New UKSP Nugget #76

February 8, 2017, from Iain Hannah

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://www.uksolphys.org/uksp-nuggets

Iain Hannah and Lyndsay Fletcher

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http://www.uksolphys.org/?p=12381


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