CDPP / CNES

Commit 2294f7fd4722c07fd8deed7c5a93f3e8ae3ce7db

Authored by Benjamin Renard
1 parent 1a77fe0f
Exists in juice_jdc and in 1 other branch amdadev

Add Bepi/MIA/L1p datasets

Showing 16 changed files with 1026 additions and 10 deletions   Show diff stats
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NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.3dc.m1.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - 3D count M1 mode</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU–0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
  9 + <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU-0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all.xml 0 → 100644
  Diff comments   View file @2294f7f
... ... @@ -0,0 +1,126 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<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">
  3 + <Version>2.4.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>L1 - Et ALL sector</ResourceName>
  8 + <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
  9 + <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU-0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <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>
  25 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
  26 + </InformationURL>
  27 + <Association>
  28 + <AssociationID>bepi-mia-cruise</AssociationID>
  29 + <AssociationType>PartOf</AssociationType>
  30 + <Note>cruise</Note>
  31 + </Association>
  32 + </ResourceHeader>
  33 + <AccessInformation>
  34 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  35 + <Availability>Online</Availability>
  36 + <AccessRights>Restricted</AccessRights>
  37 + <AccessURL>
  38 + <Name>CDPP/AMDA HAPI Server</Name>
  39 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  40 + <Style>HAPI</Style>
  41 + <Description>Web Service to this product using the HAPI interface.</Description>
  42 + </AccessURL>
  43 + <Format>CSV</Format>
  44 + <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>
  45 + </AccessInformation>
  46 + <AccessInformation>
  47 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  48 + <Availability>Online</Availability>
  49 + <AccessRights>Restricted</AccessRights>
  50 + <AccessURL>
  51 + <Name>CDPP/AMDA Web application</Name>
  52 + <URL>http://amda.cdpp.eu</URL>
  53 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  54 + </AccessURL>
  55 + <Format>CSV</Format>
  56 + <Format>VOTable</Format>
  57 + <Format>CDF</Format>
  58 + <Format>PNG</Format>
  59 + <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>
  60 + </AccessInformation>
  61 + <ProviderName>JAXA</ProviderName>
  62 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
  63 + <MeasurementType>ThermalPlasma</MeasurementType>
  64 + <TemporalDescription>
  65 + <TimeSpan>
  66 + <StartDate>2020-10-15T00:00:00Z</StartDate>
  67 + <StopDate>2020-10-15T07:13:20Z</StopDate>
  68 + </TimeSpan>
  69 + <CadenceMin>PT4S</CadenceMin>
  70 + </TemporalDescription>
  71 + <ObservedRegion>Heliosphere</ObservedRegion>
  72 + <Parameter>
  73 + <Name>counts dir1</Name>
  74 + <ParameterKey>mia_cruise_etall_d1</ParameterKey>
  75 + <Description>Raw counts SpinSectorGroup0,7</Description>
  76 + <Units>counts/sample</Units>
  77 + <RenderingHints>
  78 + <DisplayType>Spectrogram</DisplayType>
  79 + </RenderingHints>
  80 + <Particle>
  81 + <ParticleType>Ion</ParticleType>
  82 + <ParticleQuantity>Counts</ParticleQuantity>
  83 + </Particle>
  84 + </Parameter>
  85 + <Parameter>
  86 + <Name>counts dir2</Name>
  87 + <ParameterKey>mia_cruise_etall_d2</ParameterKey>
  88 + <Description>Raw counts SpinSectorGroup1-2</Description>
  89 + <Units>counts/sample</Units>
  90 + <RenderingHints>
  91 + <DisplayType>Spectrogram</DisplayType>
  92 + </RenderingHints>
  93 + <Particle>
  94 + <ParticleType>Ion</ParticleType>
  95 + <ParticleQuantity>Counts</ParticleQuantity>
  96 + </Particle>
  97 + </Parameter>
  98 + <Parameter>
  99 + <Name>counts dir3</Name>
  100 + <ParameterKey>mia_cruise_etall_d3</ParameterKey>
  101 + <Description>Raw counts SpinSectorGroup3-4</Description>
  102 + <Units>counts/sample</Units>
  103 + <RenderingHints>
  104 + <DisplayType>Spectrogram</DisplayType>
  105 + </RenderingHints>
  106 + <Particle>
  107 + <ParticleType>Ion</ParticleType>
  108 + <ParticleQuantity>Counts</ParticleQuantity>
  109 + </Particle>
  110 + </Parameter>
  111 + <Parameter>
  112 + <Name>counts dir4</Name>
  113 + <ParameterKey>mia_cruise_etall_d4</ParameterKey>
  114 + <Description>Raw counts SpinSectorGroup5-6</Description>
  115 + <Units>counts/sample</Units>
  116 + <RenderingHints>
  117 + <DisplayType>Spectrogram</DisplayType>
  118 + </RenderingHints>
  119 + <Particle>
  120 + <ParticleType>Ion</ParticleType>
  121 + <ParticleQuantity>Counts</ParticleQuantity>
  122 + </Particle>
  123 + </Parameter>
  124 +
  125 + </NumericalData>
  126 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.swall.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - Et SW ALL</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU–0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
  9 + <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU-0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all.xml 0 → 100644
  Diff comments   View file @2294f7f
... ... @@ -0,0 +1,178 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<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">
  3 + <Version>2.4.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>L1p - Et ALL sector</ResourceName>
  8 + <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
  9 + <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU-0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <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>
  25 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
  26 + </InformationURL>
  27 + <Association>
  28 + <AssociationID>bepi-mia-cruise</AssociationID>
  29 + <AssociationType>PartOf</AssociationType>
  30 + <Note>cruise</Note>
  31 + </Association>
  32 + </ResourceHeader>
  33 + <AccessInformation>
  34 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  35 + <Availability>Online</Availability>
  36 + <AccessRights>Restricted</AccessRights>
  37 + <AccessURL>
  38 + <Name>CDPP/AMDA HAPI Server</Name>
  39 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  40 + <Style>HAPI</Style>
  41 + <Description>Web Service to this product using the HAPI interface.</Description>
  42 + </AccessURL>
  43 + <Format>CSV</Format>
  44 + <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>
  45 + </AccessInformation>
  46 + <AccessInformation>
  47 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  48 + <Availability>Online</Availability>
  49 + <AccessRights>Restricted</AccessRights>
  50 + <AccessURL>
  51 + <Name>CDPP/AMDA Web application</Name>
  52 + <URL>http://amda.cdpp.eu</URL>
  53 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  54 + </AccessURL>
  55 + <Format>CSV</Format>
  56 + <Format>VOTable</Format>
  57 + <Format>CDF</Format>
  58 + <Format>PNG</Format>
  59 + <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>
  60 + </AccessInformation>
  61 + <ProviderName>JAXA</ProviderName>
  62 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
  63 + <MeasurementType>ThermalPlasma</MeasurementType>
  64 + <TemporalDescription>
  65 + <TimeSpan>
  66 + <StartDate>2020-10-15T00:00:00Z</StartDate>
  67 + <StopDate>2020-10-15T07:13:20Z</StopDate>
  68 + </TimeSpan>
  69 + <CadenceMin>PT4S</CadenceMin>
  70 + </TemporalDescription>
  71 + <ObservedRegion>Heliosphere</ObservedRegion>
  72 + <Parameter>
  73 + <Name>counts dir1</Name>
  74 + <ParameterKey>mia_cruise_l1petall_d1</ParameterKey>
  75 + <Description>Raw counts SpinSectorGroup0,7</Description>
  76 + <Units>counts/sample</Units>
  77 + <RenderingHints>
  78 + <DisplayType>Spectrogram</DisplayType>
  79 + </RenderingHints>
  80 + <Particle>
  81 + <ParticleType>Ion</ParticleType>
  82 + <ParticleQuantity>Counts</ParticleQuantity>
  83 + </Particle>
  84 + </Parameter>
  85 + <Parameter>
  86 + <Name>counts dir2</Name>
  87 + <ParameterKey>mia_cruise_l1petall_d2</ParameterKey>
  88 + <Description>Raw counts SpinSectorGroup1-2</Description>
  89 + <Units>counts/sample</Units>
  90 + <RenderingHints>
  91 + <DisplayType>Spectrogram</DisplayType>
  92 + </RenderingHints>
  93 + <Particle>
  94 + <ParticleType>Ion</ParticleType>
  95 + <ParticleQuantity>Counts</ParticleQuantity>
  96 + </Particle>
  97 + </Parameter>
  98 + <Parameter>
  99 + <Name>counts dir3</Name>
  100 + <ParameterKey>mia_cruise_l1petall_d3</ParameterKey>
  101 + <Description>Raw counts SpinSectorGroup3-4</Description>
  102 + <Units>counts/sample</Units>
  103 + <RenderingHints>
  104 + <DisplayType>Spectrogram</DisplayType>
  105 + </RenderingHints>
  106 + <Particle>
  107 + <ParticleType>Ion</ParticleType>
  108 + <ParticleQuantity>Counts</ParticleQuantity>
  109 + </Particle>
  110 + </Parameter>
  111 + <Parameter>
  112 + <Name>counts dir4</Name>
  113 + <ParameterKey>mia_cruise_l1petall_d4</ParameterKey>
  114 + <Description>Raw counts SpinSectorGroup5-6</Description>
  115 + <Units>counts/sample</Units>
  116 + <RenderingHints>
  117 + <DisplayType>Spectrogram</DisplayType>
  118 + </RenderingHints>
  119 + <Particle>
  120 + <ParticleType>Ion</ParticleType>
  121 + <ParticleQuantity>Counts</ParticleQuantity>
  122 + </Particle>
  123 + </Parameter>
  124 + <Parameter>
  125 + <Name>diff E flux dir1</Name>
  126 + <ParameterKey>mia_cruise_l1petall_fluxd1</ParameterKey>
  127 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup0,7</Description>
  128 + <Units>eV/cm^2/s/sr/eV</Units>
  129 + <RenderingHints>
  130 + <DisplayType>Spectrogram</DisplayType>
  131 + </RenderingHints>
  132 + <Particle>
  133 + <ParticleType>Ion</ParticleType>
  134 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  135 + </Particle>
  136 + </Parameter>
  137 + <Parameter>
  138 + <Name>diff E flux dir2</Name>
  139 + <ParameterKey>mia_cruise_l1petall_fluxd2</ParameterKey>
  140 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup1-2</Description>
  141 + <Units>eV/cm^2/s/sr/eV</Units>
  142 + <RenderingHints>
  143 + <DisplayType>Spectrogram</DisplayType>
  144 + </RenderingHints>
  145 + <Particle>
  146 + <ParticleType>Ion</ParticleType>
  147 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  148 + </Particle>
  149 + </Parameter>
  150 + <Parameter>
  151 + <Name>diff E flux dir3</Name>
  152 + <ParameterKey>mia_cruise_l1petall_fluxd3</ParameterKey>
  153 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup3-4</Description>
  154 + <Units>eV/cm^2/s/sr/eV</Units>
  155 + <RenderingHints>
  156 + <DisplayType>Spectrogram</DisplayType>
  157 + </RenderingHints>
  158 + <Particle>
  159 + <ParticleType>Ion</ParticleType>
  160 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  161 + </Particle>
  162 + </Parameter>
  163 + <Parameter>
  164 + <Name>diff E flux dir4</Name>
  165 + <ParameterKey>mia_cruise_l1petall_fluxd4</ParameterKey>
  166 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup5-6</Description>
  167 + <Units>eV/cm^2/s/sr/eV</Units>
  168 + <RenderingHints>
  169 + <DisplayType>Spectrogram</DisplayType>
  170 + </RenderingHints>
  171 + <Particle>
  172 + <ParticleType>Ion</ParticleType>
  173 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  174 + </Particle>
  175 + </Parameter>
  176 +
  177 + </NumericalData>
  178 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.all.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - velocity moment all</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU–0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
  9 + <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU-0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.sw.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - velocity moment SW</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU–0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
  9 + <Description>The cruise phase of BepiColombo covers a wide range of heliocentric distances (0.28 AU-0.5 AU) and enables scientific studies in the inner heliosphere before its orbit insertion around Mercury in December 2025.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all.xml 0 → 100644
  Diff comments   View file @2294f7f
... ... @@ -0,0 +1,178 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<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">
  3 + <Version>2.4.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>L1p - Et ALL sector</ResourceName>
  8 + <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
  9 + <Description>The BepiColombo mission conducted the first of its six flybys of Mercury on 1 October 2021 and explored the southern hemisphere of the magnetosphere of Mercury. BepiColombo entered the dusk side magnetosphere from the nightside and exited in the dayside through the dawn side magnetosphere.</Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <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>
  25 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
  26 + </InformationURL>
  27 + <Association>
  28 + <AssociationID>bepi-mia-mercury1</AssociationID>
  29 + <AssociationType>PartOf</AssociationType>
  30 + <Note>Mercury flyby #1</Note>
  31 + </Association>
  32 + </ResourceHeader>
  33 + <AccessInformation>
  34 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  35 + <Availability>Online</Availability>
  36 + <AccessRights>Restricted</AccessRights>
  37 + <AccessURL>
  38 + <Name>CDPP/AMDA HAPI Server</Name>
  39 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  40 + <Style>HAPI</Style>
  41 + <Description>Web Service to this product using the HAPI interface.</Description>
  42 + </AccessURL>
  43 + <Format>CSV</Format>
  44 + <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>
  45 + </AccessInformation>
  46 + <AccessInformation>
  47 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  48 + <Availability>Online</Availability>
  49 + <AccessRights>Restricted</AccessRights>
  50 + <AccessURL>
  51 + <Name>CDPP/AMDA Web application</Name>
  52 + <URL>http://amda.cdpp.eu</URL>
  53 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  54 + </AccessURL>
  55 + <Format>CSV</Format>
  56 + <Format>VOTable</Format>
  57 + <Format>CDF</Format>
  58 + <Format>PNG</Format>
  59 + <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>
  60 + </AccessInformation>
  61 + <ProviderName>JAXA</ProviderName>
  62 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
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  66 + <StartDate>2020-10-15T00:00:00Z</StartDate>
  67 + <StopDate>2020-10-15T07:13:20Z</StopDate>
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  69 + <CadenceMin>PT4S</CadenceMin>
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  83 + </Particle>
  84 + </Parameter>
  85 + <Parameter>
  86 + <Name>counts dir2</Name>
  87 + <ParameterKey>mia_mercury1_l1petall_d2</ParameterKey>
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  89 + <Units>counts/sample</Units>
  90 + <RenderingHints>
  91 + <DisplayType>Spectrogram</DisplayType>
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  93 + <Particle>
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  97 + </Parameter>
  98 + <Parameter>
  99 + <Name>counts dir3</Name>
  100 + <ParameterKey>mia_mercury1_l1petall_d3</ParameterKey>
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  102 + <Units>counts/sample</Units>
  103 + <RenderingHints>
  104 + <DisplayType>Spectrogram</DisplayType>
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  106 + <Particle>
  107 + <ParticleType>Ion</ParticleType>
  108 + <ParticleQuantity>Counts</ParticleQuantity>
  109 + </Particle>
  110 + </Parameter>
  111 + <Parameter>
  112 + <Name>counts dir4</Name>
  113 + <ParameterKey>mia_mercury1_l1petall_d4</ParameterKey>
  114 + <Description>Raw counts SpinSectorGroup5-6</Description>
  115 + <Units>counts/sample</Units>
  116 + <RenderingHints>
  117 + <DisplayType>Spectrogram</DisplayType>
  118 + </RenderingHints>
  119 + <Particle>
  120 + <ParticleType>Ion</ParticleType>
  121 + <ParticleQuantity>Counts</ParticleQuantity>
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  123 + </Parameter>
  124 + <Parameter>
  125 + <Name>diff E flux dir1</Name>
  126 + <ParameterKey>mia_mercury1_l1petall_fluxd1</ParameterKey>
  127 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup0,7</Description>
  128 + <Units>eV/cm^2/s/sr/eV</Units>
  129 + <RenderingHints>
  130 + <DisplayType>Spectrogram</DisplayType>
  131 + </RenderingHints>
  132 + <Particle>
  133 + <ParticleType>Ion</ParticleType>
  134 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  135 + </Particle>
  136 + </Parameter>
  137 + <Parameter>
  138 + <Name>diff E flux dir2</Name>
  139 + <ParameterKey>mia_mercury1_l1petall_fluxd2</ParameterKey>
  140 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup1-2</Description>
  141 + <Units>eV/cm^2/s/sr/eV</Units>
  142 + <RenderingHints>
  143 + <DisplayType>Spectrogram</DisplayType>
  144 + </RenderingHints>
  145 + <Particle>
  146 + <ParticleType>Ion</ParticleType>
  147 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  148 + </Particle>
  149 + </Parameter>
  150 + <Parameter>
  151 + <Name>diff E flux dir3</Name>
  152 + <ParameterKey>mia_mercury1_l1petall_fluxd3</ParameterKey>
  153 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup3-4</Description>
  154 + <Units>eV/cm^2/s/sr/eV</Units>
  155 + <RenderingHints>
  156 + <DisplayType>Spectrogram</DisplayType>
  157 + </RenderingHints>
  158 + <Particle>
  159 + <ParticleType>Ion</ParticleType>
  160 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  161 + </Particle>
  162 + </Parameter>
  163 + <Parameter>
  164 + <Name>diff E flux dir4</Name>
  165 + <ParameterKey>mia_mercury1_l1petall_fluxd4</ParameterKey>
  166 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup5-6</Description>
  167 + <Units>eV/cm^2/s/sr/eV</Units>
  168 + <RenderingHints>
  169 + <DisplayType>Spectrogram</DisplayType>
  170 + </RenderingHints>
  171 + <Particle>
  172 + <ParticleType>Ion</ParticleType>
  173 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  174 + </Particle>
  175 + </Parameter>
  176 +
  177 + </NumericalData>
  178 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all.xml 0 → 100644
  Diff comments   View file @2294f7f
... ... @@ -0,0 +1,178 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<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">
  3 + <Version>2.4.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>L1p - Et ALL sector</ResourceName>
  8 + <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
  9 + <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).</Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <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>
  25 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
  26 + </InformationURL>
  27 + <Association>
  28 + <AssociationID>bepi-mia-mercury2</AssociationID>
  29 + <AssociationType>PartOf</AssociationType>
  30 + <Note>Mercury flyby #2</Note>
  31 + </Association>
  32 + </ResourceHeader>
  33 + <AccessInformation>
  34 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  35 + <Availability>Online</Availability>
  36 + <AccessRights>Restricted</AccessRights>
  37 + <AccessURL>
  38 + <Name>CDPP/AMDA HAPI Server</Name>
  39 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  40 + <Style>HAPI</Style>
  41 + <Description>Web Service to this product using the HAPI interface.</Description>
  42 + </AccessURL>
  43 + <Format>CSV</Format>
  44 + <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>
  45 + </AccessInformation>
  46 + <AccessInformation>
  47 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  48 + <Availability>Online</Availability>
  49 + <AccessRights>Restricted</AccessRights>
  50 + <AccessURL>
  51 + <Name>CDPP/AMDA Web application</Name>
  52 + <URL>http://amda.cdpp.eu</URL>
  53 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  54 + </AccessURL>
  55 + <Format>CSV</Format>
  56 + <Format>VOTable</Format>
  57 + <Format>CDF</Format>
  58 + <Format>PNG</Format>
  59 + <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>
  60 + </AccessInformation>
  61 + <ProviderName>JAXA</ProviderName>
  62 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
  63 + <MeasurementType>ThermalPlasma</MeasurementType>
  64 + <TemporalDescription>
  65 + <TimeSpan>
  66 + <StartDate>2020-10-15T00:00:00Z</StartDate>
  67 + <StopDate>2020-10-15T07:13:20Z</StopDate>
  68 + </TimeSpan>
  69 + <CadenceMin>PT4S</CadenceMin>
  70 + </TemporalDescription>
  71 + <ObservedRegion>Mercury</ObservedRegion>
  72 + <Parameter>
  73 + <Name>counts dir1</Name>
  74 + <ParameterKey>mia_mercury2_l1petall_d1</ParameterKey>
  75 + <Description>Raw counts SpinSectorGroup0,7</Description>
  76 + <Units>counts/sample</Units>
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  78 + <DisplayType>Spectrogram</DisplayType>
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  80 + <Particle>
  81 + <ParticleType>Ion</ParticleType>
  82 + <ParticleQuantity>Counts</ParticleQuantity>
  83 + </Particle>
  84 + </Parameter>
  85 + <Parameter>
  86 + <Name>counts dir2</Name>
  87 + <ParameterKey>mia_mercury2_l1petall_d2</ParameterKey>
  88 + <Description>Raw counts SpinSectorGroup1-2</Description>
  89 + <Units>counts/sample</Units>
  90 + <RenderingHints>
  91 + <DisplayType>Spectrogram</DisplayType>
  92 + </RenderingHints>
  93 + <Particle>
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  95 + <ParticleQuantity>Counts</ParticleQuantity>
  96 + </Particle>
  97 + </Parameter>
  98 + <Parameter>
  99 + <Name>counts dir3</Name>
  100 + <ParameterKey>mia_mercury2_l1petall_d3</ParameterKey>
  101 + <Description>Raw counts SpinSectorGroup3-4</Description>
  102 + <Units>counts/sample</Units>
  103 + <RenderingHints>
  104 + <DisplayType>Spectrogram</DisplayType>
  105 + </RenderingHints>
  106 + <Particle>
  107 + <ParticleType>Ion</ParticleType>
  108 + <ParticleQuantity>Counts</ParticleQuantity>
  109 + </Particle>
  110 + </Parameter>
  111 + <Parameter>
  112 + <Name>counts dir4</Name>
  113 + <ParameterKey>mia_mercury2_l1petall_d4</ParameterKey>
  114 + <Description>Raw counts SpinSectorGroup5-6</Description>
  115 + <Units>counts/sample</Units>
  116 + <RenderingHints>
  117 + <DisplayType>Spectrogram</DisplayType>
  118 + </RenderingHints>
  119 + <Particle>
  120 + <ParticleType>Ion</ParticleType>
  121 + <ParticleQuantity>Counts</ParticleQuantity>
  122 + </Particle>
  123 + </Parameter>
  124 + <Parameter>
  125 + <Name>diff E flux dir1</Name>
  126 + <ParameterKey>mia_mercury2_l1petall_fluxd1</ParameterKey>
  127 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup0,7</Description>
  128 + <Units>eV/cm^2/s/sr/eV</Units>
  129 + <RenderingHints>
  130 + <DisplayType>Spectrogram</DisplayType>
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  132 + <Particle>
  133 + <ParticleType>Ion</ParticleType>
  134 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  135 + </Particle>
  136 + </Parameter>
  137 + <Parameter>
  138 + <Name>diff E flux dir2</Name>
  139 + <ParameterKey>mia_mercury2_l1petall_fluxd2</ParameterKey>
  140 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup1-2</Description>
  141 + <Units>eV/cm^2/s/sr/eV</Units>
  142 + <RenderingHints>
  143 + <DisplayType>Spectrogram</DisplayType>
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  145 + <Particle>
  146 + <ParticleType>Ion</ParticleType>
  147 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  148 + </Particle>
  149 + </Parameter>
  150 + <Parameter>
  151 + <Name>diff E flux dir3</Name>
  152 + <ParameterKey>mia_mercury2_l1petall_fluxd3</ParameterKey>
  153 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup3-4</Description>
  154 + <Units>eV/cm^2/s/sr/eV</Units>
  155 + <RenderingHints>
  156 + <DisplayType>Spectrogram</DisplayType>
  157 + </RenderingHints>
  158 + <Particle>
  159 + <ParticleType>Ion</ParticleType>
  160 + <ParticleQuantity>EnergyFlux</ParticleQuantity>
  161 + </Particle>
  162 + </Parameter>
  163 + <Parameter>
  164 + <Name>diff E flux dir4</Name>
  165 + <ParameterKey>mia_mercury2_l1petall_fluxd4</ParameterKey>
  166 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup5-6</Description>
  167 + <Units>eV/cm^2/s/sr/eV</Units>
  168 + <RenderingHints>
  169 + <DisplayType>Spectrogram</DisplayType>
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  171 + <Particle>
  172 + <ParticleType>Ion</ParticleType>
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  175 + </Parameter>
  176 +
  177 + </NumericalData>
  178 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m1.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - 3D count M1 mode</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet’s surface, on the night side of the planet.</Description>
  9 + <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet's surface, on the night side of the planet.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m3.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - 3D count M3 mode</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet’s surface, on the night side of the planet.</Description>
  9 + <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet's surface, on the night side of the planet.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.all.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - Et ALL sector</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet’s surface, on the night side of the planet.</Description>
  9 + <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet's surface, on the night side of the planet.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.swall.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - Et SW ALL</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet’s surface, on the night side of the planet.</Description>
  9 + <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet's surface, on the night side of the planet.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.all.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - velocity moment all</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet’s surface, on the night side of the planet.</Description>
  9 + <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet's surface, on the night side of the planet.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.sw.xml
  Diff comments   View file @2294f7f
... ... @@ -6,7 +6,7 @@
6 6 <ResourceHeader>
7 7 <ResourceName>L1 - velocity moment SW</ResourceName>
8 8 <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
9   - <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet’s surface, on the night side of the planet.</Description>
  9 + <Description>The BepiColombo mission conducted the third of its six flybys of Mercury on 19 June 2023, about 236 km above the planet's surface, on the night side of the planet.</Description>
10 10 <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
11 11 <Contact>
12 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.l1p.et.all.xml 0 → 100644
  Diff comments   View file @2294f7f
... ... @@ -0,0 +1,178 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<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">
  3 + <Version>2.4.1</Version>
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  6 + <ResourceHeader>
  7 + <ResourceName>L1p - Et ALL sector</ResourceName>
  8 + <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
  9 + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail.</Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  13 + <Role>PrincipalInvestigator</Role>
  14 + </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <InformationURL>
  24 + <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>
  25 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
  26 + </InformationURL>
  27 + <Association>
  28 + <AssociationID>bepi-mia-venus1</AssociationID>
  29 + <AssociationType>PartOf</AssociationType>
  30 + <Note>Venus flyby #1</Note>
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  37 + <AccessURL>
  38 + <Name>CDPP/AMDA HAPI Server</Name>
  39 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  40 + <Style>HAPI</Style>
  41 + <Description>Web Service to this product using the HAPI interface.</Description>
  42 + </AccessURL>
  43 + <Format>CSV</Format>
  44 + <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>
  45 + </AccessInformation>
  46 + <AccessInformation>
  47 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  48 + <Availability>Online</Availability>
  49 + <AccessRights>Restricted</AccessRights>
  50 + <AccessURL>
  51 + <Name>CDPP/AMDA Web application</Name>
  52 + <URL>http://amda.cdpp.eu</URL>
  53 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  54 + </AccessURL>
  55 + <Format>CSV</Format>
  56 + <Format>VOTable</Format>
  57 + <Format>CDF</Format>
  58 + <Format>PNG</Format>
  59 + <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>
  60 + </AccessInformation>
  61 + <ProviderName>JAXA</ProviderName>
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  66 + <StartDate>2020-10-15T00:00:00Z</StartDate>
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  128 + <Units>eV/cm^2/s/sr/eV</Units>
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  140 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup1-2</Description>
  141 + <Units>eV/cm^2/s/sr/eV</Units>
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  151 + <Name>diff E flux dir3</Name>
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  164 + <Name>diff E flux dir4</Name>
  165 + <ParameterKey>mia_venus1_l1petall_fluxd4</ParameterKey>
  166 + <Description>Omni-directional Differential Energy Flux, SpinSectorGroup5-6</Description>
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  176 +
  177 + </NumericalData>
  178 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.l1p.et.all.xml 0 → 100644
  Diff comments   View file @2294f7f
... ... @@ -0,0 +1,178 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<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">
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  6 + <ResourceHeader>
  7 + <ResourceName>L1p - Et ALL sector</ResourceName>
  8 + <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate>
  9 + <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.</Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  11 + <Contact>
  12 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
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  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
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  24 + <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>
  25 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
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  40 + <Style>HAPI</Style>
  41 + <Description>Web Service to this product using the HAPI interface.</Description>
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  43 + <Format>CSV</Format>
  44 + <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>
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  55 + <Format>CSV</Format>
  56 + <Format>VOTable</Format>
  57 + <Format>CDF</Format>
  58 + <Format>PNG</Format>
  59 + <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>
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  61 + <ProviderName>JAXA</ProviderName>
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... ...