bepi-mia-mercury2.et.swall.xml 6.84 KB
<?xml version="1.0" encoding="UTF-8"?>
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  <Version>2.4.1</Version>
  <NumericalData>
    <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.swall</ResourceID>
    <ResourceHeader>
      <ResourceName>L1 - Et SW ALL</ResourceName>
      <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
      <Description>The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface).

L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description>
      <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
      <Contact>
        <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
        <Role>PrincipalInvestigator</Role>
      </Contact>
      <Contact>       
         <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID> 
         <Role>DataProducer</Role>
      </Contact>
      <Contact>
        <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
        <Role>DataProducer</Role>
      </Contact>
      <InformationURL>
        <Name>Aizawa, S., Harada, Y., André, N., Saito, Y., Barabash, S., Delcourt, D., Sauvaud, J.-A., Barthe, A., Fedorov, A., Penou, E., Yokota, S., Miyake, W., Persson, M., Nenon, Q., Rojo, M., Futaana, Y., Asamura, K., Shimoyama, M., Hadid, L., … Murakami, G. (2023). Direct evidence of substorm-related impulsive injections of electrons at Mercury (version 1) [Data set]. Zenodo.</Name>
        <URL>https://doi.org/10.5281/zenodo.7926905</URL>
      </InformationURL>
      <Association>
        <AssociationID>bepi-mia-mercury2</AssociationID>
        <AssociationType>PartOf</AssociationType>
        <Note>Mercury flyby #2</Note>
      </Association>
    </ResourceHeader>
    <AccessInformation>
      <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
      <Availability>Online</Availability>
      <AccessRights>Restricted</AccessRights>
      <AccessURL>
        <Name>CDPP/AMDA HAPI Server</Name>
        <URL>http://amda.irap.omp.eu/service/hapi</URL>
        <Style>HAPI</Style>
        <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 http://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>Restricted</AccessRights>
      <AccessURL>
        <Name>CDPP/AMDA Web application</Name>
        <URL>http://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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers.</Acknowledgement>
    </AccessInformation>
    <ProviderName>JAXA</ProviderName>
    <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
    <MeasurementType>ThermalPlasma</MeasurementType>
    <TemporalDescription>
      <TimeSpan>
        <StartDate>2020-10-15T00:00:00Z</StartDate>
        <StopDate>2020-10-15T07:13:20Z</StopDate>
      </TimeSpan>
      <CadenceMin>PT32S</CadenceMin>
    </TemporalDescription>
    <ObservedRegion>Mercury</ObservedRegion>
        <Parameter>
      <Name>counts dir1</Name>
      <ParameterKey>mia_mercury2_etswall_d1</ParameterKey>
      <Description>Raw counts SpinSectorGroup0,7</Description>
      <Units>counts/sample</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>Counts</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>counts dir2</Name>
      <ParameterKey>mia_mercury2_etswall_d2</ParameterKey>
      <Description>Raw counts SpinSectorGroup1-2</Description>
      <Units>counts/sample</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>Counts</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>counts dir3</Name>
      <ParameterKey>mia_mercury2_etswall_d3</ParameterKey>
      <Description>Raw counts SpinSectorGroup3-4</Description>
      <Units>counts/sample</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>Counts</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>counts dir4</Name>
      <ParameterKey>mia_mercury2_etswall_d4</ParameterKey>
      <Description>Raw counts SpinSectorGroup5-6</Description>
      <Units>counts/sample</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>Counts</ParticleQuantity>
      </Particle>
    </Parameter>
    <Parameter>
      <Name>counts SW</Name>
      <ParameterKey>mia_mercury2_etswall_sw</ParameterKey>
      <Description>Raw counts Solar Wind channel</Description>
      <Units>counts/sample</Units>
      <RenderingHints>
        <DisplayType>Spectrogram</DisplayType>
      </RenderingHints>
      <Particle>
        <ParticleType>Ion</ParticleType>
        <ParticleQuantity>Counts</ParticleQuantity>
      </Particle>
    </Parameter>

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