Magnetohydrodynamic Waves in Open Coronal Structures

被引：64

作者：

Banerjee, D. ^{[1
,2
,3
]}

Krishna Prasad, S. ^{[4
]}

Pant, V. ^{[1
]}

McLaughlin, J. A. ^{[5
]}

Antolin, P. ^{[6
]}

Magyar, N. ^{[7
]}

Ofman, L. ^{[8
,9
]}

Tian, H. ^{[10
,11
]}

Van Doorsselaere, T. ^{[4
]}

De Moortel, I. ^{[12
,13
]}

Wang, T. J. ^{[8
,9
]}

机构：

[1] Aryabhatta Res Inst Observat Sci, Naini Tal 263002, India

[2] Indian Inst Astrophys, Bangalore 560034, Karnataka, India

[3] Indian Inst Sci Educ & Res Kolkata, Ctr Excellence Space Sci India, Mohanpur 741246, W Bengal, India

[4] Katholieke Univ Leuven, Ctr Math Plasma Astrophys, Dept Math, Celestijnenlaan 200B, B-3001 Leuven, Belgium

[5] Northumbria Univ, Newcastle Upon Tyne NE1 8ST, Tyne & Wear, England

[6] Northumbria Univ, Dept Math Phys & Elect Engn, Newcastle Upon Tyne NE1 8ST, Tyne & Wear, England

[7] Univ Warwick, Dept Phys, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England

[8] Catholic Univ Amer, Code 671, Greenbelt, MD 20771 USA

[9] NASA Goddard Space Flight Ctr, Code 671, Greenbelt, MD 20771 USA

[10] Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China

[11] Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing 100012, Peoples R China

[12] Univ St Andrews, Sch Math & Stat, St Andrews KY16 9SS, Fife, Scotland

[13] Univ Oslo, Rosseland Ctr Solar Phys, POB 1029, N-0315 Oslo, Norway

来源：

SPACE SCIENCE REVIEWS | 2021年 / 217卷 / 07期

基金：

英国科学技术设施理事会; 欧洲研究理事会; 欧盟地平线“2020”;

关键词：

Solar corona; Magnetohydrodynamics; Waves and oscillations; SLOW MAGNETOACOUSTIC WAVES; EMISSION-LINE SPECTRUM; PROPAGATING KINK WAVES; ALFVEN WAVES; SOLAR CORONA; MHD WAVES; ACTIVE-REGION; TRANSITION-REGION; LOOP OSCILLATIONS; INTENSITY DISTURBANCES;

D O I：

10.1007/s11214-021-00849-0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic waves in the solar corona. The propagating waves (in contrast to the standing waves) are usually originated in the lower solar atmosphere which makes them particularly relevant to coronal heating. Furthermore, open coronal structures are believed to be the source regions of solar wind, therefore, the detection of MHD waves in these structures is also pertinent to the acceleration of solar wind. Besides, the advanced capabilities of the current generation telescopes have allowed us to extract important coronal properties through MHD seismology. The recent progress made in the detection, origin, and damping of both propagating slow magnetoacoustic waves and kink (Alfvenic) waves is presented in this review article especially in the context of open coronal structures. Where appropriate, we give an overview on associated theoretical modelling studies. A few of the important seismological applications of these waves are discussed. The possible role of Alfvenic waves in the acceleration of solar wind is also touched upon.

引用

页数：37

共 253 条

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