76. Non-thermal line broadening in flaring coronal loops
by Mykola Gordovskyy, Philippa Browning (Manchester) & Eduard Kontar (Glasgow)
Broad spectral line profiles in flares can be explained by flows and turbulence in a twisting, reconnecting loop.
76. Non-thermal line broadening in flaring coronal loops
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UKSP Nuggets are published on a monthly basis highlighting solar physics research led from the UK.
http://uksolphys.org/uksp-nuggets
Iain Hannah and Lyndsay Fletcher
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