CDPP / CNES

Commit 3cc563ad751e946d3403a01cda847571976de6fe

Authored by Benjamin Renard
1 parent 27bd265a
Exists in bepi_update

WIP

Showing 35 changed files with 482 additions and 74 deletions   Show diff stats
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Instrument/CDPP-AMDA/BepiColombo/Ephemeris.xml
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5 5 <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Ephemeris</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>Ephemeris</ResourceName>
8   - <AlternateName>BepiColombo Orbit</AlternateName>
  8 + <AlternateName>BepiColombo Trajectory</AlternateName>
9 9 <ReleaseDate>2017-05-20T21:10:13Z</ReleaseDate>
10   - <Description>Bepi Ephemeris are calculated in IRAP by using BepiColombo SPICE kernels</Description>
11   - <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA</Acknowledgement>
  10 + <Description>BepiColombo Ephemeris are calculated by IRAP using BepiColombo SPICE kernels from the ESA SPICE Service.</Description>
  11 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
12 12 <Contact>
13 13 <PersonID>spase://CNES/Person/CDPP-AMDA/Marc.Sitja</PersonID>
14 14 <Role>PrincipalInvestigator</Role>
15   - </Contact>
  15 + </Contact>
  16 + <InformationURL>
  17 + <Name>ESA SPICE Service</Name>
  18 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  19 + </InformationURL>
16 20 </ResourceHeader>
17 21 <InstrumentType>Platform</InstrumentType>
18 22 <InvestigationName>Spacecraft Position</InvestigationName>
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Instrument/CDPP-AMDA/BepiColombo/MPO/MAG.xml
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4 4 <Instrument>
5 5 <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/MPO/MAG</ResourceID>
6 6 <ResourceHeader>
7   - <ResourceName>MAG</ResourceName>
  7 + <ResourceName>MPO-MAG</ResourceName>
8 8 <AlternateName>Mercury Magnetometer</AlternateName>
9 9 <ReleaseDate>2020-09-22T16:02:13Z</ReleaseDate>
10 10 <Description>MPO-MAG is designed as follows: Two identical magnetometers are used each with
... ... @@ -35,6 +35,11 @@
35 35 <PersonID>spase://SMWG/Person/C.Carr</PersonID>
36 36 <Role>CoInvestigator</Role>
37 37 </Contact>
  38 + <InformationURL>
  39 + <Name>Heyner, D., Auster, HU., Fornaçon, KH. et al. The BepiColombo Planetary Magnetometer MPO-MAG: What Can We Learn from the Hermean Magnetic Field?. Space Sci Rev 217, 52 (2021). </Name>
  40 + <URL>https://doi.org/10.1007/s11214-021-00822-x</URL>
  41 + <Description>Reference paper</Description>
  42 + </InformationURL>
38 43 </ResourceHeader>
39 44 <InstrumentType>Magnetometer</InstrumentType>
40 45 <InvestigationName>Mercury Magnetometer on MPO/InvestigationName</InvestigationName>
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Instrument/CDPP-AMDA/BepiColombo/Mio/MGF.xml
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5 5 <ResourceID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MGF</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>MGF</ResourceName>
8   - <AlternateName>Mercury Magnetometer</AlternateName>
  8 + <AlternateName>Mercury Fluxgate Magnetometer</AlternateName>
9 9 <ReleaseDate>2020-09-22T16:02:13Z</ReleaseDate>
10   - <Description>The MMO/MGF consists of two sets of fluxgate magnetometers on a boom: MGF-O(outboard),
11   - a digital sensor of the same type used in MPO-MAG, mounted on the end of the 4.4 m boom;
12   - and MGF-I (inboard), an analogue sensor designed and made by ISAS/JAXA, mounted 1.6 m
13   - from the end of the boom typically done in the Earth's magnetosphere.</Description>
  10 + <Description>The Fluxgate Magnetometer onboard Mio (MGF) measures the magnetic field to study various magnetospheric processes
  11 + (such as magnetic reconnection, field-aligned currents etc.) in Mercury’s magnetosphere, physics of bowshock and magnetosheath,
  12 + also magnetic field properties in the inner-heliosphere. It consists of two tir-axial fluxgate magnetometers and power supply units.
  13 + The magnetometer is able to observe the magnetic field with a vector rate of maximum 128 Hz. </Description>
14 14 <Contact>
15 15 <PersonID>spase://SMWG/Person/Wolfgang.Baumjohann</PersonID>
16 16 <Role>PrincipalInvestigator</Role>
17 17 </Contact>
18 18 <Contact>
19 19 <PersonID>spase://SMWG/Person/Ayako.Matsuoka</PersonID>
20   - <Role>CoInvestigator</Role>
  20 + <Role>CoPI</Role>
21 21 </Contact>
  22 + <InformationURL>
  23 + <Name>Mio Science Center</Name>
  24 + <URL>https://miosc.isee.nagoya-u.ac.jp/about/satellite/mgf.php</URL>
  25 + </InformationURL>
  26 + <InformationURL>
  27 + <Name>Baumjohann, W., Matsuoka, A., Narita, Y. et al. The BepiColombo–Mio Magnetometer en Route to Mercury. Space Sci Rev 216, 125 (2020).</Name>
  28 + <URL>https://doi.org/10.1007/s11214-020-00754-y</URL>
  29 + <Description>Reference paper</Description>
  30 + </InformationURL>
22 31 </ResourceHeader>
23 32 <InstrumentType>Magnetometer</InstrumentType>
24 33 <InvestigationName>Mercury Magnetometer on Mio</InvestigationName>
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Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml
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7 7 <ResourceName>MPPE/MIA</ResourceName>
8 8 <AlternateName>Mercury Ion Analyzer</AlternateName>
9 9 <ReleaseDate>2017-05-20T21:10:13Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>The Mercury Plasma Particle Experiment (MPPE) suite is a comprehensive instrument package to observe the solar wind at
  11 + Mercury’s position and the whole plasma environment at Mercury. It consists of seven sensors including Mercury Electron Analyzers
  12 + (MEA1 and MEA2), Mercury Ion Analyzer (MIA), Mass Spectrum Analyzer (MSA), High-Energy Particle instrument for electron (HEP-e),
  13 + High-Energy Particle instrument for ion (HEP-i), and Energetic Neutrals Analyzer (ENA).
  14 + These sensors measure plasma, high-energy particles and energetic neutral atoms with sufficiently high time resolution,
  15 + wide energy and dynamic range, wide angle coverage, and high mass resolution.
  16 +
  17 + Mercury Ion Analyzer (MIA), one of MPPE sensors onboard Mio, measures both the 3D distribution function of solar wind ions
  18 + around Mercury and the planet’s magnetospheric ions to understand the structure and plasma dynamics of Mercury’s magnetosphere,
  19 + Mercury-solar wind interaction, atmospheric abundances, structures, and generation/loss processes, and the solar wind at Mercury’s
  20 + position. MIA consists of a top-hat type electrostatic analyzer with toroidal deflectors, microchannel plates (MCPs),
  21 + high-voltage power supplies. The analyzer selects energies of ions from 10 eV/q up to 30 keV/q depending on the operation modes with 64
  22 + spin angle sectors.</Description>
11 23 <Contact>
12 24 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
13 25 <Role>PrincipalInvestigator</Role>
14   - </Contact>
  26 + </Contact>
  27 + <InformationURL>
  28 + <Name>Mio Science Center</Name>
  29 + <URL>https://miosc.isee.nagoya-u.ac.jp/about/satellite/mppe_mia.php</URL>
  30 + </InformationURL>
  31 + <InformationURL>
  32 + <Name>Saito, Y., Delcourt, D., Hirahara, M. et al. Pre-flight Calibration and Near-Earth Commissioning Results of the Mercury Plasma Particle Experiment (MPPE) Onboard MMO (Mio). Space Sci Rev 217, 70 (2021).</Name>
  33 + <URL>https://doi.org/10.1007/s11214-021-00839-2</URL>
  34 + <Description>Reference paper</Description>
  35 + </InformationURL>
15 36 </ResourceHeader>
16 37 <InstrumentType>ElectrostaticAnalyser</InstrumentType>
17 38 <InvestigationName>Mercury Ion Analyzer on Mio</InvestigationName>
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Instrument/CDPP-AMDA/BepiColombo/Mio/MSA.xml
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7 7 <ResourceName>MPPE/MSA</ResourceName>
8 8 <AlternateName>Mass Spectrum Analyzer</AlternateName>
9 9 <ReleaseDate>2017-05-20T21:10:13Z</ReleaseDate>
10   - <Description>ToDo</Description>
  10 + <Description>The Mercury Plasma Particle Experiment (MPPE) suite is a comprehensive instrument package to observe the solar wind at
  11 + Mercury’s position and the whole plasma environment at Mercury. It consists of seven sensors including Mercury Electron Analyzers
  12 + (MEA1 and MEA2), Mercury Ion Analyzer (MIA), Mass Spectrum Analyzer (MSA), High-Energy Particle instrument for electron (HEP-e),
  13 + High-Energy Particle instrument for ion (HEP-i), and Energetic Neutrals Analyzer (ENA).
  14 + These sensors measure plasma, high-energy particles and energetic neutral atoms with sufficiently high time resolution,
  15 + wide energy and dynamic range, wide angle coverage, and high mass resolution.
  16 +
  17 + The Mass Spectrum Analyzer (MSA) that is part of the MPPE consortium onboard Mio, measures mass resolved 3D distribution functions
  18 + of ions from 1 eV/q up to 38 keV/q. As such, it allows us to investigate the magnetospheric plasma dynamics and to characterize the c
  19 + ontribution of ions of planetary origin such as Na+ or K+. MSA consists of a spherical top-hat for energy per charge analysis,
  20 + followed by a polarized Time-Of-Flight chamber for mass per charge discrimination. The "reflectron" design adopted in this TOF chamber
  21 + leads to isochronous times of flight ; hence, an enhanced mass resolution (above 50) of the measured ions.</Description>
11 22 <Contact>
12 23 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
13 24 <Role>PrincipalInvestigator</Role>
14   - </Contact>
  25 + </Contact>
  26 + <Contact>
  27 + <PersonID>spase://CNES/Person/CDPP-AMDA/Dominique.Delcourt</PersonID>
  28 + <Role>CoPI</Role>
  29 + </Contact>
  30 + <InformationURL>
  31 + <Name>Mio Science Center</Name>
  32 + <URL>https://miosc.isee.nagoya-u.ac.jp/about/satellite/mppe_msa.php</URL>
  33 + </InformationURL>
  34 + <InformationURL>
  35 + <Name>Saito, Y., Delcourt, D., Hirahara, M. et al. Pre-flight Calibration and Near-Earth Commissioning Results of the Mercury Plasma Particle Experiment (MPPE) Onboard MMO (Mio). Space Sci Rev 217, 70 (2021).</Name>
  36 + <URL>https://doi.org/10.1007/s11214-021-00839-2</URL>
  37 + <Description>Reference paper</Description>
  38 + </InformationURL>
15 39 </ResourceHeader>
16 40 <InstrumentType>MassSpectrometer</InstrumentType>
17 41 <InvestigationName>Mass Spectrum Analyzer on Mio</InvestigationName>
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Instrument/CDPP-AMDA/BepiColombo/Models.xml
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6 6 <ResourceName>Analytical Models</ResourceName>
7 7 <AlternateName>KT17: Mercury magnetic field model</AlternateName>
8 8 <ReleaseDate>2023-06-21T09:40:40Z</ReleaseDate>
9   - <Description>Dynamic model of Mercury's magnetospheric magnetic field parameterized by heliocentric distance and magnetic activity</Description>
  9 + <Description>Dynamic model of Mercury's magnetospheric magnetic field parameterized by heliocentric distance and magnetic activity.</Description>
10 10 <Contact>
11 11 <PersonID>spase://CNES/Person/CDPP-AMDA/Haje.Korth</PersonID>
12 12 <Role>PrincipalInvestigator</Role>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-cruise-all.xml
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5 5 <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-cruise-all</ResourceID>
6 6 <ResourceHeader>
7 7 <ResourceName>cruise</ResourceName>
8   - <AlternateName>Bepi ephemeris during cruise phase</AlternateName>
  8 + <AlternateName>BepiColombo ephemeris during cruise phase</AlternateName>
9 9 <DOI>10.5270/esa-dwuc9bs</DOI>
10 10 <ReleaseDate>2023-06-20T14:02:24Z</ReleaseDate>
11   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  11 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  12 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
12 13 <Contact>
13 14 <PersonID>spase://CNES/Person/CDPP-AMDA/Marc.Sitja</PersonID>
14 15 <Role>PrincipalInvestigator</Role>
15 16 </Contact>
16 17 <InformationURL>
17   - <Name>Landing Page at ESAC</Name>
18   - <URL>https://doi.org/10.5270/esa-dwuc9bs</URL>
19   - </InformationURL>
  18 + <Name>ESA SPICE Service</Name>
  19 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  20 + </InformationURL>
20 21 </ResourceHeader>
21 22 <AccessInformation>
22 23 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-orb-earth.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Earth flyby</ResourceName>
8 8 <ReleaseDate>2021-07-20T06:08:31Z</ReleaseDate>
9   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  9 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  10 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Marc.Sitja</PersonID>
12 13 <Role>PrincipalInvestigator</Role>
13 14 </Contact>
  15 + <InformationURL>
  16 + <Name>ESA SPICE Service</Name>
  17 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  18 + </InformationURL>
14 19 </ResourceHeader>
15 20 <AccessInformation>
16 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-orb-mercury1.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Mercury flyby #1</ResourceName>
8 8 <ReleaseDate>2023-06-20T14:41:58Z</ReleaseDate>
9   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  9 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  10 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Benjamin.Renard</PersonID>
12 13 <Role>DataProducer</Role>
13 14 </Contact>
14 15 <InformationURL>
15   - <Name>Landing Page at ESAC</Name>
16   - <URL>https://doi.org/10.5270/esa-dwuc9bs</URL>
17   - </InformationURL>
  16 + <Name>ESA SPICE Service</Name>
  17 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  18 + </InformationURL>
18 19 </ResourceHeader>
19 20 <AccessInformation>
20 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-orb-mercury2.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Mercury flyby #2</ResourceName>
8 8 <ReleaseDate>2023-06-20T14:42:18Z</ReleaseDate>
9   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  9 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  10 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Benjamin.Renard</PersonID>
12 13 <Role>DataProducer</Role>
13 14 </Contact>
14 15 <InformationURL>
15   - <Name>Landing Page at ESAC</Name>
16   - <URL>https://doi.org/10.5270/esa-dwuc9bs</URL>
17   - </InformationURL>
  16 + <Name>ESA SPICE Service</Name>
  17 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  18 + </InformationURL>
18 19 </ResourceHeader>
19 20 <AccessInformation>
20 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-orb-mercury3.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Mercury flyby #3</ResourceName>
8 8 <ReleaseDate>2023-06-20T14:42:38Z</ReleaseDate>
9   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  9 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  10 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Benjamin.Renard</PersonID>
12 13 <Role>DataProducer</Role>
13 14 </Contact>
14 15 <InformationURL>
15   - <Name>Landing Page at ESAC</Name>
16   - <URL>https://doi.org/10.5270/esa-dwuc9bs</URL>
17   - </InformationURL>
  16 + <Name>ESA SPICE Service</Name>
  17 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  18 + </InformationURL>
18 19 </ResourceHeader>
19 20 <AccessInformation>
20 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-orb-venus1.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Venus flyby #1</ResourceName>
8 8 <ReleaseDate>2021-07-20T06:10:05Z</ReleaseDate>
9   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  9 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  10 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Benjamin.Renard</PersonID>
12 13 <Role>DataProducer</Role>
13 14 </Contact>
14 15 <InformationURL>
15   - <Name>Landing Page at ESAC</Name>
16   - <URL>https://doi.org/10.5270/esa-dwuc9bs</URL>
17   - </InformationURL>
  16 + <Name>ESA SPICE Service</Name>
  17 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  18 + </InformationURL>
18 19 </ResourceHeader>
19 20 <AccessInformation>
20 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
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NumericalData/CDPP-AMDA/BepiColombo/Ephemeris/bepi-orb-venus2.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Venus flyby #2</ResourceName>
8 8 <ReleaseDate>2021-07-20T06:11:24Z</ReleaseDate>
9   - <Description>Calculated in IRAP by using Bepi SPICE kernels</Description>
  9 + <Description>Calculated by IRAP using BepiColombo SPICE kernels</Description>
  10 + <Acknowledgement>Please acknowledge the European Space Agency, ESA, and the Japanese Aerospace Exploration Agency, JAXA.</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://CNES/Person/CDPP-AMDA/Benjamin.Renard</PersonID>
12 13 <Role>DataProducer</Role>
13 14 </Contact>
14 15 <InformationURL>
15   - <Name>Landing Page at ESAC</Name>
16   - <URL>https://doi.org/10.5270/esa-dwuc9bs</URL>
17   - </InformationURL>
  16 + <Name>ESA SPICE Service</Name>
  17 + <URL>https://www.cosmos.esa.int/web/spice/spice-for-bepicolombo</URL>
  18 + </InformationURL>
18 19 </ResourceHeader>
19 20 <AccessInformation>
20 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/MPO/MAG/bepi-mpo-earth.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Earth flyby</ResourceName>
8 8 <ReleaseDate>2020-09-22T13:30:15Z</ReleaseDate>
9   - <Description>THIS FILE CONTAINS DERIVED 1-SECOND-AVERAGED MAGNETIC FIELD VECTOR DATA OBTAINED BY THE OB
10   - MAGNETOMETER ABOARD THE BEPICOLOMBO MPO S/C. ALL FIELD VALUES ARE GROUND CALIBRATED DATA IN NANOTESLA AND
11   - AVERAGED TO 1-SECOND-MEAN VALUES.FIELD IS GIVEN IN ECLIPJ2000 COORDINATES.
12   - THESE DATA WERE CALCULATED USING THE RESULTS OF THE GROUND CALIBRATION ONLY. THIS MEANS THAT
13   - TEMPERATURE DEPENDENT SENSITIVITIES, MISALIGNMENT, AND OFFSETS OF THE INSTRUMENT ARE TAKEN INTO
14   - ACCOUNT. ALL S/C EFFECTS LIKE TIME DEPENDENT DISTURBANCES AND THE S/C MAGNETIC FIELD ARE NOT
15   - ELIMINATED YET. ONLY A STEPWISE CONSTANT ESTIMATE OF THE S/C FIELD IS SUBTRACTED.
16   - FOR PROPER SCIENTIFIC RESEARCH DERIVED INFLIGHT CALIBRATED DATA SHOULD BE USED</Description>
  9 + <Description>The BepiColombo Earth flyby took place on 10 April 2020. </Description>
17 10 <Contact>
18 11 <PersonID>spase://CNES/Person/CDPP-AMDA/Daniel.Heyner</PersonID>
19 12 <Role>PrincipalInvestigator</Role>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruiselet32m1.xml
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... ... @@ -6,11 +6,16 @@
6 6 <ResourceHeader>
7 7 <ResourceName>cruise</ResourceName>
8 8 <ReleaseDate>2022-03-28T14:00:23Z</ReleaseDate>
9   - <Description>ToDo</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 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
12 13 <Role>PrincipalInvestigator</Role>
13 14 </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
14 19 </ResourceHeader>
15 20 <AccessInformation>
16 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.xml
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6 6 <ResourceHeader>
7 7 <ResourceName>Earth flyby</ResourceName>
8 8 <ReleaseDate>2020-09-09T15:19:00Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>The BepiColombo Earth flyby took place on 10 April 2020. </Description>
  10 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
10 11 <Contact>
11 12 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
12 13 <Role>PrincipalInvestigator</Role>
13 14 </Contact>
  15 + <Contact>
  16 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  17 + <Role>DataProducer</Role>
  18 + </Contact>
14 19 </ResourceHeader>
15 20 <AccessInformation>
16 21 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.xml 0 → 100644
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... ... @@ -0,0 +1,82 @@
  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</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>Mercury flyby #1</ResourceName>
  8 + <ReleaseDate>2024-01-24T14:57:21Z</ReleaseDate>
  9 + <Description>The BepiColombo mission conducted the first of its six flybys of Mercury on 1 October 2021 and explored the southern
  10 + hemisphere of the magnetosphere of Mercury. BepiColombo entered the dusk side magnetosphere from the nightside and exited in the
  11 + dayside through the dawn side magnetosphere.</Description>
  12 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  13 + <Contact>
  14 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  15 + <Role>PrincipalInvestigator</Role>
  16 + </Contact>
  17 + <Contact>
  18 + <PersonID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</PersonID>
  19 + <Role>DataProducer</Role>
  20 + </Contact>
  21 + <Contact>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  23 + <Role>DataProducer</Role>
  24 + </Contact>
  25 + <InformationURL>
  26 + <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>
  27 + <URL>https://doi.org/10.5281/zenodo.7926905</URL>
  28 + </InformationURL>
  29 + </ResourceHeader>
  30 + <AccessInformation>
  31 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  32 + <Availability>Online</Availability>
  33 + <AccessRights>Restricted</AccessRights>
  34 + <AccessURL>
  35 + <Name>CDPP/AMDA HAPI Server</Name>
  36 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  37 + <Style>HAPI</Style>
  38 + <Description>Web Service to this product using the HAPI interface.</Description>
  39 + </AccessURL>
  40 + <Format>CSV</Format>
  41 + <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>
  42 + </AccessInformation>
  43 + <AccessInformation>
  44 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  45 + <Availability>Online</Availability>
  46 + <AccessRights>Restricted</AccessRights>
  47 + <AccessURL>
  48 + <Name>CDPP/AMDA Web application</Name>
  49 + <URL>http://amda.cdpp.eu</URL>
  50 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  51 + </AccessURL>
  52 + <Format>CSV</Format>
  53 + <Format>VOTable</Format>
  54 + <Format>CDF</Format>
  55 + <Format>PNG</Format>
  56 + <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>
  57 + </AccessInformation>
  58 + <ProviderName>IRAP</ProviderName>
  59 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA</InstrumentID>
  60 + <MeasurementType>ThermalPlasma</MeasurementType>
  61 + <TemporalDescription>
  62 + <TimeSpan>
  63 + <StartDate>2020-10-15T00:00:00Z</StartDate>
  64 + <StopDate>2020-10-15T07:13:20Z</StopDate>
  65 + </TimeSpan>
  66 + <CadenceMin>PT1S</CadenceMin>
  67 + </TemporalDescription>
  68 + <ObservedRegion>Mercury</ObservedRegion>
  69 + <Parameter>
  70 + <Name>cnts</Name>
  71 + <ParameterKey>mia_venus1_let4m23</ParameterKey>
  72 + <Units>cnts</Units>
  73 + <RenderingHints>
  74 + <DisplayType>Spectrogram</DisplayType>
  75 + </RenderingHints>
  76 + <Particle>
  77 + <ParticleType>Ion</ParticleType>
  78 + <ParticleQuantity>Counts</ParticleQuantity>
  79 + </Particle>
  80 + </Parameter>
  81 + </NumericalData>
  82 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.xml
  Diff comments   View file @3cc563a
... ... @@ -6,11 +6,17 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Venus flyby #1</ResourceName>
8 8 <ReleaseDate>2021-07-30T14:57:21Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled
  10 + along the induced magnetotail.</Description>
  11 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
10 12 <Contact>
11 13 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
12 14 <Role>PrincipalInvestigator</Role>
13 15 </Contact>
  16 + <Contact>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  18 + <Role>DataProducer</Role>
  19 + </Contact>
14 20 </ResourceHeader>
15 21 <AccessInformation>
16 22 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.xml
  Diff comments   View file @3cc563a
... ... @@ -6,11 +6,25 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Venus flyby #2</ResourceName>
8 8 <ReleaseDate>2021-10-12T14:04:46Z</ReleaseDate>
9   - <Description>ToDo</Description>
  9 + <Description>The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath
  10 + from the nightside down to the almost unexplored subsolar region.</Description>
  11 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
10 12 <Contact>
11 13 <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
12 14 <Role>PrincipalInvestigator</Role>
13 15 </Contact>
  16 + <Contact>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Moa.Persson </PersonID>
  18 + <Role>DataProducer</Role>
  19 + </Contact>
  20 + <Contact>
  21 + <PersonID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</PersonID>
  22 + <Role>DataProducer</Role>
  23 + </Contact>
  24 + <InformationURL>
  25 + <Name>Persson, M., BepiColombo VFB2 team (full team added in description). (2022). Supplementary data for "BepiColombo mission confirms stagnation region of Venus and reveals its large extent" [Data set]. Zenodo.</Name>
  26 + <URL>https://doi.org/10.5281/zenodo.7297140</URL>
  27 + </InformationURL>
14 28 </ResourceHeader>
15 29 <AccessInformation>
16 30 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MSA/bepi-msa-cruise.xml
  Diff comments   View file @3cc563a
... ... @@ -6,11 +6,24 @@
6 6 <ResourceHeader>
7 7 <ResourceName>cruise</ResourceName>
8 8 <ReleaseDate>2022-04-04T14:28:18Z</ReleaseDate>
9   - <Description>ToDo</Description>
10   - <Contact>
11   - <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
12   - <Role>PrincipalInvestigator</Role>
13   - </Contact>
  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/Dominique.Delcourt</PersonID>
  17 + <Role>CoPI</Role>
  18 + </Contact>
  19 + <Contact>
  20 + <PersonID>spase://CNES/Person/CDPP-AMDA/Lina.Hadid</PersonID>
  21 + <Role>DataProducer</Role>
  22 + </Contact>
  23 + <Contact>
  24 + <PersonID>spase://CNES/Person/CDPP-AMDA/Bruno.Katra</PersonID>
  25 + <Role>DataProducer</Role>
  26 + </Contact>
14 27 </ResourceHeader>
15 28 <AccessInformation>
16 29 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MSA/bepi-msa-mercury1.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,118 @@
  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://amda.irap.omp.eu/public/schemas/spase-2.4.1.xsd">
  3 + <Version>2.4.1</Version>
  4 + <NumericalData>
  5 + <ResourceID>spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MSA/bepi-msa-mercury1</ResourceID>
  6 + <ResourceHeader>
  7 + <ResourceName>Mercury flyby #1</ResourceName>
  8 + <ReleaseDate>2024-01-24T14:05:41Z</ReleaseDate>
  9 + <Description>The BepiColombo mission conducted the first of its six flybys of Mercury on 1 October 2021 and explored the southern
  10 + hemisphere of the magnetosphere of Mercury. BepiColombo entered the dusk side magnetosphere from the nightside and exited in the
  11 + dayside through the dawn side magnetosphere.</Description>
  12 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  13 + <Contact>
  14 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  15 + <Role>PrincipalInvestigator</Role>
  16 + </Contact>
  17 + <Contact>
  18 + <PersonID>spase://CNES/Person/CDPP-AMDA/Dominique.Delcourt</PersonID>
  19 + <Role>CoPI</Role>
  20 + </Contact>
  21 + <Contact>
  22 + <PersonID>spase://CNES/Person/CDPP-AMDA/Lina.Hadid</PersonID>
  23 + <Role>DataProducer</Role>
  24 + </Contact>
  25 + <Contact>
  26 + <PersonID>spase://CNES/Person/CDPP-AMDA/Bruno.Katra</PersonID>
  27 + <Role>DataProducer</Role>
  28 + </Contact>
  29 + </ResourceHeader>
  30 + <AccessInformation>
  31 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  32 + <Availability>Online</Availability>
  33 + <AccessRights>Restricted</AccessRights>
  34 + <AccessURL>
  35 + <Name>CDPP/AMDA HAPI Server</Name>
  36 + <URL>http://amda.irap.omp.eu/service/hapi</URL>
  37 + <Style>HAPI</Style>
  38 + <Description>Web Service to this product using the HAPI interface.</Description>
  39 + </AccessURL>
  40 + <Format>CSV</Format>
  41 + <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>
  42 + </AccessInformation>
  43 + <AccessInformation>
  44 + <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
  45 + <Availability>Online</Availability>
  46 + <AccessRights>Restricted</AccessRights>
  47 + <AccessURL>
  48 + <Name>CDPP/AMDA Web application</Name>
  49 + <URL>http://amda.cdpp.eu</URL>
  50 + <Description>Access to Data via CDPP/AMDA Web application.</Description>
  51 + </AccessURL>
  52 + <Format>CSV</Format>
  53 + <Format>VOTable</Format>
  54 + <Format>CDF</Format>
  55 + <Format>PNG</Format>
  56 + <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>
  57 + </AccessInformation>
  58 + <ProviderName>LPP</ProviderName>
  59 + <InstrumentID>spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MSA</InstrumentID>
  60 + <MeasurementType>IonComposition</MeasurementType>
  61 + <TemporalDescription>
  62 + <TimeSpan>
  63 + <StartDate>2021-08-10T12:00:00Z</StartDate>
  64 + <StopDate>2021-08-10T13:59:28Z</StopDate>
  65 + </TimeSpan>
  66 + <CadenceMin>PT64S</CadenceMin>
  67 + </TemporalDescription>
  68 + <ObservedRegion>Venus</ObservedRegion>
  69 + <Parameter>
  70 + <Name>alpha : cnts</Name>
  71 + <ParameterKey>msa_venus2_alpha</ParameterKey>
  72 + <Units>cnts</Units>
  73 + <RenderingHints>
  74 + <DisplayType>Spectrogram</DisplayType>
  75 + </RenderingHints>
  76 + <Particle>
  77 + <ParticleType>AlphaParticle</ParticleType>
  78 + <ParticleQuantity>Counts</ParticleQuantity>
  79 + </Particle>
  80 + </Parameter>
  81 + <Parameter>
  82 + <Name>heavy : cnts</Name>
  83 + <ParameterKey>msa_venus2_heavy</ParameterKey>
  84 + <Units>cnts</Units>
  85 + <RenderingHints>
  86 + <DisplayType>Spectrogram</DisplayType>
  87 + </RenderingHints>
  88 + <Particle>
  89 + <ParticleType>Ion</ParticleType>
  90 + <ParticleQuantity>Counts</ParticleQuantity>
  91 + </Particle>
  92 + </Parameter>
  93 + <Parameter>
  94 + <Name>protons : cnts</Name>
  95 + <ParameterKey>msa_venus2_protons</ParameterKey>
  96 + <Units>cnts</Units>
  97 + <RenderingHints>
  98 + <DisplayType>Spectrogram</DisplayType>
  99 + </RenderingHints>
  100 + <Particle>
  101 + <ParticleType>Proton</ParticleType>
  102 + <ParticleQuantity>Counts</ParticleQuantity>
  103 + </Particle>
  104 + </Parameter>
  105 + <Parameter>
  106 + <Name>total : cnts</Name>
  107 + <ParameterKey>msa_venus2_total</ParameterKey>
  108 + <Units>cnts</Units>
  109 + <RenderingHints>
  110 + <DisplayType>Spectrogram</DisplayType>
  111 + </RenderingHints>
  112 + <Particle>
  113 + <ParticleType>Ion</ParticleType>
  114 + <ParticleQuantity>Counts</ParticleQuantity>
  115 + </Particle>
  116 + </Parameter>
  117 + </NumericalData>
  118 +</Spase>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Mio/MSA/bepi-msa-venus2.xml
  Diff comments   View file @3cc563a
... ... @@ -6,11 +6,25 @@
6 6 <ResourceHeader>
7 7 <ResourceName>Venus flyby #2</ResourceName>
8 8 <ReleaseDate>2021-10-12T14:05:41Z</ReleaseDate>
9   - <Description>ToDo</Description>
10   - <Contact>
11   - <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
12   - <Role>PrincipalInvestigator</Role>
13   - </Contact>
  9 + <Description>The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath
  10 + from the nightside down to the almost unexplored subsolar region.</Description>
  11 + <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement>
  12 + <Contact>
  13 + <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID>
  14 + <Role>PrincipalInvestigator</Role>
  15 + </Contact>
  16 + <Contact>
  17 + <PersonID>spase://CNES/Person/CDPP-AMDA/Dominique.Delcourt</PersonID>
  18 + <Role>CoPI</Role>
  19 + </Contact>
  20 + <Contact>
  21 + <PersonID>spase://CNES/Person/CDPP-AMDA/Lina.Hadid</PersonID>
  22 + <Role>DataProducer</Role>
  23 + </Contact>
  24 + <Contact>
  25 + <PersonID>spase://CNES/Person/CDPP-AMDA/Bruno.Katra</PersonID>
  26 + <Role>DataProducer</Role>
  27 + </Contact>
14 28 </ResourceHeader>
15 29 <AccessInformation>
16 30 <RepositoryID>spase://SMWG/Repository/CDPP/AMDA</RepositoryID>
... ...
NumericalData/CDPP-AMDA/BepiColombo/Models/bepi-kt17-model1.xml
  Diff comments   View file @3cc563a
... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>Mercury flyby #1</ResourceName>
8 8 <AlternateName>KT17 mercury magnetic field model for flyby #1</AlternateName>
9 9 <ReleaseDate>2023-06-20T14:41:58Z</ReleaseDate>
10   - <Description>Magnetic field along S/C orbit at Mercury is being real-time calculated.
  10 + <Description>Magnetic field along S/C orbit at Mercury, custom calculation.
  11 +
11 12 S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user.
12 13  
13 14 KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
... ...
NumericalData/CDPP-AMDA/BepiColombo/Models/bepi-kt17-model2.xml
  Diff comments   View file @3cc563a
... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>Mercury flyby #2</ResourceName>
8 8 <AlternateName>KT17 mercury magnetic field model for flyby #2</AlternateName>
9 9 <ReleaseDate>2023-06-20T14:42:18Z</ReleaseDate>
10   - <Description>Magnetic field along S/C orbit at Mercury is being real-time calculated.
  10 + <Description>Magnetic field along S/C orbit at Mercury, custom calculation.
  11 +
11 12 S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user.
12 13  
13 14 KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
... ...
NumericalData/CDPP-AMDA/BepiColombo/Models/bepi-kt17-model3.xml
  Diff comments   View file @3cc563a
... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>Mercury flyby #3</ResourceName>
8 8 <AlternateName>KT17 mercury magnetic field model for flyby #3</AlternateName>
9 9 <ReleaseDate>2023-06-20T14:42:38Z</ReleaseDate>
10   - <Description>Magnetic field along S/C orbit at Mercury is being real-time calculated.
  10 + <Description>Magnetic field along S/C orbit at Mercury, custom calculation.
  11 +
11 12 S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user.
12 13  
13 14 KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
... ...
NumericalData/CDPP-AMDA/MESSENGER/Models/mes-kt17-model.xml
  Diff comments   View file @3cc563a
... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>KT17 model</ResourceName>
8 8 <AlternateName>KT17 mercury magnetic field model</AlternateName>
9 9 <ReleaseDate>2016-04-04T16:53:40Z</ReleaseDate>
10   - <Description>Magnetic field along Mercury orbit is being real-time calculated.
  10 + <Description>Magnetic field along S/C orbit at Mercury, custom calculation.
  11 +
11 12 S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user.
12 13  
13 14 KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
... ...
NumericalData/CDPP-AMDA/Mariner10/Models/m10-kt17-model.xml
  Diff comments   View file @3cc563a
... ... @@ -7,7 +7,8 @@
7 7 <ResourceName>KT17 model</ResourceName>
8 8 <AlternateName>KT17 mercury magnetic field model</AlternateName>
9 9 <ReleaseDate>2021-02-12T09:12:39Z</ReleaseDate>
10   - <Description>Magnetic field along Mercury orbit is being real-time calculated.
  10 + <Description>Magnetic field along S/C orbit at Mercury, custom calculation.
  11 +
11 12 S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user.
12 13  
13 14 KT17 magnetic field model (Korth et al., 2017) model is used in calculations.
... ...
Observatory/CDPP-AMDA/BepiColombo/MPO.xml
  Diff comments   View file @3cc563a
... ... @@ -7,17 +7,21 @@
7 7 <ResourceName>MPO</ResourceName>
8 8 <AlternateName>Mercury Planetary Orbiter</AlternateName>
9 9 <ReleaseDate>2019-03-01T20:05:54Z</ReleaseDate>
10   - <Description>The BepiColombo project is a large-scale mission to perform a comprehensive study on Mercury including its magnetic field, magnetosphere, interior and surface.
11   -
12   -The Mercury Planetary Orbiter (MPO) is ESA's scientific contribution to the mission.
  10 + <Description>BepiColombo consists of two spacecraft, the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (Mio).
  11 + The MPO will focus on geology, planetary composition, inner structure, and the exosphere of Mercury.
13 12 </Description>
14 13 <Contact>
15 14 <PersonID>spase://CNES/Person/CDPP-AMDA/J.Benkhoff</PersonID>
16 15 <Role>ProjectScientist</Role>
17 16 </Contact>
18 17 <InformationURL>
19   - <Name>Home page</Name>
20   - <URL>http://sci.esa.int/bepicolombo</URL>
  18 + <Name>ESA Website</Name>
  19 + <URL>https://www.esa.int/Science_Exploration/Space_Science/BepiColombo</URL>
  20 + </InformationURL>
  21 + <InformationURL>
  22 + <Name>Benkhoff, J., Murakami, G., Baumjohann, W. et al. BepiColombo - Mission Overview and Science Goals. Space Sci Rev 217, 90 (2021).</Name>
  23 + <URL>https://doi.org/10.1007/s11214-021-00861-4</URL>
  24 + <Description>Reference paper</Description>
21 25 </InformationURL>
22 26 </ResourceHeader>
23 27 <ObservatoryGroupID>spase://CNES/Observatory/CDPP-AMDA/BepiColombo</ObservatoryGroupID>
... ...
Person/CDPP-AMDA/Bruno.Katra.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,11 @@
  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 +<Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Bruno.Katra</ResourceID>
  6 + <ReleaseDate>2024-01-24T00:00:00Z</ReleaseDate>
  7 + <PersonName>Dr. Bruno Katra</PersonName>
  8 + <OrganizationName>Laboratoire de Physique des Plasmas (LPP, UMR 7648)</OrganizationName>
  9 + <Email>bruno.katra@lpp.polytechnique.fr</Email>
  10 + </Person>
  11 +</Spase>
... ...
Person/CDPP-AMDA/Dominique.Delcourt.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,11 @@
  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 +<Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Dominique.Delcourt</ResourceID>
  6 + <ReleaseDate>2024-01-24T00:00:00Z</ReleaseDate>
  7 + <PersonName>Dr. Dominique Delcourt</PersonName>
  8 + <OrganizationName>Laboratoire de Physique des Plasmas (LPP, UMR 7648)</OrganizationName>
  9 + <Email>dominique.delcourt@lpp.polytechnique.fr</Email>
  10 + </Person>
  11 +</Spase>
... ...
Person/CDPP-AMDA/Jonas.Rabia.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,10 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" 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 + <Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Jonas.Rabia</ResourceID>
  6 + <PersonName>Mr. Jonas Rabia</PersonName>
  7 + <OrganizationName>IRAP, Toulouse</OrganizationName>
  8 + <Email>Jonas.Rabia@irap.omp.eu</Email>
  9 + </Person>
  10 +</Spase>
... ...
Person/CDPP-AMDA/Lina.Hadid.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,11 @@
  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 +<Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Lina.Hadid</ResourceID>
  6 + <ReleaseDate>2024-01-24T00:00:00Z</ReleaseDate>
  7 + <PersonName>Dr. Lina Hadid</PersonName>
  8 + <OrganizationName>Laboratoire de Physique des Plasmas (LPP, UMR 7648)</OrganizationName>
  9 + <Email>lina.hadid@lpp.polytechnique.fr</Email>
  10 + </Person>
  11 +</Spase>
... ...
Person/CDPP-AMDA/Mathias.Rojo.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,10 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" 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 + <Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Mathias.Rojo</ResourceID>
  6 + <PersonName>Dr. Mathias Rojo</PersonName>
  7 + <OrganizationName>IRAP, Toulouse</OrganizationName>
  8 + <Email>Mathias.Rojo@irap.omp.eu</Email>
  9 + </Person>
  10 +</Spase>
... ...
Person/CDPP-AMDA/Sae.Aizawa.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,11 @@
  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 +<Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Sae.Aizawa</ResourceID>
  6 + <ReleaseDate>2024-01-24T00:00:00Z</ReleaseDate>
  7 + <PersonName>Dr. Sae Aizawa</PersonName>
  8 + <OrganizationName>Laboratoire de Physique des Plasmas (LPP, UMR 7648)</OrganizationName>
  9 + <Email>sae.aizawa@lpp.polytechnique.fr</Email>
  10 + </Person>
  11 +</Spase>
... ...
Person/CDPP-AMDA/Yuki.Harada.xml 0 → 100644
  Diff comments   View file @3cc563a
... ... @@ -0,0 +1,11 @@
  1 +<?xml version="1.0" encoding="UTF-8"?>
  2 +<Spase xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.spase-group.org/data/schema" xsi:schemaLocation="http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_0.xsd">
  3 + <Version>2.4.1</Version>
  4 + <Person>
  5 + <ResourceID>spase://CNES/Person/CDPP-AMDA/Yuki.Harada</ResourceID>
  6 + <ReleaseDate>2024-01-24T17:35:48Z</ReleaseDate>
  7 + <PersonName>Dr. Yuki Harada</PersonName>
  8 + <OrganizationName>Kyoto University</OrganizationName>
  9 + <Email>haraday@kugi.kyoto-u.ac.jp</Email>
  10 + </Person>
  11 +</Spase>
... ...