Magnetohydrodynamic Waves in Open Coronal Structures

Banerjee, D.; Krishna Prasad, S.; Pant, V.; McLaughlin, J. A.; Antolin, P.; Magyar, N.; Ofman, L.; Tian, H.; Van Doorsselaere, T.; De Moortel, I.; Wang, T. J.

doi:10.1007/s11214-021-00849-0

Published: 21 September 2021

Magnetohydrodynamic Waves in Open Coronal Structures

D. Banerjee^1,2,3,
S. Krishna Prasad⁴,
V. Pant¹,
J. A. McLaughlin ORCID: orcid.org/0000-0002-7863-624X⁵,
P. Antolin⁶,
N. Magyar⁷,
L. Ofman⁸,
H. Tian^9,10,
T. Van Doorsselaere⁴,
I. De Moortel^11,12 &
…
T. J. Wang⁸

Space Science Reviews volume 217, Article number: 76 (2021) Cite this article

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Abstract

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 (Alfvénic) 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 Alfvénic waves in the acceleration of solar wind is also touched upon.

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Acknowledgements

The authors thank the anonymous referees for their helpful suggestions. We wish to acknowledge ISSI-BJ for hosting the workshop at Beijing and for their generous Support for all the participants. SKP is grateful to FWO Vlaanderen for a senior postdoctoral fellowship (No. 12ZF420N). VP was supported by the Spanish Ministerio de Ciencia, Innovación y Universidades through project PGC2018-102108-B-I00 and FEDER funds. VP and TVD are supported by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 724326). J.A.M. acknowledges UK Science and Technology Facilities Council (STFC) support from grant ST/T000384/1. L.O. acknowledges support by NASA grants NNX16AF78G, 80NSSC18K1131 and NASA Cooperative Agreement NNG11PL10A to CUA. P.A. acknowledges funding from his STFC Ernest Rutherford Fellowship (No. ST/R004285/2). IDM acknowledges support from the UK Science and Technology Facilities Council (consolidated grants ST/N000609/1 and ST/S000402/1), the European Union Horizon 2020 research and innovation programme (grant agreement No. 647214) and the Research Council of Norway through its Centres of Excellence scheme, project number 262622. H.T. is supported by NSFC grants 11825301 and 11790304(11790300). T.J.W. acknowledges support by NASA grants 80NSSC18K1131, 80NSSC18K0668, and NASA Cooperative Agreement NNG11PL10A to CUA.

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Authors and Affiliations

Aryabhatta Research Institute of Observational Sciences, Nainital, 263002, India
D. Banerjee & V. Pant
Indian Institute of Astrophysics, Koramangala, Bangalore, 560034, India
D. Banerjee
Center of Excellence in Space Sciences India, Indian Institute of Science Education and Research Kolkata, Mohanpur, 741246, West Bengal, India
D. Banerjee
Centre for Mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Celestijnenlaan 200B, 3001, Leuven, Belgium
S. Krishna Prasad & T. Van Doorsselaere
Northumbria University, Newcastle Upon Tyne, NE1 8ST, UK
J. A. McLaughlin
Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, NE1 8ST, UK
P. Antolin
Centre for Fusion, Space and Astrophysics, Physics Department, University of Warwick, Coventry, CV4 7AL, UK
N. Magyar
The Catholic University of America and NASA Goddard Space Flight Center, Code 671, Greenbelt, MD, 20771, USA
L. Ofman & T. J. Wang
School of Earth and Space Sciences, Peking University, Beijing, 100871, China
H. Tian
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China
H. Tian
School of Mathematics and Statistics, University of St. Andrews, St. Andrews, KY16 9SS, UK
I. De Moortel
Rosseland Centre for Solar Physics, University of Oslo, PO Box 1029, Blindern, 0315, Oslo, Norway
I. De Moortel

Authors

D. Banerjee
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S. Krishna Prasad
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V. Pant
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J. A. McLaughlin
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P. Antolin
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N. Magyar
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L. Ofman
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H. Tian
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T. Van Doorsselaere
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I. De Moortel
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T. J. Wang
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Correspondence to D. Banerjee.

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Oscillatory Processes in Solar and Stellar Coronae

Edited by Valery M. Nakariakov, Dipankar Banerjee, Bo Li, Tongjiang Wang, Ivan Zimovets and Maurizio Falanga

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Banerjee, D., Krishna Prasad, S., Pant, V. et al. Magnetohydrodynamic Waves in Open Coronal Structures. Space Sci Rev 217, 76 (2021). https://doi.org/10.1007/s11214-021-00849-0

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Received: 12 December 2020
Accepted: 25 August 2021
Published: 21 September 2021
DOI: https://doi.org/10.1007/s11214-021-00849-0

Keywords

Solar corona
Magnetohydrodynamics
Waves and oscillations