Version:2.4.1
NumericalData
ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Rosetta/IES/ros-ion-azimuth
ResourceHeader
ResourceName
azimuthal spectra : eflux
AlternateName
ion azimuthal spectra : dE flux
ReleaseDate
2019-03-19 09:34:08Z
Description
Ion azimuthal (16 anodes) spectra : differential energy flux summed over energies and elevations.
* Azimuth 45 - 90 - Anode #0
* Azimuth 00 - 45 - Anode #1
* Azimuth 315-360 - Anode #2
* Azimuth 310-315 - Anode #3
* Azimuth 305-310 - Anode #4
* Azimuth 300-305 - Anode #5
* Azimuth 295-300 - Anode #6
* Azimuth 290-295 - Anode #7
* Azimuth 285-290 - Anode #8
* Azimuth 280-285 - Anode #9
* Azimuth 275-280 - Anode #10
* Azimuth 270-275 - Anode #11
* Azimuth 225-270 - Anode #12
* Azimuth 180-225 - Anode #13
* Azimuth 135-180 - Anode #14
* Azimuth 90-135 - Anode #15
Acknowledgement
Principal Investigator : James L. Burch, SwRI
Contacts
Association
AssociationID
AssociationType
PartOf
Note
ions
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
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 http://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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.
ProviderName
SwRI
ProviderResourceName
V02
ProviderProcessingLevel
Calibrated
InstrumentIDs
MeasurementType
ThermalPlasma
TemporalDescription
TimeSpan
StartDate
2014-03-25 00:36:27Z
StopDate
2016-09-30 23:58:44Z
CadenceMin
PT128S
CadenceMax
PT1024S
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).
Anodes 13 and 14 are often noisy so caution is recommended when using data from them.
The so-called "fine anodes" (3 - 11) are sometimes combined on board in certain operating modes
because of telemetry limitations. In those cases each of these 9 anodes are given identical values (the
sum/9).
The data from individual fine anodes, when provided, suffer from crosstalk between these anodes and
thus may not be reliable.
It was discovered after launch, apparently as a result of a light leak, that when the sun is incident between
anodes 2 and 3, a high count rate is seen in anode 12. It is also seen in anode 13 when counts in 12 and 13
are combined.
Parameter #1
Name
ion flux
ParameterKey
ros_ion_az_flux
Units
eV/(m**2*s*sr*eV)
RenderingHints
Structure
FillValue
-1
Particle
ParticleType
Ion
ParticleQuantity
EnergyFlux