HDPWS

Rosetta - IES - electrons - azimuthal spectra : countrate

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Rosetta/IES/ros-elc-az

Description
Electron azimuthal (16 anodes) spectra : Countrates summed over energies and elevations. * Azimuth 180.0-202.5 - Anode #0 * Azimuth 202.5-225.0 - Anode #1 * Azimuth 225.0-247.5 - Anode #2 * Azimuth 247.5-270.0 - Anode #3 * Azimuth 270.0-292.5 - Anode #4 * Azimuth 292.5-315.0 - Anode #5 * Azimuth 315.0-337.5 - Anode #6 * Azimuth 337.5-360.0 - Anode #7 * Azimuth 00.0 - 22.5 - Anode #8 * Azimuth 22.5 - 45.0 - Anode #9 * Azimuth 45.0 - 67.5 - Anode #10 * Azimuth 67.5 - 90.0 - Anode #11 * Azimuth 90.0 -112.5 - Anode #12 * Azimuth 112.5-135.0 - Anode #13 * Azimuth 135.0-157.5 - Anode #14 * Azimuth 157.5-180.0 - Anode #15

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NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Rosetta/IES/ros-elc-az
ResourceHeader
ResourceName
Rosetta - IES - electrons - azimuthal spectra : countrate
AlternateName
electron azimuthal spectra : countrates
ReleaseDate
2017-03-18 00:15:10Z
Description
Electron azimuthal (16 anodes) spectra : Countrates summed over energies and elevations. * Azimuth 180.0-202.5 - Anode #0 * Azimuth 202.5-225.0 - Anode #1 * Azimuth 225.0-247.5 - Anode #2 * Azimuth 247.5-270.0 - Anode #3 * Azimuth 270.0-292.5 - Anode #4 * Azimuth 292.5-315.0 - Anode #5 * Azimuth 315.0-337.5 - Anode #6 * Azimuth 337.5-360.0 - Anode #7 * Azimuth 00.0 - 22.5 - Anode #8 * Azimuth 22.5 - 45.0 - Anode #9 * Azimuth 45.0 - 67.5 - Anode #10 * Azimuth 67.5 - 90.0 - Anode #11 * Azimuth 90.0 -112.5 - Anode #12 * Azimuth 112.5-135.0 - Anode #13 * Azimuth 135.0-157.5 - Anode #14 * Azimuth 157.5-180.0 - Anode #15
Acknowledgement
Principal Investigator : James L. Burch, SwRI
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://SMWG/Person/James.L.Burch
2. CoInvestigator spase://CNES/Person/CDPP-AMDA/Ray.Goldstein
3. DataProducer spase://CNES/Person/CDPP-AMDA/Brad.Trantham

Association
AssociationID
AssociationType
PartOf
Note
electrons
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
ros-elc-az
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
SwRI / ImperialCollege
ProviderResourceName
V02
ProviderProcessingLevel
Uncalibrated
InstrumentIDs
MeasurementType
ThermalPlasma
TemporalDescription
TimeSpan
StartDate
2010-11-29 23:18:19Z
StopDate
2016-09-30 23:58:44Z
Cadence
PT128S
ObservedRegion
Comet
Caveats
Sometimes anode data are combined on board in certain operating modes because of telemetry limitations. In those cases each of the anodes is given identical values (sum/number of anodes). Occasionally the electron data exhibit a signal at narrow energy ranges between 200-2000 eV, appearing as short dashes in spectrograms, as a result of interference from a neighboring instrument (ICA). Anode 11 became noisy shortly after launch and since 16 September 2007 data from that anode have not been downloaded. In those operating modes for which data from 2 or more anodes are combined will result in the absence of data from one or more anodes adjacent to number 11. It was discovered after launch, apparently as a result of a light leak, that when the sun is incident between elevation steps 6 and 7 a high count rate may be seen in anodes 8 - 10.
Parameter #1
Name
e- countrate
ParameterKey
ros_elc_az
Units
s**-1
RenderingHints
DisplayType
Spectrogram
Structure
Size
16
FillValue
-1
Particle
ParticleType
Electron
ParticleQuantity
CountRate