HDPWS

SolarOrbiter - EPD/STEP - L2 : rates - flux

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

Description
Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates. 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-rates
ResourceHeader
ResourceName
SolarOrbiter - EPD/STEP - L2 : rates - flux
AlternateName
Flux averaged over sectors
ReleaseDate
2024-09-29 23:47:55Z
Description
Solar Orbiter, Level 2 Data, Energetic Particle Detector, SupraThermal Electrons and Protons, Rates. 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
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/J.Rodrigues-Pacheco
InformationURL
Association
AssociationID
AssociationType
PartOf
Note
L2 : rates
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
so-step-rates
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
2020-04-30 00:00:11Z
StopDate
2021-10-22 11:48:29Z
CadenceMin
PT10S
CadenceMax
PT60S
ObservedRegion
Heliosphere.Inner
ObservedRegion
Sun.Corona
Parameter #1
Name
ion flux
ParameterKey
solo_step_mflux
Description
Magnet channel. Uses a permanet magnet to deflect electrons. Measuring only ions (mostly protons)
Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
48
Particle
ParticleQuantity
EnergyFlux
Parameter #2
Name
ion flux unc
ParameterKey
solo_step_munc
Description
Uncertainty in sector averaged magnet channel flux
Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
48
Particle
ParticleQuantity
EnergyFlux
Parameter #3
Name
ion cntrate
ParameterKey
solo_step_mrate
Description
Sector averaged magnet channel count rate
Units
cnts/s
RenderingHints
DisplayType
Spectrogram
Structure
Size
48
Particle
ParticleQuantity
CountRate
Parameter #4
Name
el flux
ParameterKey
solo_step_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
48
Particle
ParticleQuantity
EnergyFlux
Parameter #5
Name
total flux
ParameterKey
solo_step_iflux
Description
Integral channel. Measures all incoming particles
Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
48
Particle
ParticleQuantity
EnergyFlux
Parameter #6
Name
total flux unc
ParameterKey
solo_step_iunc
Description
Uncertainty in sector averaged integral channel flux
Units
1/(s cm^2 sr MeV)
RenderingHints
DisplayType
Spectrogram
Structure
Size
48
Particle
ParticleQuantity
EnergyFlux
Parameter #7
Name
total cntrate
ParameterKey
solo_step_irate
Description
Sector averaged integral channel count rate
Units
cnts/s
RenderingHints
DisplayType
Spectrogram
Structure
Size
48
Particle
ParticleQuantity
CountRate
Parameter #8
Name
quality flag
ParameterKey
solo_step_qf
Description
0: Bad, 1: Known problems, 2: Survey data, 3: Good, 4: Excellent
RenderingHints
DisplayType
TimeSeries
Support
SupportQuantity
DataQuality