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SolarOrbiter - EPD/STEP - L2 : main - flux

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-main

Description

Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Main product.

      STEP is designed to measure electrons and ions in the suprathermal energy range (280 keV). To 
      allow for the separation of electrons and ions, STEP has 2 different channels, each equipped with its 
      own solid state detectors for detecting particles: 
      * Magnet channel. Uses a permanent magnet to deflect electrons, measuring only ions (mostly protons). 
      * Integral channel. Measures all incoming particles.
      
      The electron flux is recovered by subtracting the magnet channel measurements from the integral 
      channel ones. Each channel is divided in 15 sectors, disposed in 3 rows of 5 pixels, providing 
      directional information of the incoming particles within the field of view. An additional pixel, not directly 
      exposed to the incoming flux, measures the cosmic ray background.

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Details

Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-step-main
ResourceHeader
ResourceName
SolarOrbiter - EPD/STEP - L2 : main - flux
AlternateName
Flux averaged over sectors
ReleaseDate
2024-09-29 23:56:42Z
Description

Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Main product.

      STEP is designed to measure electrons and ions in the suprathermal energy range (280 keV). To 
      allow for the separation of electrons and ions, STEP has 2 different channels, each equipped with its 
      own solid state detectors for detecting particles: 
      * Magnet channel. Uses a permanent magnet to deflect electrons, measuring only ions (mostly protons). 
      * Integral channel. Measures all incoming particles.
      
      The electron flux is recovered by subtracting the magnet channel measurements from the integral 
      channel ones. Each channel is divided in 15 sectors, disposed in 3 rows of 5 pixels, providing 
      directional information of the incoming particles within the field of view. An additional pixel, not directly 
      exposed to the incoming flux, measures the cosmic ray background.
Acknowledgement
See http://espada.uah.es/epd/EPD_data.php
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://CNES/Person/CDPP-AMDA/J.Rodrigues-Pacheco
InformationURL
Association
AssociationID
AssociationType
PartOf
Note
L2 : main
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
so-step-main
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
http://soar.esac.esa.int/soar
ProviderResourceName
epd-step-rates
InstrumentIDs
MeasurementType
EnergeticParticles
TemporalDescription
TimeSpan
StartDate
2021-10-22 11:38:20Z
StopDate
2024-05-31 23:59:59Z
CadenceMin
PT1S
CadenceMax
PT10S
ObservedRegion
Heliosphere.Inner
ObservedRegion
Sun.Corona
Parameter #1
Name
ion flux
ParameterKey
solo_stepmain_mflux
Description

Particle intensities in magnet channel (ions) averaged for all pixels

Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
32
Particle
ParticleQuantity
EnergyFlux
Parameter #2
Name
ion flux unc
ParameterKey
solo_stepmain_munc
Description

Uncertainty in magnet channel flux averaged for all pixels

Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
32
Particle
ParticleQuantity
EnergyFlux
Parameter #3
Name
el flux
ParameterKey
solo_stepmain_eflux
Description

The electron flux is recovered by subtracting the magnet channel measurements from the integral channel ones

Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
32
Particle
ParticleQuantity
EnergyFlux
Parameter #4
Name
total flux
ParameterKey
solo_stepmain_iflux
Description

Particle intensities in integral channel (ions + electrons) averaged for all pixels

Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
32
Particle
ParticleQuantity
EnergyFlux
Parameter #5
Name
total flux unc
ParameterKey
solo_stepmain_iunc
Description

Uncertainty in integral channel flux averaged for all pixels

Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
32
Particle
ParticleQuantity
EnergyFlux
Parameter #6
Name
quality flag
ParameterKey
solo_stepmain_qf
Description

0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent

RenderingHints
DisplayType
TimeSeries
Support
SupportQuantity
DataQuality