diff --git a/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml b/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml index ed46308..3fb4051 100644 --- a/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml +++ b/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA.xml @@ -19,7 +19,14 @@ Mercury-solar wind interaction, atmospheric abundances, structures, and generation/loss processes, and the solar wind at Mercury’s position. MIA consists of a top-hat type electrostatic analyzer with toroidal deflectors, microchannel plates (MCPs), 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 - spin angle sectors. + spin angle sectors. + + ==== Data Procucts: ==== + + MIA LEVEL1 CDF files consist of three sub-levels: + * 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. + * l1p: Data preliminarily converted to physical units. Background counts are not subtracted. May be used for preliminary analysis with great caution. + * l1p2: Calibrated data in physical units. Background counts are subtracted. Will be converted to LEVEL2 data with full metadata by Nagoya Mio Science Center. spase://SMWG/Person/Yoshifumi.Saito PrincipalInvestigator diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.3dc.m1.xml index 6f1d925..4e2de57 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - 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. + 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. + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all.xml index af62737..1d106fc 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - 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. + 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. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.swall.xml index cb8de4a..964ae13 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - 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. + 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. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all.xml index 23d4886..94a8d20 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all.xml @@ -6,7 +6,9 @@ L1p - Et ALL sector 2024-02-23T14:57:21Z - 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. + 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. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.all.xml index 6d79e1a..5a770e8 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - 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. + 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. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.sw.xml index bd532c5..49fa4d2 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - 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. + 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. + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m1.xml index 28041fa..53ea0c3 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - The BepiColombo Earth flyby took place on 10 April 2020. + The BepiColombo Earth flyby took place on 10 April 2020. + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m3.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m3.xml index d955c72..e12fe2d 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m3.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.3dc.m3.xml @@ -6,7 +6,9 @@ L1 - 3D count M3 mode 2024-02-23T14:57:21Z - The BepiColombo Earth flyby took place on 10 April 2020. + The BepiColombo Earth flyby took place on 10 April 2020. + +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.all.xml index effe23b..d57be5e 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - The BepiColombo Earth flyby took place on 10 April 2020. + The BepiColombo Earth flyby took place on 10 April 2020. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.swall.xml index a1b3797..0b4718c 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - The BepiColombo Earth flyby took place on 10 April 2020. + The BepiColombo Earth flyby took place on 10 April 2020. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.all.xml index 58d8b7e..13a2f19 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - The BepiColombo Earth flyby took place on 10 April 2020. + The BepiColombo Earth flyby took place on 10 April 2020. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.sw.xml index 6198e55..c07ed51 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-earth.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - The BepiColombo Earth flyby took place on 10 April 2020. + The BepiColombo Earth flyby took place on 10 April 2020. + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m1.xml index aa63218..84f5a07 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - 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. + 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. + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m3.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m3.xml index 1eb962c..a6c901c 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m3.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.3dc.m3.xml @@ -6,7 +6,9 @@ L1 - 3D count M3 mode 2024-02-23T14:57:21Z - 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. + 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. + +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.all.xml index b536550..e80dad9 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - 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. + 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. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.swall.xml index f1ff1b4..6c26aed 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - 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. + 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. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all.xml index f9c934c..46c8074 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.l1p.et.all.xml @@ -6,7 +6,9 @@ L1p - Et ALL sector 2024-02-23T14:57:21Z - 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. + 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. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.all.xml index 9d78de5..640a934 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - 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. + 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. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.sw.xml index a53536f..9af5ec3 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury1.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - 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. + 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. + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m1.xml index 941760f..5892068 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m3.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m3.xml index 3c95233..b34a70d 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m3.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.3dc.m3.xml @@ -6,7 +6,9 @@ L1 - 3D count M3 mode 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.all.xml index b52ea73..feebb3b 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.swall.xml index 3973f4a..6e91442 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode 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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all.xml index 9647be3..ac998df 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.l1p.et.all.xml @@ -6,7 +6,9 @@ L1p - Et ALL sector 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.all.xml index 30fd674..404e60b 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode 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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.sw.xml index 6a69162..b64ab98 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - 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). + The BepiColombo mission conducted the second of its six flybys of Mercury on 23 June 2022. Like the first encounter with Mercury that took place on October 1st 2021, the spacecraft approached the planet from dusk-nightside to dawn-dayside down to an extremely close distance (within about 200 km altitude from the planet surface). + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m1.xml index 3e84ab8..96fc314 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - 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. + 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. + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m3.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m3.xml index 2f0bb2f..719311b 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m3.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.3dc.m3.xml @@ -6,7 +6,9 @@ L1 - 3D count M3 mode 2024-02-23T14:57:21Z - 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. + 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. + +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.all.xml index 8dffa73..97780cb 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - 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. + 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. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.swall.xml index 72cbe46..748d1dd 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - 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. + 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. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.all.xml index 2e11436..1c5bc11 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - 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. + 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. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.sw.xml index aae20f0..a68f5b5 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury3.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - 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. + 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. + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m1.xml index 8ad9fc5..a595201 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m3.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m3.xml index bb6bf96..366a584 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m3.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.3dc.m3.xml @@ -6,7 +6,9 @@ L1 - 3D count M3 mode 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.all.xml index 66defdc..4cd0645 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.swall.xml index 5ea5f0e..5d3fc91 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.l1p.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.l1p.et.all.xml index ebd54ee..136ff35 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.l1p.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.l1p.et.all.xml @@ -6,7 +6,9 @@ L1p - Et ALL sector 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.all.xml index 2c26f95..dc97f78 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.sw.xml index 5f9dcb0..264b859 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus1.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + The first BepiColombo Venus flyby took place on 15 October 2020. After passing the bow shock, BepiColombo travelled along the induced magnetotail. + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m1.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m1.xml index 2522910..f72e953 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m1.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m1.xml @@ -6,7 +6,9 @@ L1 - 3D count M1 mode 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode 3D velocity distribution function data in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m3.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m3.xml index 754b08a..1afcc9e 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m3.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.3dc.m3.xml @@ -6,7 +6,9 @@ L1 - 3D count M3 mode 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode 3D velocity distribution function data in M1 mode (Magnetospheric Ion Low Angular Resolution Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.all.xml index cd3cb51..b2bcafa 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.all.xml @@ -6,7 +6,9 @@ L1 - Et ALL sector 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.swall.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.swall.xml index 2a2997a..3cc1777 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.swall.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.et.swall.xml @@ -6,7 +6,9 @@ L1 - Et SW ALL 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode energy-time spectrogram data from anode channels with mechanical attenuation grid (sw channels) and without mechanical attenuation grid (all channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.l1p.et.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.l1p.et.all.xml index a5c1737..afda280 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.l1p.et.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.l1p.et.all.xml @@ -6,7 +6,9 @@ L1p - Et ALL sector 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode energy-time spectrogram data from anode channels without mechanical attenuation grid (all channels) in M2 and M3 modes (Magnetospheric Ion Modes). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.all.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.all.xml index 46b59ef..f1c6e63 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.all.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.all.xml @@ -6,7 +6,9 @@ L1 - velocity moment all 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode 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). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito diff --git a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.sw.xml b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.sw.xml index 7bee666..dda7e91 100644 --- a/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.sw.xml +++ b/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-venus2.vm.sw.xml @@ -6,7 +6,9 @@ L1 - velocity moment SW 2024-02-23T14:57:21Z - 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. + The second BepiColombo Venus flyby took place on 10 August 2021. BepiColombo passed through the Venusian magnetosheath from the nightside down to the almost unexplored subsolar region. + +L mode onboard velocity moment data from anode channels with mechanical attenuation grid (sw channels) in M1 mode (Solar Wind Mode). MPPE is funded by JAXA, CNES, the Center National de la Recherche scientifique (CNRS, France), the Italian Space Agency (ASI) spase://SMWG/Person/Yoshifumi.Saito -- libgit2 0.21.2