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    <ResourceID>spase://NASA/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M</ResourceID>
    <NamingAuthority>NASA</NamingAuthority>
    <ResourceType>NumericalData</ResourceType>
    <ResourceHeader>
      <ResourceName>STEREO-B IMPACT (In-Situ Measurements of Particles and CME Transients) Solar Electron Proton Telescope (SEPT) 1-min Level 1 Electron and Proton Spectra</ResourceName>
      <DOI>https://doi.org/10.48322/y2fy-vb66</DOI>
      <ReleaseDate>2025-12-04T13:31:38Z</ReleaseDate>
      <RevisionHistory>
        <RevisionEvent>
          <ReleaseDate>2021-04-27T15:38:11</ReleaseDate>
          <Note>Only known prior ReleaseDate of the metadata</Note>
        </RevisionEvent>
        <RevisionEvent>
          <ReleaseDate>2023-07-30T12:34:56.789</ReleaseDate>
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        <RevisionEvent>
          <ReleaseDate>2025-10-03T10:49:14Z</ReleaseDate>
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        <RevisionEvent>
          <ReleaseDate>2025-12-04T13:31:38Z</ReleaseDate>
          <Note>Added MetadataRightsList and RightsList(s). Updated to 2.7.1. ZCB</Note>
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      <Description>The IMPACT Solar Electron Proton Telescope (SEPT) Level 1 data consist of electron and proton fluxes from each of 32 energy bands that span ~20 keV to 2000(electrons) or 7000(protons) keV. These spectra are determined each minute, in each of 4 directions with 60 deg fields of view (parallel and anti-parallel to the Parker magnetic field direction, and northward and southward from the ecliptic plane.</Description>
      <Acknowledgement>Please acknowledge the IMPACT P.I., Janet Luhmann of UCB</Acknowledgement>
      <PublicationInfo>
        <Authors>Luhmann, Janet, G.</Authors>
        <PublicationDate>2023-01-01T00:00:00</PublicationDate>
        <PublishedBy>Space Physics Data Facility</PublishedBy>
      </PublicationInfo>
      <Contact>
        <PersonID>spase://SMWG/Person/Janet.G.Luhmann</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <Contact>
        <PersonID>spase://SMWG/Person/Lee.Frost.Bargatze</PersonID>
        <Role>MetadataContact</Role>
      </Contact>
      <InformationURL>
        <Name>SEPT site at U. Kiel</Name>
        <URL>http://www2.physik.uni-kiel.de/stereo/index.php?doc=home</URL>
      </InformationURL>
      <InformationURL>
        <Name>CDAWeb Skeleton Table</Name>
        <URL>https://cdaweb.gsfc.nasa.gov/pub/software/cdawlib/0SKELTABLES/stb_l1_sept_00000000_v01.skt</URL>
      </InformationURL>
      <PriorID>spase://VEPO/NumericalData/STEREO-B/IMPACT/SEPT/L1/PT1M</PriorID>
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      <Availability>Online</Availability>
      <AccessRights>Open</AccessRights>
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          <RightsName>Creative Commons Zero v1.0 Universal</RightsName>
          <Note>CC0 1.0 Universal is the Creative Commons license applicable to all publicly available NASA Heliophysics data products</Note>
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      </RightsList>
      <AccessURL>
        <Name>CDAWeb</Name>
        <URL>https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=STB_L1_SEPT&amp;index=sp_phys</URL>
        <ProductKey>STB_L1_SEPT</ProductKey>
        <Description>With subset, plot and ASCII list functions from CDAWeb</Description>
      </AccessURL>
      <AccessURL>
        <Name>FTPS from SPDF (not with most browsers)</Name>
        <URL>ftps://spdf.gsfc.nasa.gov/pub/data/stereo/behind/l1/impact/sept/</URL>
      </AccessURL>
      <AccessURL>
        <Name>HTTPS from SPDF</Name>
        <URL>https://spdf.gsfc.nasa.gov/pub/data/stereo/behind/l1/impact/sept/</URL>
        <Description>In CDF via HTTP from SPDF</Description>
      </AccessURL>
      <Format>CDF</Format>
      <DataExtent>
        <Quantity>3275</Quantity>
        <Units>kB</Units>
        <Per>P1D</Per>
      </DataExtent>
      <Acknowledgement>Please acknowledge the P.I., Janet Luhmann of UCB, and CDAWeb at GSFC/SPDF</Acknowledgement>
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      <AccessURL>
        <Name>CDAWeb HAPI Server</Name>
        <URL>https://cdaweb.gsfc.nasa.gov/hapi</URL>
        <Style>HAPI</Style>
        <ProductKey>STB_L1_SEPT@0</ProductKey>
        <ProductKey>STB_L1_SEPT@1</ProductKey>
        <Description>Web Service to this product using the HAPI interface.</Description>
      </AccessURL>
      <Format>CSV</Format>
      <Acknowledgement>Please acknowledge the P.I., Janet Luhmann of UCB, and CDAWeb at GSFC/SPDF</Acknowledgement>
    </AccessInformation>
    <InstrumentID>spase://SMWG/Instrument/STEREO-B/IMPACT/SEPT</InstrumentID>
    <MeasurementType>EnergeticParticles</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2006-11-13T00:00:00</StartDate>
        <RelativeStopDate>-P5M</RelativeStopDate>
      </TimeSpan>
      <Cadence>PT1M</Cadence>
    </TemporalDescription>
    <ObservedRegion>Heliosphere.Remote1AU</ObservedRegion>
    <Parameter>
      <Name>Electron spectrum viewing northward from ecliptic plane</Name>
      <ParameterKey>Spec_0_NS</ParameterKey>
      <Description>Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed northward from the ecliptic plane</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 electron fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Electron spectrum viewing southward from ecliptic plane</Name>
      <ParameterKey>Spec_2_NS</ParameterKey>
      <Description>Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed southward from the ecliptic plane</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 electron fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Proton spectrum viewing northward from ecliptic plane</Name>
      <ParameterKey>Spec_3_NS</ParameterKey>
      <Description>Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed northward from the ecliptic plane</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 proton fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Proton</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Proton spectrum viewing southward from ecliptic plane</Name>
      <ParameterKey>Spec_1_NS</ParameterKey>
      <Description>Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed southward from the ecliptic plane</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 proton fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Proton</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Electron spectrum viewing sunward along the Parker IMF angle</Name>
      <ParameterKey>Spec_2_E</ParameterKey>
      <Description>Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed sunward along the Parker IMF spiral angle</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 electron fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Electron spectrum viewing antisunward along the Parker IMF angle</Name>
      <ParameterKey>Spec_0_E</ParameterKey>
      <Description>Electron flux in each of 32 energy bands between 20 keV and 4000 keV, from the SEPT sensor pointed antisunward along the Parker IMF spiral angle</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 electron fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Electron</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Proton spectrum viewing sunward along the Parker IMF angle</Name>
      <ParameterKey>Spec_1_E</ParameterKey>
      <Description>Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed sunward along the Parker IMF spiral angle</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 proton fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Proton</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>Proton spectrum viewing antisunward along the Parker IMF angle</Name>
      <ParameterKey>Spec_3_E</ParameterKey>
      <Description>Proton flux in each of 32 energy bands between 20 keV and 7000 keV, from the SEPT sensor pointed antisunward along the Parker IMF spiral angle</Description>
      <Cadence>PT1M</Cadence>
      <Units>1/(sec sr cm^2 MeV)</Units>
      <Structure>
        <Size>32</Size>
        <Description>Set of 32 proton fluxes</Description>
      </Structure>
      <FillValue>-1.0e+31</FillValue>
      <Particle>
        <ParticleType>Proton</ParticleType>
        <ParticleQuantity>NumberFlux</ParticleQuantity>
      </Particle>
    </Parameter>
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