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Why the outer regions of the solar atmosphere are much hotter than the underlying surface is a long-standing question. New high-resolution observations revise the role of waves in the energy
transfer and offer an insight into the processes at play. Access through your institution Buy or subscribe This is a preview of subscription content, access via your institution ACCESS
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480–483 (2018). Article Google Scholar Download references AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * ASI Italian Space Agency, Rome, Italy Marco Stangalini Authors * Marco Stangalini
View author publications You can also search for this author inPubMed Google Scholar CORRESPONDING AUTHOR Correspondence to Marco Stangalini. ETHICS DECLARATIONS COMPETING INTERESTS The
author declares no competing interests. RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Stangalini, M. Wave energy in the solar atmosphere. _Nat Astron_
7, 761–762 (2023). https://doi.org/10.1038/s41550-023-01955-5 Download citation * Published: 25 May 2023 * Issue Date: July 2023 * DOI: https://doi.org/10.1038/s41550-023-01955-5 SHARE THIS
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