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Correction: The influence of opacity on inferred MHD wave signatures in the lower solar atmosphere

Samuel J. Skirvin*, Samuel D. T. Grant, David B. Jess, Ryan J. Campbell, Shahin Jafarzadeh, Mika V. Kontiainen, Michele Berretti, Timothy J. Duckenfield, Glen Chambers, Marco Stangalini, Luc Rouppe van de Voort

*Corresponding author for this work

Research output: Contribution to journalComment/debatepeer-review

Abstract

A Correction on
The influence of opacity on inferred MHD wave signatures in the lower solar atmosphere
by Skirvin SJ, Grant SDT, Jess DB, Campbell RJ, Jafarzadeh S, Kontiainen MV, Berretti M, Duckenfield TJ, Chambers G, Stangalini M and Rouppe van der Voort L (2026). Front. Astron. Space Sci. 13:1814323. doi: 10.3389/fspas.2026.1814323

Incorrect data availability statement.

The Data Availability statement was erroneously given as “The raw data supporting the conclusions of this article will be made available by the authors, without undue reservation”.

The correct Data Availability statement is below.

“The data behind figures are available in Figshare at DOI: 10.25398/rd.northumbria.30896033. Additional data supporting the findings of this study are available from the corresponding author upon reasonable request.”

The original version of this article has been updated.
Original languageEnglish
Article number1926327
Number of pages1
JournalFrontiers in Astronomy and Space Sciences
Volume13
DOIs
Publication statusPublished - 28 Jul 2026

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