ICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter

被引:0
作者
Krasnoselskikh, Vladimir [1 ]
Tsurutani, Bruce T. [2 ]
Dudok de Wit, Thierry [1 ,3 ]
Walker, Simon [4 ]
Balikhin, Michael [4 ]
Balat-Pichelin, Marianne [5 ]
Velli, Marco [6 ]
Bale, Stuart D. [7 ]
Maksimovic, Milan [8 ]
Agapitov, Oleksiy [7 ]
Baumjohann, Wolfgang [9 ]
Berthomier, Matthieu [10 ]
Bruno, Roberto [11 ]
Cranmer, Steven R. [12 ]
de Pontieu, Bart [13 ]
Meneses, Domingos de Sousa [14 ]
Eastwood, Jonathan
Erdelyi, Robertus [16 ]
Ergun, Robert [12 ]
Fedun, Viktor [4 ]
Ganushkina, Natalia [17 ]
Greco, Antonella [18 ]
Harra, Louise [19 ]
Henri, Pierre [1 ]
Horbury, Timothy [15 ]
Hudson, Hugh [20 ]
Kasper, Justin [17 ]
Khotyaintsev, Yuri [21 ]
Kretzschmar, Matthieu [1 ]
Krucker, Sam [22 ]
Kucharek, Harald [23 ]
Langevin, Yves [24 ]
Lavraud, Benoit [25 ]
Lebreton, Jean-Pierre [1 ]
Lepri, Susan [26 ]
Liemohn, Michael [26 ]
Louarn, Philippe [25 ]
Moebius, Eberhard [27 ,28 ]
Mozer, Forrest [7 ]
Nemecek, Zdenek [29 ]
Panasenco, Olga [30 ]
Retino, Alessandro [10 ]
Safrankova, Jana [29 ]
Scudder, Jack [31 ]
Servidio, Sergio [32 ]
Sorriso-Valvo, Luca [33 ]
Soucek, Jan [34 ]
Szabo, Adam [35 ]
Vaivads, Andris [36 ]
Vekstein, Grigory [37 ]
机构
[1] Univ Orleans, CNRS, CNES, LPC2E, Orleans, France
[2] CALTECH, Jet Prop Lab, Pasadena, CA USA
[3] ISSI, Bern, Switzerland
[4] Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield, England
[5] CNRS, PROMES, Font Romeu, France
[6] UCLA, EPSS, Los Angeles, LA USA
[7] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA
[8] Paris Observ, LESIA, Meudon, France
[9] IWF Austrian Acad Sci, Space Res Inst, Graz, Austria
[10] Ecole Polytech, LPP, CNRS, Palaiseau, France
[11] INAF Ist Astrofis & Planetol Spaziali, Rome, Italy
[12] Univ Colorado, Dept Astrophys & Planetary Sci, LASP, Boulder, CO USA
[13] Astrophys Lab, Lockheed Martin Solar, Palo Alto, CA USA
[14] CNRS, CEMHTI, Orleans, France
[15] Imperial Coll, Blackett Lab, London, England
[16] Univ Sheffield, Solar Phys & Space Plasma Res Ctr, Sheffield, England
[17] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI USA
[18] Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy
[19] PMOD WRC, Davos, Switzerland
[20] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA
[21] Swedish Inst Space Phys, Uppsala, Sweden
[22] Univ Appl Sci & Arts Northwestern Switzerland, Windisch, Switzerland
[23] Univ New Hampshire, Durham, NC USA
[24] Univ Paris Sud, IAS, CNRS, Orsay, France
[25] CNES, CNRS, IRAP, Toulouse, France
[26] Univ Michigan, Climate & Space Sci & Engn, Ann Arbor, MI USA
[27] Univ New Hampshire, Space Sci Ctr, Durham, NC USA
[28] Univ New Hampshire, Dept Phys, Durham, NC USA
[29] Charles Univ Prague, Prague, Czech Republic
[30] Adv Heliophys Inc, Los Angeles, LA USA
[31] Univ Iowa, Dept Phys & Astron, Iowa City, IA USA
[32] Univ Calabria, Dipartimento Fis, Cosenza, Italy
[33] CNR, Nanotec, UOS LICRYL Cosenza, Cubo 31C, Arcavacata Di Rende, CS, Italy
[34] Acad Sci Czech Republ, Inst Atmospher Phys, Prague, Czech Republic
[35] NASA Goddard Space Flight Ctr, Heliospher Phys Lab, Code 672, Greenbelt, MD USA
[36] Swedish Inst Space Phys, Uppsala, Sweden
[37] Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester, England
[38] Austrian Acad Sci, Space Res Inst, Graz, Austria
[39] Karl Franzens Univ Graz, Inst Phys, IGAM, Graz, Austria
[40] OMP, IRAP, Toulouse, France
关键词
Solar wind; Heliophysics; Solar atmosphere; Space mission; EJECTION DRIVEN SHOCKS; ALFVEN WAVES; PARTICLE EVENTS; MASS EJECTIONS; MHD TURBULENCE; WIND SPEED; NEAR-SUN; 30; R; VELOCITY; MODEL;
D O I
10.1007/s10686-022-09878-1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The primary scientific goal of ICARUS (Investigation of Coronal AcceleRation and heating of solar wind Up to the Sun), a mother-daughter satellite mission, proposed in response to the ESA "Voyage 2050" Call, will be to determine how the magnetic field and plasma dynamics in the outer solar atmosphere give rise to the corona, the solar wind, and the entire heliosphere. Reaching this goal will be a Rosetta Stone step, with results that are broadly applicable within the fields of space plasma physics and astrophysics. Within ESA's Cosmic Vision roadmap, these science goals address Theme 2: "How does the Solar System work?" by investigating basic processes occurring "From the Sun to the edge of the Solar System". ICARUS will not only advance our understanding of the plasma environment around our Sun, but also of the numerous magnetically active stars with hot plasma coronae. ICARUS I will perform the first direct in situ measurements of electromagnetic fields, particle acceleration, wave activity, energy distribution, and flows directly in the regions in which the solar wind emerges from the coronal plasma. ICARUS I will have a perihelion altitude of 1 solar radius and will cross the region where the major energy deposition occurs. The polar orbit of ICARUS I will enable crossing the regions where both the fast and slow winds are generated. It will probe the local characteristics of the plasma and provide unique information about the physical processes involved in the creation of the solar wind. ICARUS II will observe this region using remote-sensing instruments, providing simultaneous, contextual information about regions crossed by ICARUS I and the solar atmosphere below as observed by solar telescopes. It will thus provide bridges for understanding the magnetic links between the heliosphere and the solar atmosphere. Such information is crucial to our understanding of the plasma physics and electrodynamics of the solar atmosphere. ICARUS II will also play a very important relay role, enabling the radio-link with ICARUS I. It will receive, collect, and store information transmitted from ICARUS I during its closest approach to the Sun. It will also perform preliminary data processing before transmitting it to Earth. Performing such unique in situ observations in the area where presumably hazardous solar energetic particles are energized, ICARUS will provide fundamental advances in our capabilities to monitor and forecast the space radiation environment. Therefore, the results from the ICARUS mission will be extremely crucial for future space explorations, especially for long-term crewed space missions.
引用
收藏
页码:277 / 315
页数:39
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