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://cdpp.irap.omp.eu/AMDA-NG/public/schemas/spase-amda-1_2_0.xsd">
<Version>2.2.6</Version>
<NumericalData>
<ResourceID>spase://CDPP/NumericalData/AMDA/MAVEN/EUV/mvn-euv-mod</ResourceID>
<ResourceHeader>
<ResourceName>modelled EUV flux</ResourceName>
<ReleaseDate>2015-10-12T10:48:29Z</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 irrandiance and interpolated
Earth-based solar indices and measurements as proxies.
</Description>
<Acknowledgement> Principal Investigator : Frank Eparvier, LASP, Colorado
</Acknowledgement>
<Contact>
<PersonID>spase://CDPP/Person/Frank.Eparvier</PersonID>
<Role>PrincipalInvestigator</Role>
</Contact>
<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>AMDA at CDPP</Name>
<URL>
http://amda.cdpp.eu
</URL>
</AccessURL>
<Format>Text.ASCII</Format>
<Acknowledgement>AMDA is a science analysis system provided by the Centre de Donnees de la
Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and
Universite Paul Sabatier, Toulouse
</Acknowledgement>
</AccessInformation>
<ProviderName>PDS</ProviderName>
<ProviderResourceName>maven-euv-modelled/minute</ProviderResourceName>
<InstrumentID>spase://CDPP/Instrument/AMDA/MAVEN/EUV</InstrumentID>
<MeasurementType>ThermalPlasma</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2014-10-19T00:00:00Z</StartDate>
<StopDate>2017-05-14T23:59:00Z</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>
<Description/>
<Ucd/>
<Units>Watts/m^2/nm</Units>
<UnitsConversion/>
<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>
<Description/>
<Ucd/>
<Units>%</Units>
<UnitsConversion/>
<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>
<Description/>
<Ucd/>
<Units/>
<RenderingHints>
<DisplayType>TimeSeries</DisplayType>
</RenderingHints>
<Support>
<SupportQuantity>Other</SupportQuantity>
</Support>
</Parameter>
</NumericalData>
</Spase>