Commit 4c062c1c08c39396ed564c441130b9bd85f1c57b
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a931c2d5
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Finalize BEPI/MIA + cleanup
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Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml
| ... | ... | @@ -19,7 +19,14 @@ |
| 19 | 19 | Mercury-solar wind interaction, atmospheric abundances, structures, and generation/loss processes, and the solar wind at Mercury’s |
| 20 | 20 | position. MIA consists of a top-hat type electrostatic analyzer with toroidal deflectors, microchannel plates (MCPs), |
| 21 | 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> | |
| 22 | + spin angle sectors. | |
| 23 | + | |
| 24 | + ==== Data Procucts: ==== | |
| 25 | + | |
| 26 | + MIA LEVEL1 CDF files consist of three sub-levels: | |
| 27 | + * l1: Raw data with minimal processing for an archive purpose. Not useful for most users. Logarithmically compressed counts of E-t products are not uncompressed. Onboard velocity moments are stored as CDF_UNIT2 and are not converted to physical units. | |
| 28 | + * l1p: Data preliminarily converted to physical units. Background counts are not subtracted. May be used for preliminary analysis with great caution. | |
| 29 | + * l1p2: Calibrated data in physical units. Background counts are subtracted. Will be converted to LEVEL2 data with full metadata by Nagoya Mio Science Center.</Description> | |
| 23 | 30 | <Contact> |
| 24 | 31 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> |
| 25 | 32 | <Role>PrincipalInvestigator</Role> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et ALL sector</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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1p - Et ALL sector</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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 Earth flyby took place on 10 April 2020.</Description> | |
| 9 | + <Description>The BepiColombo Earth flyby took place on 10 April 2020. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m3.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 Earth flyby took place on 10 April 2020.</Description> | |
| 9 | + <Description>The BepiColombo Earth flyby took place on 10 April 2020. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et ALL sector</ResourceName> |
| 8 | 8 | <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate> |
| 9 | - <Description>The BepiColombo Earth flyby took place on 10 April 2020.</Description> | |
| 9 | + <Description>The BepiColombo Earth flyby took place on 10 April 2020. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et SW ALL</ResourceName> |
| 8 | 8 | <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate> |
| 9 | - <Description>The BepiColombo Earth flyby took place on 10 April 2020.</Description> | |
| 9 | + <Description>The BepiColombo Earth flyby took place on 10 April 2020. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - velocity moment all</ResourceName> |
| 8 | 8 | <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate> |
| 9 | - <Description>The BepiColombo Earth flyby took place on 10 April 2020.</Description> | |
| 9 | + <Description>The BepiColombo Earth flyby took place on 10 April 2020. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - velocity moment SW</ResourceName> |
| 8 | 8 | <ReleaseDate>2024-02-23T14:57:21Z</ReleaseDate> |
| 9 | - <Description>The BepiColombo Earth flyby took place on 10 April 2020.</Description> | |
| 9 | + <Description>The BepiColombo Earth flyby took place on 10 April 2020. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m3.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1p - Et ALL sector</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m3.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1p - Et ALL sector</ResourceName> |
| 8 | 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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 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> | |
| 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). | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m3.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - 3D count M1 mode</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m3.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - 3D count M3 mode</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et ALL sector</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et SW ALL</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.l1p.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1p - Et ALL sector</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - velocity moment all</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - velocity moment SW</ResourceName> |
| 8 | 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> | |
| 9 | + <Description>The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m1.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - 3D count M1 mode</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m3.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - 3D count M3 mode</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et ALL sector</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.swall.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - Et SW ALL</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.l1p.et.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1p - Et ALL sector</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.all.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - velocity moment all</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels without mechanical attenuation grid (all channels) in M1, M2, and M3 modes (Solar Wind and Magnetospheric Ion Modes combined).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |
NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.sw.xml
| ... | ... | @@ -6,7 +6,9 @@ |
| 6 | 6 | <ResourceHeader> |
| 7 | 7 | <ResourceName>L1 - velocity moment SW</ResourceName> |
| 8 | 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> | |
| 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. | |
| 10 | + | |
| 11 | +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode).</Description> | |
| 10 | 12 | <Acknowledgement>MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI)</Acknowledgement> |
| 11 | 13 | <Contact> |
| 12 | 14 | <PersonID>spase://SMWG/Person/Yoshifumi.Saito</PersonID> | ... | ... |