2.4.1 spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-cruise.l1p.et.all L1p - Et ALL sector 2024-04-10T12:07:26Z 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 PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/Sae.Aizawa DataProducer spase://CNES/Person/CDPP-AMDA/Yuki.Harada DataProducer Aizawa, S., Harada, Y., André, N., Saito, Y., Barabash, S., Delcourt, D., Sauvaud, J.-A., Barthe, A., Fedorov, A., Penou, E., Yokota, S., Miyake, W., Persson, M., Nenon, Q., Rojo, M., Futaana, Y., Asamura, K., Shimoyama, M., Hadid, L., … Murakami, G. (2023). Direct evidence of substorm-related impulsive injections of electrons at Mercury (version 1) [Data set]. Zenodo. https://doi.org/10.5281/zenodo.7926905 bepi-mia-cruise PartOf cruise spase://SMWG/Repository/CDPP/AMDA Online Restricted CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi bepi-mia-cruise.l1p.et.all Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Restricted CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. JAXA spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA ThermalPlasma 2022-03-11T16:32:15Z 2022-03-11T16:32:15Z PT4S Heliosphere counts dir1 mia_cruise_l1petall_d1 Raw counts SpinSectorGroup0,7 counts/sample Spectrogram Ion Counts counts dir2 mia_cruise_l1petall_d2 Raw counts SpinSectorGroup1-2 counts/sample Spectrogram Ion Counts counts dir3 mia_cruise_l1petall_d3 Raw counts SpinSectorGroup3-4 counts/sample Spectrogram Ion Counts counts dir4 mia_cruise_l1petall_d4 Raw counts SpinSectorGroup5-6 counts/sample Spectrogram Ion Counts diff E flux dir1 mia_cruise_l1petall_fluxd1 Omni-directional Differential Energy Flux, SpinSectorGroup0,7 eV/cm^2/s/sr/eV Spectrogram Ion EnergyFlux diff E flux dir2 mia_cruise_l1petall_fluxd2 Omni-directional Differential Energy Flux, SpinSectorGroup1-2 eV/cm^2/s/sr/eV Spectrogram Ion EnergyFlux diff E flux dir3 mia_cruise_l1petall_fluxd3 Omni-directional Differential Energy Flux, SpinSectorGroup3-4 eV/cm^2/s/sr/eV Spectrogram Ion EnergyFlux diff E flux dir4 mia_cruise_l1petall_fluxd4 Omni-directional Differential Energy Flux, SpinSectorGroup5-6 eV/cm^2/s/sr/eV Spectrogram Ion EnergyFlux