BibTex format
@article{Krasnoselskikh:2023:10.1007/s10686-022-09878-1,
author = {Krasnoselskikh, V and Tsurutani, BT and Dudok, de Wit T and Walker, S and Balikhin, M and Balat-Pichelin, M and Velli, M and Bale, SD and Maksimovic, M and Agapitov, O and Baumjohann, W and Berthomier, M and Bruno, R and Cranmer, SR and de, Pontieu B and Meneses, DDS and Eastwood, J and Erdelyi, R and Ergun, R and Fedun, V and Ganushkina, N and Greco, A and Harra, L and Henri, P and Horbury, T and Hudson, H and Kasper, J and Khotyaintsev, Y and Kretzschmar, M and Krucker, S and Kucharek, H and Langevin, Y and Lavraud, B and Lebreton, J-P and Lepri, S and Liemohn, M and Louarn, P and Moebius, E and Mozer, F and Nemecek, Z and Panasenco, O and Retino, A and Safrankova, J and Scudder, J and Servidio, S and Sorriso-Valvo, L and Souek, J and Szabo, A and Vaivads, A and Vekstein, G and Vörös, Z and Zaqarashvili, T and Zimbardo, G and Fedorov, A},
doi = {10.1007/s10686-022-09878-1},
journal = {Experimental Astronomy},
pages = {277--315},
title = {ICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter},
url = {http://dx.doi.org/10.1007/s10686-022-09878-1},
volume = {54},
year = {2023}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - 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 atmosph
AU - Krasnoselskikh,V
AU - Tsurutani,BT
AU - Dudok,de Wit T
AU - Walker,S
AU - Balikhin,M
AU - Balat-Pichelin,M
AU - Velli,M
AU - Bale,SD
AU - Maksimovic,M
AU - Agapitov,O
AU - Baumjohann,W
AU - Berthomier,M
AU - Bruno,R
AU - Cranmer,SR
AU - de,Pontieu B
AU - Meneses,DDS
AU - Eastwood,J
AU - Erdelyi,R
AU - Ergun,R
AU - Fedun,V
AU - Ganushkina,N
AU - Greco,A
AU - Harra,L
AU - Henri,P
AU - Horbury,T
AU - Hudson,H
AU - Kasper,J
AU - Khotyaintsev,Y
AU - Kretzschmar,M
AU - Krucker,S
AU - Kucharek,H
AU - Langevin,Y
AU - Lavraud,B
AU - Lebreton,J-P
AU - Lepri,S
AU - Liemohn,M
AU - Louarn,P
AU - Moebius,E
AU - Mozer,F
AU - Nemecek,Z
AU - Panasenco,O
AU - Retino,A
AU - Safrankova,J
AU - Scudder,J
AU - Servidio,S
AU - Sorriso-Valvo,L
AU - Souek,J
AU - Szabo,A
AU - Vaivads,A
AU - Vekstein,G
AU - Vörös,Z
AU - Zaqarashvili,T
AU - Zimbardo,G
AU - Fedorov,A
DO - 10.1007/s10686-022-09878-1
EP - 315
PY - 2023///
SN - 0922-6435
SP - 277
TI - ICARUS: in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter
T2 - Experimental Astronomy
UR - http://dx.doi.org/10.1007/s10686-022-09878-1
UR - https://link.springer.com/article/10.1007/s10686-022-09878-1
UR - http://hdl.handle.net/10044/1/102133
VL - 54
ER -