mvn-euv-mod.xml
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<?xml version="1.0" encoding="UTF-8"?>
<Spase xmlns="http://www.spase-group.org/data/schema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2.4.1.xsd">
<Version>2.4.1</Version>
<NumericalData>
<ResourceID>spase://CNES/NumericalData/CDPP-AMDA/MAVEN/EUV/mvn-euv-mod</ResourceID>
<ResourceHeader>
<ResourceName>modelled EUV flux</ResourceName>
<ReleaseDate>2024-09-02T02:32:53Z</ReleaseDate>
<Description> Extreme UltraViolet (EUV) modelled 1 minute irradiances in 1-nm bins
from 0 -190 nm. See Eparvier et al, Space Research, 195, 203-301 2015.
This dataset contains solar irradiance spectra in 1-nm bins from 0-190 nm.
The spectra are generated based upon the Flare Irradiance Spectra Model -
Mars (FISM-M) using the EUV calibrated band irradiance and interpolated
Earth-based solar indices and measurements as proxies.
</Description>
<Acknowledgement> Principal Investigator : Frank Eparvier, LASP, Colorado
</Acknowledgement>
<Contact>
<PersonID>spase://CNES/Person/CDPP-AMDA/Frank.Eparvier</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<InformationURL>
<Name>Flare Irradiance Spectral Model (FISM): Daily component algorithms and results - Chamberlin, Phillip C.; Woods, Thomas N.; Eparvier, Francis G. - 2017</Name>
<URL>https://doi.org/10.1029/2007SW000316</URL>
<Description>
</Description>
</InformationURL>
<InformationURL>
<Name>EUV web page, Summary sheet </Name>
<URL>http://lasp.colorado.edu/home/maven/science/instrument-package/lpw/extreme-ultraviolet-euv-monitor/</URL>
<Description>
</Description>
</InformationURL>
</ResourceHeader>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>CDPP/AMDA HAPI Server</Name>
<URL>https://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<ProductKey>mvn-euv-mod</ProductKey>
<Description>Web Service to this product using the HAPI interface.</Description>
</AccessURL>
<Format>CSV</Format>
<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.</Acknowledgement>
</AccessInformation>
<AccessInformation>
<RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
<Availability>Online</Availability>
<AccessRights>Open</AccessRights>
<AccessURL>
<Name>CDPP/AMDA Web application</Name>
<URL>https://amda.cdpp.eu</URL>
<Description>Access to Data via CDPP/AMDA Web application.</Description>
</AccessURL>
<Format>CSV</Format>
<Format>VOTable</Format>
<Format>CDF</Format>
<Format>PNG</Format>
<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.</Acknowledgement>
</AccessInformation>
<ProviderName>PDS</ProviderName>
<ProviderResourceName>maven-euv-modelled/minute</ProviderResourceName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/MAVEN/EUV</InstrumentID>
<MeasurementType>ThermalPlasma</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2014-10-19T00:00:00Z</StartDate>
<StopDate>2024-05-14T23:58:58Z</StopDate>
</TimeSpan>
<Cadence>PT60S</Cadence>
</TemporalDescription>
<ObservedRegion>Mars</ObservedRegion>
<Caveats>
Data flag:
* 0 : uses best MAVEN proxies,
* 1 : uses lower quality or partial MAVEN proxies,
* 2 : uses no MAVEN proxies but best extrapolated Earth proxies
* 3 : uses no MAVEN proxies AND poor quality Earth proxies.
</Caveats>
<Parameter>
<Name>irradiance flux</Name>
<ParameterKey>mav_euv_fluxm</ParameterKey>
<Units>Watts/m^2/nm</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>190</Size>
</Structure>
<Wave>
<WaveType>Photon</WaveType>
<WaveQuantity>EnergyFlux</WaveQuantity>
</Wave>
</Parameter>
<Parameter>
<Name>irradiance flux uncertainty</Name>
<ParameterKey>mav_euv_deltam</ParameterKey>
<Units>%</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Structure>
<Size>190</Size>
</Structure>
<Support>
<SupportQuantity>Other</SupportQuantity>
</Support>
</Parameter>
<Parameter>
<Name>quality flag</Name>
<ParameterKey>mav_euv_flagm</ParameterKey>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Support>
<SupportQuantity>Other</SupportQuantity>
</Support>
</Parameter>
</NumericalData>
</Spase>