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ICARUS: in-Situ Studies of the Solar Corona Beyond Parker Solar Probe and Solar OrbiterThe 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.
Document ID
20230015487
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Vladimir Krasnoselskikh ORCID
(University of Orléans Orléans, France)
Bruce T. Tsurutani
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Thierry Dudok de Wit ORCID
(University of Orléans Orléans, France)
Simon Walker
(University of Sheffield Sheffield, United Kingdom)
Michael Balikhin
(University of Sheffield Sheffield, United Kingdom)
Marianne Balat-Pichelin
(Canadian Nautical Research Society Ottawa, Ontario, Canada)
Marco Velli ORCID
(University of California, Los Angeles Los Angeles, California, United States)
Stuart D. Bale ORCID
(University of California, Berkeley Berkeley, California, United States)
Milan Maksimovic ORCID
(Laboratory of Space Studies and Instrumentation in Astrophysics Meudon, France)
Oleksiy Agapitov
(University of California, Berkeley Berkeley, California, United States)
Wolfgang Baumjohann
(Space Research Institute Graz, Austria)
Matthieu Berthomier
(Canadian Nautical Research Society Ottawa, Ontario, Canada)
Roberto Bruno ORCID
(Istituto di Astrofisica e Planetologia Spaziali Rome, Italy)
Steven R. Cranmer ORCID
(University of Colorado Boulder Boulder, Colorado, United States)
Bart de Pontieu
(Lockheed Martin (United States) Bethesda, Maryland, United States)
Domingos de Sousa Meneses
(Canadian Nautical Research Society Ottawa, Ontario, Canada)
Jonathan Eastwood
(Imperial College London London, Westminster, United Kingdom)
Robertus Erdelyi
(University of Sheffield Sheffield, United Kingdom)
Robert Ergun
(University of Colorado Boulder Boulder, Colorado, United States)
Viktor Fedun
(University of Sheffield Sheffield, United Kingdom)
Natalia Ganushkina
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
Antonella Greco
(University of Calabria Cosenza, Italy)
Louise Harra ORCID
(Physikalisch-Meteorologisches Observatorium Davos– World Radiation Center Davos, Switzerland)
Pierre Henri
(University of Orléans Orléans, France)
Timothy Horbury
(Imperial College London London, Westminster, United Kingdom)
Hugh Hudson ORCID
(University of California, Berkeley Berkeley, California, United States)
Justin Kasper ORCID
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
Yuri Khotyaintsev ORCID
(Swedish Institute of Space Physics Kiruna, Sweden)
Matthieu Kretzschmar ORCID
(University of Orléans Orléans, France)
Säm Krucker
(University of Applied Sciences and Arts Northwestern Switzerland Windisch, Switzerland)
Harald Kucharek
(University of New Hampshire Durham, New Hampshire, United States)
Yves Langevin
(University of Paris-Saclay Gif-sur-Yvette, France)
Benoît Lavraud
(Canadian Nautical Research Society Ottawa, Ontario, Canada)
Jean-Pierre Lebreton
(University of Orléans Orléans, France)
Adam Szabo
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
October 25, 2023
Publication Date
February 4, 2023
Publication Information
Publication: Experimental Astronomy
Publisher: Springer
Volume: 54
Issue Publication Date: December 1, 2022
ISSN: 0922-6435
e-ISSN: 1572-9508
Subject Category
Solar Physics
Space Sciences (General)
Funding Number(s)
WBS: 388443.04.01
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
Keywords
Solar wind
Heliophysics
Solar atmosphere
Space mission
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