplayType
TimeSeries
Particle
ParticleType
Electron
ParticleQuantity
NumberDensity
Parameter #2
Name
density e- min
ParameterKey
ulys_urap_nemin
UCD
phys.density;phys.electron
Units
cm-3
RenderingHints
DisplayType
TimeSeries
Particle
ParticleType
Electron
ParticleQuantity
NumberDensity
Parameter #3
Name
density e- max
ParameterKey
ulys_urap_nemax
UCD
phys.density;phys.electron
Units
cm-3
RenderingHints
DisplayType
TimeSeries
Particle
ParticleType
Electron
ParticleQuantity
NumberDensity
Parameter #4
Name
method
ParameterKey
ulys_urap_method
UCD
meta.code
RenderingHints
DisplayType
TimeSeries
Support
SupportQuantity
Other