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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00009483naa a2201021 4500
001oai:DiVA.org:uu-512819
003SwePub
008230929s2022 | |||||||||||000 ||eng|
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-5128192 URI
0247 a https://doi.org/10.1007/s10686-022-09878-12 DOI
040 a (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
1001 a Krasnoselskikh, Vladimiru Univ Orleans, CNRS, CNES, LPC2E, Orleans, France.4 aut
2451 0a ICARUS :b in-situ studies of the solar corona beyond Parker Solar Probe and Solar Orbiter
264 c 2023-02-04
264 1b Springer Nature,c 2022
338 a electronic2 rdacarrier
520 a 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.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng
653 a Solar wind
653 a Heliophysics
653 a Solar atmosphere
653 a Space mission
7001 a Tsurutani, Bruce T.u CALTECH, Jet Prop Lab, Pasadena, CA USA.4 aut
7001 a Dudok de Wit, Thierryu Univ Orleans, CNRS, CNES, LPC2E, Orleans, France.;ISSI, Bern, Switzerland.4 aut
7001 a Walker, Simonu Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield, England.4 aut
7001 a Balikhin, Michaelu Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield, England.4 aut
7001 a Balat-Pichelin, Marianneu CNRS, PROMES, Font Romeu, France.4 aut
7001 a Velli, Marcou UCLA, EPSS, Los Angeles, LA USA.4 aut
7001 a Bale, Stuart D.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA.4 aut
7001 a Maksimovic, Milanu Paris Observ, LESIA, Meudon, France.4 aut
7001 a Agapitov, Oleksiyu Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA.4 aut
7001 a Baumjohann, Wolfgangu IWF Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
7001 a Berthomier, Matthieuu Ecole Polytech, LPP, CNRS, Palaiseau, France.4 aut
7001 a Bruno, Robertou INAF Ist Astrofis & Planetol Spaziali, Rome, Italy.4 aut
7001 a Cranmer, Steven R.u Univ Colorado, Dept Astrophys & Planetary Sci, LASP, Boulder, CO USA.4 aut
7001 a de Pontieu, Bartu Astrophys Lab, Lockheed Martin Solar, Palo Alto, CA USA.4 aut
7001 a Meneses, Domingos de Sousau CNRS, CEMHTI, Orleans, France.4 aut
7001 a Eastwood, Jonathan4 aut
7001 a Erdelyi, Robertusu Univ Sheffield, Solar Phys & Space Plasma Res Ctr, Sheffield, England.4 aut
7001 a Ergun, Robertu Univ Colorado, Dept Astrophys & Planetary Sci, LASP, Boulder, CO USA.4 aut
7001 a Fedun, Viktoru Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield, England.4 aut
7001 a Ganushkina, Nataliau Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI USA.4 aut
7001 a Greco, Antonellau Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.4 aut
7001 a Harra, Louiseu PMOD WRC, Davos, Switzerland.4 aut
7001 a Henri, Pierreu Univ Orleans, CNRS, CNES, LPC2E, Orleans, France.4 aut
7001 a Horbury, Timothyu Imperial Coll, Blackett Lab, London, England.4 aut
7001 a Hudson, Hughu Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA.4 aut
7001 a Kasper, Justinu Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI USA.4 aut
7001 a Khotyaintsev, Yuriu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ykh28990
7001 a Kretzschmar, Matthieuu Univ Orleans, CNRS, CNES, LPC2E, Orleans, France.4 aut
7001 a Krucker, Sämu Univ Appl Sci & Arts Northwestern Switzerland, Windisch, Switzerland.4 aut
7001 a Kucharek, Haraldu Univ New Hampshire, Durham, NC USA.4 aut
7001 a Langevin, Yvesu Univ Paris Sud, IAS, CNRS, Orsay, France.4 aut
7001 a Lavraud, Benoitu CNES, CNRS, IRAP, Toulouse, France.4 aut
7001 a Lebreton, Jean-Pierreu Univ Orleans, CNRS, CNES, LPC2E, Orleans, France.4 aut
7001 a Lepri, Susanu Univ Michigan, Climate & Space Sci & Engn, Ann Arbor, MI USA.4 aut
7001 a Liemohn, Michaelu Univ Michigan, Climate & Space Sci & Engn, Ann Arbor, MI USA.4 aut
7001 a Louarn, Philippeu CNES, CNRS, IRAP, Toulouse, France.4 aut
7001 a Moebius, Eberhardu Univ New Hampshire, Space Sci Ctr, Durham, NC USA.;Univ New Hampshire, Dept Phys, Durham, NC USA.4 aut
7001 a Mozer, Forrestu Univ Calif Berkeley, Space Sci Lab, Berkeley, CA USA.4 aut
7001 a Nemecek, Zdeneku Charles Univ Prague, Prague, Czech Republic.4 aut
7001 a Panasenco, Olgau Adv Heliophys Inc, Los Angeles, LA USA.4 aut
7001 a Retino, Alessandrou Ecole Polytech, LPP, CNRS, Palaiseau, France.4 aut
7001 a Safrankova, Janau Charles Univ Prague, Prague, Czech Republic.4 aut
7001 a Scudder, Jacku Univ Iowa, Dept Phys & Astron, Iowa City, IA USA.4 aut
7001 a Servidio, Sergiou Univ Calabria, Dipartimento Fis, Cosenza, Italy.4 aut
7001 a Sorriso-Valvo, Lucau CNR, Nanotec, UOS LICRYL Cosenza, Cubo 31C, Arcavacata Di Rende, CS, Italy.4 aut
7001 a Soucek, Janu Acad Sci Czech Republ, Inst Atmospher Phys, Prague, Czech Republic.4 aut
7001 a Szabo, Adamu NASA Goddard Space Flight Ctr, Heliospher Phys Lab, Code 672, Greenbelt, MD USA.4 aut
7001 a Vaivads, Andrisu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)anvai517
7001 a Vekstein, Grigoryu Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester, England.4 aut
7001 a Vörös, Zoltanu Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
7001 a Zaqarashvili, Teimurazu Karl Franzens Univ Graz, Inst Phys, IGAM, Graz, Austria.4 aut
7001 a Zimbardo, Gaetanou Univ Calabria, Dipartimento Fis, Arcavacata Di Rende, Italy.4 aut
7001 a Fedorov, Andreiu OMP, IRAP, Toulouse, France.4 aut
7102 a Univ Orleans, CNRS, CNES, LPC2E, Orleans, France.b CALTECH, Jet Prop Lab, Pasadena, CA USA.4 org
7730 t Experimental astronomyd : Springer Natureg 54:2-3, s. 277-315q 54:2-3<277-315x 0922-6435x 1572-9508
8564 u https://doi.org/10.1007/s10686-022-09878-1y Fulltext
8564 u https://uu.diva-portal.org/smash/get/diva2:1801085/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-512819
8564 8u https://doi.org/10.1007/s10686-022-09878-1

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