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Magnetohydrodynamic Waves in Open Coronal Structures
DOI: 10.1007/s11214-021-00849-0 Bibcode: 2021SSRv..217...76B

Tian, H.; Wang, T. J.; Banerjee, D. +8 more

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 reg…

2021 Space Science Reviews
IRIS 66