Jess, D.B., Morton, R.J., Verth, G. et al. (3 more authors) (2015) Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results. Space Science Reviews. Published Online 05 Mar 2015 . ISSN 0038-6308
Abstract
The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool photosphere and the intensely heated transition region and corona. Compressible and incompressible waves propagating through the chromosphere can supply significant amounts of energy to the interface region and corona. In recent years an abundance of high-resolution observations from state-of-the-art facilities have provided new and exciting ways of disentangling the characteristics of oscillatory phenomena propagating through the dynamic chromosphere. Coupled with rapid advancements in magnetohydrodynamic wave theory, we are now in an ideal position to thoroughly investigate the role waves play in supplying energy to sustain chromospheric and coronal heating. Here, we review the recent progress made in characterising, categorising and interpreting oscillations manifesting in the solar chromosphere, with an impetus placed on their intrinsic energetics.
Metadata
Item Type: | Article |
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Authors/Creators: |
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Copyright, Publisher and Additional Information: | © 2015 Springer. This is an author produced version of a paper subsequently published in Space Science Reviews. Uploaded in accordance with the publisher's self-archiving policy. |
Keywords: | astro-ph.SR; astro-ph.SR |
Dates: |
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Institution: | The University of Sheffield |
Academic Units: | The University of Sheffield > Faculty of Engineering (Sheffield) > Department of Automatic Control and Systems Engineering (Sheffield) |
Depositing User: | Symplectic Sheffield |
Date Deposited: | 19 May 2015 14:54 |
Last Modified: | 15 Mar 2016 16:56 |
Published Version: | http://dx.doi.org/10.1007/s11214-015-0141-3 |
Status: | Published |
Publisher: | Springer |
Identification Number: | 10.1007/s11214-015-0141-3 |
Related URLs: | |
Open Archives Initiative ID (OAI ID): | oai:eprints.whiterose.ac.uk:86089 |