Partially Ionized Plasmas in Astrophysics

被引：142

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：

欧洲研究理事会; 美国国家科学基金会;

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 516 条

[1] JIM: A time-dependent, three-dimensional model of Jupiter's thermosphere and ionosphere [J].

Achilleos, N ;

Miller, S ;

Tennyson, J ;

Aylward, AD ;

Mueller-Wodarg, I ;

Rees, D .

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1998, 103 (E9) :20089-20112

[2] MAGNETICALLY CONTROLLED OUTFLOWS FROM HOT JUPITERS [J].

Adams, Fred C. .

ASTROPHYSICAL JOURNAL, 2011, 730 (01)

[3]

Akasofu S.-I., 1972, Solar-terrestrial physics

[4]

Alexeev I., 2014, 40 COSPAR SCI ASSEBL, V40

[5]

Alexeev I. I., 2015, ASTROPHYSICS SPACE S, V411, P189

[6] A global magnetic model of Saturn's magnetosphere and a comparison with Cassini SOI data [J].

Alexeev, II ;

Kalegaev, VV ;

Belenkaya, ES ;

Bobrovnikov, SY ;

Bunce, EJ ;

Cowley, SWH ;

Nichols, JD .

GEOPHYSICAL RESEARCH LETTERS, 2006, 33 (08)

[7] Modeling of the Jovian magnetosphere [J].

Alexeev, II ;

Belenkaya, ES .

ANNALES GEOPHYSICAE, 2005, 23 (03) :809-826

[8] Modelling of the electromagnetic field in the interplanetary space and in the earth's magnetosphere [J].

Alexeev, II ;

Belenkaya, ES ;

Bobrovnikov, SY ;

Kalegaev, VV .

SPACE SCIENCE REVIEWS, 2003, 107 (1-2) :7-26

[9]

Alexiades V, 1996, COMMUN NUMER METH EN, V12, P31, DOI 10.1002/(SICI)1099-0887(199601)12:1<31::AID-CNM950>3.0.CO

[10]

2-5

← 1 2 3 4 5 6 7 8 9 10 →