The ESA M7 candidate mission Plasma Observatory.
- 1INAF-IAPS, Roma, Italy (maria.marcucci@inaf.it)
- *A full list of authors appears at the end of the abstract
Particle energization and transport of energy are key open problems of space plasma physics. Their comprehension has implications on research fields that span from space weather to the understanding of the farthest astrophysical plasmas. The Magnetospheric System is the complex and highly dynamic plasma environment where the strongest energization and energy transport occurs in near-Earth space. Previous multi-point observations from missions such as ESA/Cluster and NASA/MMS have greatly improved our understanding of plasma processes and evidenced the fundamental role of cross-scales coupling. Simultaneous measurements at both large, fluid and small, kinetic scales are required to resolve scale coupling and ultimately fully understand plasma energization and energy transport processes. Such measurements are currently not available. Here we present the Plasma Observatory (PO) multi-scale mission concept tailored to study plasma energization and energy transport in the Earth's Magnetospheric System through simultaneous measurements at both fluid and ion scales. These are the scales at which the largest amount of electromagnetic energy is converted into energized particles and energy is transported. PO baseline mission includes one mothercraft (MSC) and six identical smallsat daughtercraft (DSC) in two nested tetrahedra formation with MSC at the common vertex for both tetrahedra. PO orbit is an HEO 8x18 RE orbit, covering all the key regions of the Magnetospheric System including the foreshock, the bow shock, the magnetosheath, the magnetopause, the magnetotail current sheet, and the transition region. Along the orbit, the separations between the spacecraft range from fluid (5000 km) to ion (30 km) scales. The MSC payload provides a complete characterization of electromagnetic fields and particles in a single point with time resolution sufficient to resolve kinetic physics at sub-ion scales (for both protons and heavy ions). The DSCs have identical payload, simpler than the MSC payload, yet giving a full characterization of the plasma at the ion and fluid scales. PO is the next logical step after Cluster and MMS and will allow us to resolve for the first time scale coupling in the Earth's Magnetospheric System, leading to transformative advances in the field of space plasma physics. Plasma Observatory is one of the three ESA M7 candidates, which have been selected in November 2023 for a competitive Phase A with a mission selection planned in 2026 and launch in 2037.
T. Amano 1), V. Angelopoulos 2), S. D. Bale 3), M. Berthomier 4), R. D'Amicis 5), J. De Keyser 6), U. Derz 7), A. Dimmock 8), M. Dunlop 9), C. Forsyth 10), M. Fränz 11), H. Fu 12), A. Galli 13), V. Genot 14), K. Kauristie 15), Y. Khotyaintsev 8), L. Kistler 16), M. Kretzschmar 17), H. Kucharek 16), K. Issautier 18), B. Lavraud, 14,19), O. Le Contel 1), I. Mann 20), L. Matteini 21), K. McWilliams 22), M. Maksimovic 18), R. Nakamura 23), A. C. Norgren 24), M. Palmroth 25), E. Panov 23), O. Pezzi 26), F. Plaschke 27), H. Rothkaehl 28), E. Roussos 11), Y. Saito 29), J. Soucek 30), A. Stankov 8), M. Steller 23), M. Taylor 8), M. Yamauchi 31), R. Vainio 32), A. Vaivads 33), F. Valentini 34), R. F. Wimmer-Schweingruber 35) and the Plasma Observatory Science Team. Affiliations: 1) Univ. of Tokyo, JP, 2) UCLA, US, 3) Univ. California, Berkeley, US, 4) LPP, FR, 5) INAF-IAPS, IT, 6) BIRA, BE, 7) ESTEC, 8) IRF-U, SE, 9) RAL, UK, 10) MSSL-UCL, UK, 11) MPS, DE, 12) Beihang Univ., CN, 13) Univ. of Bern, CH, 14) IRAP, FR, 15) FMI, FI, 16) UNH, US, 17) LPC2E, FR, 18) LESIA, FR, 19) LAB, FR, 20) Univ. of Alberta, CA, 21) ICL, UK, 22) Univ. of Saskatoon, CA, 23) IWF/ÖAW, AT, 24) Univ. of Bergen, NO, 25) Univ. of Helsinki, FI, 26) ISTP, IT, 27) TU Braunschweig, DE, 28) CBK, PL, 29) ISAS-JAXA, JP, 30) IAP-CAS, CZ, 31) IRF-K, SE, 32) Univ. of Turku, FI; 33) KTH, SE, 34) Univ. of Calabria, IT, 35) Univ. of Kiel, DE
How to cite: Marcucci, M. F. and Retinò, A. and the Plasma Observatory team: The ESA M7 candidate mission Plasma Observatory., EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-11903, https://doi.org/10.5194/egusphere-egu24-11903, 2024.
