bepi-mia-venus2.et.all.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/BepiColombo/Mio/MIA/bepi-mia-venus2.et.all</ResourceID>
<ResourceHeader>
<ResourceName>L1 - Et ALL sector</ResourceName>
<ReleaseDate>2024-04-10T12:07:17Z</ReleaseDate>
<Description>The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region.
L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</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-venus2</AssociationID>
<AssociationType>PartOf</AssociationType>
<Note>Venus 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>https://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<ProductKey>bepi-mia-venus2.et.all</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>Restricted</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>JAXA</ProviderName>
<InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
<MeasurementType>ThermalPlasma</MeasurementType>
<TemporalDescription>
<TimeSpan>
<StartDate>2021-08-09T01:05:01Z</StartDate>
<StopDate>2021-08-10T23:30:42Z</StopDate>
</TimeSpan>
<CadenceMin>PT4S</CadenceMin>
</TemporalDescription>
<ObservedRegion>Venus</ObservedRegion>
<Parameter>
<Name>counts dir1</Name>
<ParameterKey>mia_venus2_etall_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_venus2_etall_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_venus2_etall_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_venus2_etall_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>
</NumericalData>
</Spase>