Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 676, Issue 1, Pages L73-L75Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/587029
Keywords
MHD; sun : corona; sun : oscillations
Categories
Funding
- Engineering and Physical Sciences Research Council [EP/D062837/1] Funding Source: researchfish
- Science and Technology Facilities Council [ST/F00205X/1] Funding Source: researchfish
- EPSRC [EP/D062837/1] Funding Source: UKRI
- STFC [ST/F00205X/1] Funding Source: UKRI
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Recently, the omnipresence of waves has been discovered in the corona using the CoMP instrument. We demonstrate that the observational findings can be explained in terms of guided kink magnetoacoustic modes. The interpretation of the observations in terms of Alfven waves is shown to be inconsistent with MHD wave theory. The implications of the interpretation in terms of kink waves are discussed.
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