2.4.1 spase://CNES/NumericalData/CDPP-AMDA/BepiColombo/Mio/MIA/bepi-mia-mercury2.vm.sw 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). 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 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-mercury2 PartOf Mercury flyby #2 spase://SMWG/Repository/CDPP/AMDA Online Restricted CDPP/AMDA HAPI Server http://amda.irap.omp.eu/service/hapi 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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Restricted CDPP/AMDA Web application http://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 http://amda.cdpp.eu/help/policy.html. Please acknowledge the Data Providers. JAXA spase://CNES/Instrument/CDPP-AMDA/BepiColombo/Mio/MIA ThermalPlasma 2020-10-15T00:00:00Z 2020-10-15T07:13:20Z PT4S Mercury n mia_mercury2_vmsw_n Uncalibrated density count/cm^3 TimeSeries -1.0e+31 Ion NumberDensity v_spc mia_mercury2_vmsw_v Uncalibrated velocity in SPC coordinates km/s Cartesian SC TimeSeries 3 vx Component.I 1 mia_mercury2_vmsw_v(0) vy Component.J 2 mia_mercury2_vmsw_v(1) vz Component.K 3 mia_mercury2_vmsw_v(2) -1.0e+31 Ion Vector Velocity |v| mia_mercury2_vmsw_vtot Uncalibrated velocity magnitude km/s TimeSeries Ion Magnitude Velocity t_spc mia_mercury2_vmsw_t Uncalibrated temperature in SPC coordinates eV Cartesian SC TimeSeries 6 Txx 1 mia_mercury2_vmsw_t(0) Tyy 2 mia_mercury2_vmsw_t(1) Tzz 3 mia_mercury2_vmsw_t(2) Txy 4 mia_mercury2_vmsw_t(3) Tyz 5 mia_mercury2_vmsw_t(4) Tzx 6 mia_mercury2_vmsw_t(5) -1.0e+31 Ion Scalar Temperature