Chromospheric Heating by Magnetohydrodynamic Waves and Instabilities

被引：40

作者：

Srivastava, A. K. ^{[1
]}

Ballester, J. L. ^{[2
,3
]}

Cally, P. S. ^{[4
]}

Carlsson, M. ^{[5
,6
]}

Goossens, M. ^{[7
]}

Jess, D. B. ^{[8
]}

Khomenko, E. ^{[9
,10
]}

Mathioudakis, M. ^{[8
]}

Murawski, K. ^{[11
]}

Zaqarashvili, T. V. ^{[12
,13
,14
]}

机构：

[1] Indian Inst Technol BHU, Dept Phys, Varanasi, Uttar Pradesh, India

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

[3] Univ Illes Balears, Inst Aplicac Computac Codi Comunitari IAC3, Palma De Mallorca, Spain

[4] Monash Univ, Sch Math, Clayton, Vic, Australia

[5] Univ Oslo, Inst Theoret Astrophys, Oslo, Norway

[6] Univ Oslo, Rosseland Ctr Solar Phys, Oslo, Norway

[7] Katholieke Univ Leuven, Ctr Math Plasma Astrophys CmPA, Leuven, Belgium

[8] Queens Univ Belfast, Sch Math & Phys, Astrophys Res Ctr, Belfast, Antrim, North Ireland

[9] Inst Astrofis Canarias, San Cristobal la Laguna, Spain

[10] Univ La Laguna, Dept Astrofis, San Cristobal la Laguna, Spain

[11] Univ M Curie Sklodowska, Inst Phys, Lublin, Poland

[12] Karl Franzens Univ Graz, Inst Phys, IGAM, Graz, Austria

[13] Ilia State Univ, Tbilisi, Georgia

[14] Abastumani Astrophys Observ, Abastumani, Georgia

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 2021年 / 126卷 / 06期

基金：

奥地利科学基金会; 英国科学技术设施理事会;

关键词：

chromosphere; instabilities; magnetohydrodynamics (MHD); shockssolar atmosphere; waves; MAGNETIC-FLUX TUBES; CORONAL LOOP OSCILLATIONS; PARTIALLY-IONIZED PLASMAS; FREQUENCY ACOUSTIC-WAVES; TORSIONAL ALFVEN WAVES; SOLAR P-MODES; RESONANT ABSORPTION; MHD WAVES; ENERGY FLUX; INTENSITY OSCILLATIONS;

D O I：

10.1029/2020JA029097

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The importance of the chromosphere in the mass and energy transport within the solar atmosphere is now widely recognized. This review discusses the physics of magnetohydrodynamic waves and instabilities in large-scale chromospheric structures as well as in magnetic flux tubes. We highlight a number of key observational aspects that have helped our understanding of the role of the solar chromosphere in various dynamic processes and wave phenomena, and the heating scenario of the solar chromosphere is also discussed. The review focuses on the physics of waves and invokes the basics of plasma instabilities in the context of this important layer of the solar atmosphere. Potential implications, future trends and outstanding questions are also delineated.

引用

页数：46

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