Partially Ionized Plasmas in Astrophysics

被引：134

作者：

Ballester, Jose Luis ^{[1
,2
]}

Alexeev, Igor ^{[3
]}

Collados, Manuel ^{[4
]}

Downes, Turlough ^{[5
]}

Pfaff, Robert F. ^{[6
]}

Gilbert, Holly ^{[7
]}

Khodachenko, Maxim ^{[8
]}

Khomenko, Elena ^{[4
]}

Shaikhislamov, Ildar F. ^{[9
]}

Soler, Roberto ^{[1
,2
]}

Vazquez-Semadeni, Enrique ^{[10
]}

Zaqarashvili, Teimuraz ^{[8
,11
]}

机构：

[1] Univ Illes Balears, Dept Fis, Palma De Mallorca 07122, Spain

[2] Univ Illes Balears, IAC3, Palma De Mallorca 07122, Spain

[3] Lomonosov Moscow State Univ, Skobeltsyn Inst Nucl Phys MSU SINP, Moscow 119992, Russia

[4] Inst Astrofis Canarias, C Via Lactea S-N, Tenerife 38205, Spain

[5] Dublin City Univ, Sch Math Sci, Ctr Astrophys & Relat, Dublin 9, Ireland

[6] NASA, Goddard Space Flight Ctr, Mail Code 674-0, Greenbelt, MD 20771 USA

[7] Goddard Space Flight Ctr, Heliophys Sci Div, Solar Phys Lab, Mail Code 671, Greenbelt, MD 20771 USA

[8] Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria

[9] SB RAS, Inst Laser Phys, Novosibirsk, Russia

[10] UNAM, IRyA, Campus Morelia,Apdp Postal 3-72, Morelia 58089, Michoacan, Mexico

[11] Ilia State Univ, Abastumani Astrophys Observ, Tbilisi, Georgia

来源：

SPACE SCIENCE REVIEWS | 2018年 / 214卷 / 02期

基金：

美国国家科学基金会; 欧洲研究理事会;

关键词：

Plasmas; Magnetohydrodynamics; Sun; Molecular clouds; Ionospheres; Exoplanets; KELVIN-HELMHOLTZ INSTABILITY; MOLECULAR CLOUD EVOLUTION; NONADIABATIC MAGNETOHYDRODYNAMIC WAVES; CHROMOSPHERIC MAGNETIC RECONNECTION; AURORAL ELECTRON-PRECIPITATION; FARLEY-BUNEMAN INSTABILITY; ANGULAR-MOMENTUM EVOLUTION; MHD TURBULENCE SIMULATIONS; THERMALLY BISTABLE FLOW; ENERGETIC NEUTRAL ATOMS;

D O I：

10.1007/s11214-018-0485-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Partially ionized plasmas are found across the Universe in many different astrophysical environments. They constitute an essential ingredient of the solar atmosphere, molecular clouds, planetary ionospheres and protoplanetary disks, among other environments, and display a richness of physical effects which are not present in fully ionized plasmas. This review provides an overview of the physics of partially ionized plasmas, including recent advances in different astrophysical areas in which partial ionization plays a fundamental role. We outline outstanding observational and theoretical questions and discuss possible directions for future progress.

引用

页数：149

共 50 条

[21] PLASMON DISPERSION IN DENSE, PARTIALLY IONIZED PLASMAS
BARRAT, JL
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PHYSICA A, 1988, 149 (03): : 613 - 621
[22] Equation of state of partially-ionized plasmas
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STRONGLY COUPLED COULOMB SYSTEMS, 1998, : 15 - 23
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[24] Transport algorithms for partially ionized and unmagnetized plasmas
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[27] Coalescence instability in chromospheric partially ionized plasmas
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[28] Alfvenic localized structures in partially ionized plasmas
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[29] SPECIAL ISSUE ON APPLICATIONS OF PARTIALLY IONIZED PLASMAS
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IEEE TRANSACTIONS ON PLASMA SCIENCE, 1991, 19 (06) : 989 - 990
[30] INSTABILITY OF PARTIALLY-IONIZED SUPERPOSED PLASMAS
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ASTROPHYSICS AND SPACE SCIENCE, 1991, 181 (01) : 103 - 110

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