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Plasma-neutral gas interactions in various space environments : Assessment beyond simplified approximations as a Voyage 2050 theme

Yamauchi, M. (författare)
Swedish Institute of Space Physics (IRF), Kiruna, Sweden
De Keyser, J. (författare)
Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Brussels, Belgium
Parks, G. (författare)
Space Science Laboratory (SSL), University of California Berkeley, CA, Berkeley, United States
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Oyama, S. -I (författare)
Institute for Space-Earth Environmental Research (ISEE), Nagoya University, Nagoya, Japan; Space Physics and Astronomy Research Unit, University of Oulu, Oulu, Finland; National Institute of Polar Research (NIPR), Tachikawa, Japan
Wurz, P. (författare)
University of Bern, Bern, Switzerland
Abe, T. (författare)
Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan
Beth, Arnaud (författare)
Umeå universitet,Institutionen för fysik,Department of Physics, Imperial College London, London, United Kingdom
Daglis, I. A. (författare)
National and Kapodistrian University of Athens, Athens, Greece; Hellenic Space Center, Athens, Greece
Dandouras, I. (författare)
Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France
Dunlop, M. (författare)
Science and Technology Facilities Council (STFC), Swindon, United Kingdom; School of Space and Environment, BUAA, Beijing, China
Henri, P. (författare)
CNRS, University of Orléans and CNES, Laboratoire de Physique et Chimie de l’Environment et de l’Espace, Orléans, France; CNRS, UCA, OCA, Lagrange, Nice, France
Ivchenko, Nickolay, 1976- (författare)
KTH,Rymd- och plasmafysik,Royal Institute of Technology KTH, Stockholm, Sweden
Kallio, E. (författare)
Aalto University, Espoo, Finland
Kucharek, H. (författare)
University of New Hampshire, NH, Durham, United States
Liu, Y. C. -M (författare)
National Space Science Center (NSSC), Beijing, China
Mann, I. (författare)
Arctic University of Norway in Tromsø, Tromsø, Norway
Marghitu, O. (författare)
Institute for Space Sciences (ISS), Bucharest, Romania
Nicolaou, G. (författare)
Mullard Space Science Laboratory (MSSL), University College London, London, United Kingdom
Rong, Z. (författare)
Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
Sakanoi, T. (författare)
Tohoku University, Sendai, Japan
Saur, J. (författare)
University of Köln, Köln, Germany
Shimoyama, M. (författare)
Swedish Institute of Space Physics (IRF), Kiruna, Sweden
Taguchi, S. (författare)
Kyoto University, Kyoto, Japan
Tian, F. (författare)
Macau University of Science and Technology, Macao; Blue Marble Space Institute of Science, CO, Boulder, United States
Tsuda, T. (författare)
University of Electro-Communications, Tokyo, Japan
Tsurutani, B. (författare)
Jet Propulsion Laboratory (JPL), CA, Pasadena, United States
Turner, D. (författare)
Johns Hopkins Applied Physics Laboratory, MD, Laurel, United States
Ulich, T. (författare)
Sodankylä Geophysical Observatory, Sodankylä, Finland
Yau, A. (författare)
University of Calgary, Calgary, Canada
Yoshikawa, I. (författare)
University of Tokyo, Tokyo, Japan
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 (creator_code:org_t)
2022-03-26
2022
Engelska.
Ingår i: Experimental astronomy. - : Springer Nature. - 0922-6435 .- 1572-9508.
Relaterad länk:
https://doi.org/10.1...
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https://umu.diva-por... (primary) (Raw object)
https://urn.kb.se/re...
https://doi.org/10.1...
https://urn.kb.se/re...
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  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • In the White Paper, submitted in response to the European Space Agency (ESA) Voyage 2050 Call, we present the importance of advancing our knowledge of plasma-neutral gas interactions, and of deepening our understanding of the partially ionized environments that are ubiquitous in the upper atmospheres of planets and moons, and elsewhere in space. In future space missions, the above task requires addressing the following fundamental questions: (A) How and by how much do plasma-neutral gas interactions influence the re-distribution of externally provided energy to the composing species? (B) How and by how much do plasma-neutral gas interactions contribute toward the growth of heavy complex molecules and biomolecules? Answering these questions is an absolute prerequisite for addressing the long-standing questions of atmospheric escape, the origin of biomolecules, and their role in the evolution of planets, moons, or comets, under the influence of energy sources in the form of electromagnetic and corpuscular radiation, because low-energy ion-neutral cross-sections in space cannot be reproduced quantitatively in laboratories for conditions of satisfying, particularly, (1) low-temperatures, (2) tenuous or strong gradients or layered media, and (3) in low-gravity plasma. Measurements with a minimum core instrument package (< 15 kg) can be used to perform such investigations in many different conditions and should be included in all deep-space missions. These investigations, if specific ranges of background parameters are considered, can also be pursued for Earth, Mars, and Venus. 

Ämnesord

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

Collision cross-section
Future missions
Low-energy
Neutral gas
Plasma
Voyage 2050

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