HPDE.io

pitch-angle distribution

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/EPS/mess-eps-spec

Description

The particle measurements are averaged in 120-second bins.
Pitch angle bins are 11.25 degrees wide, and run from 0 to 180 degrees.

            Please note that the D03 detector on EPS has a very high background and is 
            not useable for any science data product.

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Details

Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MESSENGER/EPS/mess-eps-spec
ResourceHeader
ResourceName
pitch-angle distribution
ReleaseDate
2019-06-11 16:04:45Z
Description

The particle measurements are averaged in 120-second bins.
Pitch angle bins are 11.25 degrees wide, and run from 0 to 180 degrees.

            Please note that the D03 detector on EPS has a very high background and is 
            not useable for any science data product.
Contacts
RolePersonStartDateStopDateNote
1.DataProducerspase://SMWG/Person/George.Ho
InformationURL
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.
ProcessingLevel
Calibrated
ProviderName
PDS
ProviderResourceName
MESS-E_V_H_SW-EPPS-3-EPS-DDR-V1.0/EPS_PA_DAILY_SPECTROGRAM
InstrumentIDs
MeasurementType
EnergeticParticles
TemporalDescription
TimeSpan
StartDate
2011-03-23 00:00:00Z
StopDate
2015-04-30 23:59:58Z
Cadence
PT120S
ObservedRegion
Mercury
Caveats
EPS PDS data products are derivate from the “Shaped” channel on EPS which is an integrated (hardware) channel. The hardware channel responded to all particles (ion and electron) that are above the threshold (~30 keV). Our experience at Mercury’s magnetosphere is that the primary particles are mostly energetic electrons. Please note that the D03 detector on the EPS has a very high background and is not useable for any of these science data products.
Parameter #1
Name
countrate
ParameterKey
mes_eps_pad
Units
cnts/s
RenderingHints
DisplayType
Spectrogram
Structure
Size
16
Particle
ParticleType
Electron
ParticleQuantity
EnergyFlux