bepi-mia-mercury2.3dc.m1.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-mercury2.3dc.m1</ResourceID>
<ResourceHeader>
<ResourceName>L1 - 3D count M1 mode</ResourceName>
<ReleaseDate>2024-04-10T12:07:12Z</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 3D velocity distribution function data 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>https://amda.irap.omp.eu/service/hapi</URL>
<Style>HAPI</Style>
<ProductKey>bepi-mia-mercury2.3dc.m1</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>2022-06-22T04:58:33Z</StartDate>
<StopDate>2022-06-23T20:39:36Z</StopDate>
</TimeSpan>
<CadenceMin>PT3600S</CadenceMin>
</TemporalDescription>
<ObservedRegion>Mercury</ObservedRegion>
<Parameter>
<Name>counts : sum on elev; azim/energy : 2D</Name>
<ParameterKey>mia_mercury2_3dcm1_elev</ParameterKey>
<Description>Raw counts. Sum on elevation</Description>
<Units>counts/sample</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Particle>
<ParticleType>Ion</ParticleType>
<ParticleQuantity>Counts</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>counts : sum on azim; elev/energy : 2D</Name>
<ParameterKey>mia_mercury2_3dcm1_azim</ParameterKey>
<Description>Raw counts. Sum on azimuth</Description>
<Units>counts/sample</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Particle>
<ParticleType>Ion</ParticleType>
<ParticleQuantity>Counts</ParticleQuantity>
</Particle>
</Parameter>
<Parameter>
<Name>counts : sum on energy; azim/elev : 2D</Name>
<ParameterKey>mia_mercury2_3dcm1_energy</ParameterKey>
<Description>Raw counts. Sum on energy</Description>
<Units>counts/sample</Units>
<RenderingHints>
<DisplayType>Spectrogram</DisplayType>
</RenderingHints>
<Particle>
<ParticleType>Ion</ParticleType>
<ParticleQuantity>Counts</ParticleQuantity>
</Particle>
</Parameter>
</NumericalData>
</Spase>