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        <meta content="Robert.M.Candey" name="rno"/>
        <meta content="Tamara.J.Kovalick" name="content-owner"/>
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        <title>SPASE Resource Description</title>
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      "name": "SolarOrbiter - EPD/EPT - L2 : electron flux - anti-sunward flow",
        "alternateName": "Ion Flux From Sun Direction ( mean Parker spiral )",
      "dateModified": "2025-10-12",
      
    "identifier": "spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun",
        
    "creditText": "See http://espada.uah.es/epd/EPD_data.php",
    "description": "Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. \n              \n            EPT  measures electrons and ions in the lower part of the energetic particle spectrum. It \neffectuates measurements in 4 different fields of view :\n\n* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun.\n* Sunward Flow. Detector looks opposite to the Sun direction.\n* Northward Flow. Detector looks towards the south ecliptic hemisphere.\n* Southward Flow. Detector looks towards the north ecliptic hemisphere.\n\nParameter ID uses Detector looking directon.\n \nAdditionally, EPT has 2 channels that separate electrons and ions:\n* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV.\n* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. \n          ",
    "abstract": "Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. \n              \n            EPT  measures electrons and ions in the lower part of the energetic particle spectrum. It \neffectuates measurements in 4 different fields of view :\n\n* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun.\n* Sunward Flow. Detector looks opposite to the Sun direction.\n* Northward Flow. Detector looks towards the south ecliptic hemisphere.\n* Southward Flow. Detector looks towards the north ecliptic hemisphere.\n\nParameter ID uses Detector looking directon.\n \nAdditionally, EPT has 2 channels that separate electrons and ions:\n* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV.\n* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. \n          ",
    
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    "temporalCoverage": "2020-05-13T00:00:03Z/2025-06-30T23:59:59Z",

    "genre": "EnergeticParticles",
    "keywords": [  ],
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    "variableMeasured": [
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          "@type": "PropertyValue",
          "name": "el flux: anti-sunward",
          "description": "Particle flux in foil channel",
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          "name": "el cntrate: anti-sunward",
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            <a id="top"/>
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                <img class="usa-banner__header-flag" height="10px" width="20px" src="/logos/us_flag_small.png" alt="USA flag"/> An official website of the United States government
                <button class="usa-banner-button" onclick="toggle_usa_banner_details()">Here's how you know</button> <span id="usa-banner-indicator">v</span>
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        </div>
        <div class="header">
            <div class="middle">HDPWS</div>
        </div>
        <div class="page">
            <div class="spase">
                <div class="abstract">
                    <div class="access">
                        <p class="box-title">
                    Data Access
                </p>
                        <ul class="list">
                            <li class="list">
                                <a target="_blank" href="https://cdaweb.gsfc.nasa.gov/registry/hdp/hapi/hapiHtml.html#url=https://amda.irap.omp.eu/service/hapi&amp;id=so-ept-e.sun">HAPI: CDPP/AMDA HAPI Server</a>
                            </li>
                            <li class="list">
                                <a target="_blank" href="https://amda.cdpp.eu">CDPP/AMDA Web application</a>
                            </li>
                        </ul>
                    </div>
                    <div class="citation inset">
                        <h1>
                            <a name="spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun">SolarOrbiter - EPD/EPT - L2 : electron flux - anti-sunward flow</a>
                        </h1>
                        <p>
                            <div class="term">ResourceID</div>
                            <div class="definition">spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun</div>
                        </p>
                        <p>
                            <div class="term">Description</div>
                            <div class="definition">Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. 
              
            EPT  measures electrons and ions in the lower part of the energetic particle spectrum. It 
effectuates measurements in 4 different fields of view :

* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun.
* Sunward Flow. Detector looks opposite to the Sun direction.
* Northward Flow. Detector looks towards the south ecliptic hemisphere.
* Southward Flow. Detector looks towards the north ecliptic hemisphere.

Parameter ID uses Detector looking directon.
 
Additionally, EPT has 2 channels that separate electrons and ions:
* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV.
* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. 
</div>
                        </p>
                        <p/>
                    </div>
                </div>
                <div>
                    <p class="right">
                        <a target="_blank" href="/WS/hdp/1/Spase?ResourceID=spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun&amp;Format=spase_xml" download="so-ept-e.sun.xml">View XML</a> |
              <a target="_blank" href="https://spase-editor.heliocloud.org/?edit=https://heliophysicsdata.gsfc.nasa.gov/WS/hdp/1/Spase?ResourceID=spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun&amp;Format=spase_xml">Edit</a>
                    </p>
                    <h1 class="detail">Details</h1>
                </div>
                <div>
                    <div class="product">
                        <p class="version">Version:2.4.1</p>
                        <h1>NumericalData</h1>
                        <div class="term">ResourceID</div>
                        <div class="definition">spase://CNES/NumericalData/CDPP-AMDA/Solar_Orbiter/EPD/so-ept-e.sun</div>
                        <div class="term">ResourceHeader</div>
                        <div class="definition">
                            <div class="term">ResourceName</div>
                            <div class="definition">SolarOrbiter - EPD/EPT - L2 : electron flux - anti-sunward flow</div>
                            <div class="term">AlternateName</div>
                            <div class="definition">Ion Flux From Sun Direction ( mean Parker spiral )</div>
                            <div class="term">ReleaseDate</div>
                            <div class="definition">2025-10-12 20:33:33Z</div>
                            <div class="term">Description</div>
                            <div class="definition">Solar Orbiter, Level 2 Data, Energetic Particle Detector, Electron and Proton Telescope, Rates. 
              
            EPT  measures electrons and ions in the lower part of the energetic particle spectrum. It 
effectuates measurements in 4 different fields of view :

* Anti-Sunward Flow. Detector looks in the direction of the mean Parker spiral towards the Sun.
* Sunward Flow. Detector looks opposite to the Sun direction.
* Northward Flow. Detector looks towards the south ecliptic hemisphere.
* Southward Flow. Detector looks towards the north ecliptic hemisphere.

Parameter ID uses Detector looking directon.
 
Additionally, EPT has 2 channels that separate electrons and ions:
* Magnet channel. Uses a permanent magnet to deflect electrons. It measures protons with energies between 25 keV and 6.5 MeV and alpha particles up to 25 MeV.
* Foil channel. Equipped with a foil that absorbs ions, it measures electrons in the energy range 25–500 keV. Ions with energies above 400 keV can penetrate the foil, contaminating the electron measurements. 
</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">See http://espada.uah.es/epd/EPD_data.php</div>
                            <div class="term">Contacts</div>
                            <div class="definition">
                                <table class="nested" cellspacing="0">
                                    <tr>
                                        <th/>
                                        <th class="center">Role</th>
                                        <th class="center">Person</th>
                                        <th class="center">StartDate</th>
                                        <th class="center">StopDate</th>
                                        <th class="center">Note</th>
                                    </tr>
                                    <tbody>
                                        <tr>
                                            <td>1.</td>
                                            <td>PrincipalInvestigator</td>
                                            <td>
                                                <a target="_blank" href="https://spase-metadata.org/SMWG/Person/Javier.Rodriguez-Pacheco.Martin.html">spase://SMWG/Person/Javier.Rodriguez-Pacheco.Martin</a>
                                            </td>
                                            <td/>
                                            <td/>
                                            <td/>
                                        </tr>
                                    </tbody>
                                </table>
                            </div>
                            <div class="term">InformationURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">SolO Archive Support Data</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data">https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/Archive+Support+Data</a>
                                </div>
                            </div>
                            <div class="term">Association</div>
                            <div class="definition">
                                <div class="term">AssociationID</div>
                                <div class="definition">
                                    <a href="https://spase-metadata.org/.html">solo-epd-eptel</a>
                                </div>
                                <div class="term">AssociationType</div>
                                <div class="definition">PartOf</div>
                                <div class="term">Note</div>
                                <div class="definition">L2 : electron flux</div>
                            </div>
                        </div>
                        <div class="term">AccessInformation</div>
                        <div class="definition">
                            <div class="term">RepositoryID</div>
                            <div class="definition">
                                <a href="https://spase-metadata.org/SMWG/Repository/CDPP/AMDA.html">spase://SMWG/Repository/CDPP/AMDA</a>
                            </div>
                            <div class="term">Availability</div>
                            <div class="definition">Online</div>
                            <div class="term">AccessRights</div>
                            <div class="definition">Open</div>
                            <div class="term">AccessURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">CDPP/AMDA HAPI Server</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://amda.irap.omp.eu/service/hapi">https://amda.irap.omp.eu/service/hapi</a>
                                </div>
                                <div class="term">Style</div>
                                <div class="definition">HAPI</div>
                                <div class="term">ProductKey</div>
                                <div class="definition">so-ept-e.sun</div>
                                <div class="term">Description</div>
                                <div class="definition">Web Service to this product using the HAPI interface.</div>
                            </div>
                            <div class="term">Format</div>
                            <div class="definition">CSV</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">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.</div>
                        </div>
                        <div class="term">AccessInformation</div>
                        <div class="definition">
                            <div class="term">RepositoryID</div>
                            <div class="definition">
                                <a href="https://spase-metadata.org/SMWG/Repository/CDPP/AMDA.html">spase://SMWG/Repository/CDPP/AMDA</a>
                            </div>
                            <div class="term">Availability</div>
                            <div class="definition">Online</div>
                            <div class="term">AccessRights</div>
                            <div class="definition">Open</div>
                            <div class="term">AccessURL</div>
                            <div class="definition">
                                <div class="term">Name</div>
                                <div class="definition">CDPP/AMDA Web application</div>
                                <div class="term">URL</div>
                                <div class="definition">
                                    <a target="_blank" href="https://amda.cdpp.eu">https://amda.cdpp.eu</a>
                                </div>
                                <div class="term">Description</div>
                                <div class="definition">Access to Data via CDPP/AMDA Web application.</div>
                            </div>
                            <div class="term">Format</div>
                            <div class="definition">CSV</div>
                            <div class="term">Format</div>
                            <div class="definition">VOTable</div>
                            <div class="term">Format</div>
                            <div class="definition">CDF</div>
                            <div class="term">Format</div>
                            <div class="definition">PNG</div>
                            <div class="term">Acknowledgement</div>
                            <div class="definition">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.</div>
                        </div>
                        <div class="term">ProviderName</div>
                        <div class="definition">http://soar.esac.esa.int/soar</div>
                        <div class="term">ProviderResourceName</div>
                        <div class="definition">EPD-EPT-SUN-RATES</div>
                        <div class="term">InstrumentIDs</div>
                        <div class="definition">
                            <a target="_blank" href="https://spase-metadata.org/CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT.html">spase://CNES/Instrument/CDPP-AMDA/Solar_Orbiter/EPD-EPT</a>
                        </div>
                        <div class="term">MeasurementType</div>
                        <div class="definition">EnergeticParticles</div>
                        <div class="term">TemporalDescription</div>
                        <div class="definition">
                            <div class="term">TimeSpan</div>
                            <div class="definition">
                                <div class="term">StartDate</div>
                                <div class="definition">2020-05-13 00:00:03Z</div>
                                <div class="term">StopDate</div>
                                <div class="definition">2025-06-30 23:59:59Z</div>
                            </div>
                            <div class="term">CadenceMin</div>
                            <div class="definition">PT60S</div>
                            <div class="term">CadenceMax</div>
                            <div class="definition">PT300S</div>
                        </div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Heliosphere.Inner</div>
                        <div class="term">ObservedRegion</div>
                        <div class="definition">Sun.Corona</div>
                        <div class="term">Caveats</div>
                        <div class="definition">Ions with energies around 500 keV can penetrate the foil and give a signal in the electron
           channel. In the presence of high ion flux, there could be a considerable contamination from ions in this product.</div>
                        <div class="parameter">Parameter #1</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">el flux: anti-sunward</div>
                            <div class="term">ParameterKey</div>
                            <div class="definition">solo_ept_sun_eflux</div>
                            <div class="term">Description</div>
                            <div class="definition">Particle flux in foil channel</div>
                            <div class="term">Units</div>
                            <div class="definition">1/(s cm^2 sr MeV)</div>
                            <div class="term">RenderingHints</div>
                            <div class="definition">
                                <div class="term">DisplayType</div>
                                <div class="definition">Spectrogram</div>
                            </div>
                            <div class="term">Structure</div>
                            <div class="definition">
                                <div class="term">Size</div>
                                <div class="definition">34</div>
                            </div>
                            <div class="term">Particle</div>
                            <div class="definition">
                                <div class="term">ParticleType</div>
                                <div class="definition">Electron</div>
                                <div class="term">ParticleQuantity</div>
                                <div class="definition">EnergyFlux</div>
                            </div>
                        </div>
                        <div class="parameter">Parameter #2</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">el flux unc: anti-sunward</div>
                            <div class="term">ParameterKey</div>
                            <div class="definition">solo_ept_sun_eunc</div>
                            <div class="term">Description</div>
                            <div class="definition">Uncertainty in electron flux</div>
                            <div class="term">Units</div>
                            <div class="definition">1/(s cm^2 sr MeV)</div>
                            <div class="term">RenderingHints</div>
                            <div class="definition">
                                <div class="term">DisplayType</div>
                                <div class="definition">Spectrogram</div>
                            </div>
                            <div class="term">Structure</div>
                            <div class="definition">
                                <div class="term">Size</div>
                                <div class="definition">34</div>
                            </div>
                            <div class="term">Particle</div>
                            <div class="definition">
                                <div class="term">ParticleType</div>
                                <div class="definition">Electron</div>
                                <div class="term">ParticleQuantity</div>
                                <div class="definition">EnergyFlux</div>
                            </div>
                        </div>
                        <div class="parameter">Parameter #3</div>
                        <div class="definition">
                            <div class="term">Name</div>
                            <div class="definition">el cntrate: anti-sunward</div>
                            <div class="term">ParameterKey</div>
                            <div class="definition">solo_ept_sun_erate</div>
                            <div class="term">Description</div>
                            <div class="definition">Particle count rate in foil channel</div>
                            <div class="term">Units</div>
                            <div class="definition">cnts/s</div>
                            <div class="term">RenderingHints</div>
                            <div class="definition">
                                <div class="term">DisplayType</div>
                                <div class="definition">Spectrogram</div>
                            </div>
                            <div class="term">Structure</div>
                            <div class="definition">
                                <div class="term">Size</div>
                                <div class="definition">34</div>
                            </div>
                            <div class="term">Particle</div>
                            <div class="definition">
                                <div class="term">ParticleType</div>
                                <div class="definition">Electron</div>
                                <div class="term">ParticleQuantity</div>
                                <div class="definition">CountRate</div>
                            </div>
                        </div>
                    </div>
                </div>
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