IGGCAS OpenIR  > 地球与行星物理院重点实验室
Plasma-neutral gas interactions in various space environments: Assessment beyond simplified approximations as a Voyage 2050 theme
Yamauchi, Masatoshi1; De Keyser, Johan2; Parks, George3; Oyama, Shin-ichiro4,5,6; Wurz, Peter7; Abe, Takumi8; Beth, Arnaud9,10; Daglis, Ioannis A.11,12; Dandouras, Iannis13; Dunlop, Malcolm14,15; Henri, Pierre16,17,18; Ivchenko, Nickolay19; Kallio, Esa20; Kucharek, Harald21; Liu, Yong C-M22; Mann, Ingrid23; Marghitu, Octav24; Nicolaou, Georgios25; Rong, Zhaojin26; Sakanoi, Takeshi27; Saur, Joachim28; Shimoyama, Manabu1; Taguchi, Satoshi29; Tian, Feng30,31; Tsuda, Takuo32; Tsurutani, Bruce33; Turner, Drew34; Ulich, Thomas35; Yau, Andrew36; Yoshikawa, Ichiro37
2022-03-26
Source PublicationEXPERIMENTAL ASTRONOMY
ISSN0922-6435
Pages39
AbstractIn 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 ionneutral 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.
KeywordPlasma Neutral gas Collision cross-section Low-energy Voyage 2050 Future missions
DOI10.1007/s10686-022-09846-9
Funding OrganizationUniversity of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern
WOS KeywordSOLAR-SYSTEM ; THERMOSPHERE RESPONSE ; IONOSPHERIC CURRENTS ; ATMOSPHERE ; WINDS ; DISTURBANCES ; SIMULATION ; MOLECULES ; VICINITY ; MERCURY
Language英语
Funding ProjectUniversity of Bern
Funding OrganizationUniversity of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern ; University of Bern
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000773961300001
PublisherSPRINGER
Citation statistics
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/105064
Collection地球与行星物理院重点实验室
Corresponding AuthorYamauchi, Masatoshi; Wurz, Peter
Affiliation1.Swedish Inst Space Phys IRF, Kiruna, Sweden
2.Royal Belgian Inst Space Aeron BIRA IASB, Brussels, Belgium
3.Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
4.Nagoya Univ, Inst Space Earth Environm Res ISEE, Nagoya, Aichi, Japan
5.Univ Oulu, Space Phys & Astron Res Unit, Oulu, Finland
6.Natl Inst Polar Res NIPR, Tachikawa, Tokyo, Japan
7.Univ Bern, Bern, Switzerland
8.Japan Aerosp Explorat Agcy JAXA, Inst Space & Astronaut Sci ISAS, Sagamihara, Kanagawa, Japan
9.Imperial Coll London, Dept Phys, London, England
10.Umea Univ, Dept Phys, Umea, Sweden
11.Natl & Kapodistrian Univ Athens, Athens, Greece
12.Hellen Space Ctr, Athens, Greece
13.Inst Rech Astrophys & Planetol IRAP, Toulouse, France
14.Sci & Technol Facil Council STFC, Swindon, Wilts, England
15.BUAA, Sch Space & Environm, Beijing, Peoples R China
16.Univ Orleans, CNRS, Orleans, France
17.CNES, Lab Phys & Chim Environm & Espace, Orleans, France
18.UCA, OCA, CNRS, Nice, France
19.Royal Inst Technol KTH, Stockholm, Sweden
20.Aalto Univ, Espoo, Finland
21.Univ New Hampshire, Durham, NH 03824 USA
22.Natl Space Sci Ctr NSSC, Beijing, Peoples R China
23.Arctic Univ Norway Tromso, Tromso, Norway
24.Inst Space Sci ISS, Bucharest, Romania
25.UCL, Mullard Space Sci Lab MSSL, London, England
26.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
27.Tohoku Univ, Sendai, Miyagi, Japan
28.Univ Cologne, Cologne, Germany
29.Kyoto Univ, Kyoto, Japan
30.Macau Univ Sci & Technol, Macau, Peoples R China
31.Blue Marble Space Inst Sci, Boulder, CO USA
32.Univ Electrocommun, Tokyo, Japan
33.Jet Prop Lab JPL, Pasadena, CA USA
34.Johns Hopkins Appl Phys Lab, Laurel, MD USA
35.Sodankyla Geophys Observ, Sodankyla, Finland
36.Univ Calgary, Calgary, AB, Canada
37.Univ Tokyo, Tokyo, Japan
Recommended Citation
GB/T 7714
Yamauchi, Masatoshi,De Keyser, Johan,Parks, George,et al. Plasma-neutral gas interactions in various space environments: Assessment beyond simplified approximations as a Voyage 2050 theme[J]. EXPERIMENTAL ASTRONOMY,2022:39.
APA Yamauchi, Masatoshi.,De Keyser, Johan.,Parks, George.,Oyama, Shin-ichiro.,Wurz, Peter.,...&Yoshikawa, Ichiro.(2022).Plasma-neutral gas interactions in various space environments: Assessment beyond simplified approximations as a Voyage 2050 theme.EXPERIMENTAL ASTRONOMY,39.
MLA Yamauchi, Masatoshi,et al."Plasma-neutral gas interactions in various space environments: Assessment beyond simplified approximations as a Voyage 2050 theme".EXPERIMENTAL ASTRONOMY (2022):39.
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