A Possible Difficulty with a Nanoflare-Heated Corona

Details A Possible Difficulty with a Nanoflare-Heated Corona A Possible Difficulty with a Nanoflare-Heated Corona

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..167..267c&link_type=abstract

Solar Physics, Volume 167, Issue 1-2, pp. 267-279

Physics

5

Scientific paper

Spectral line profiles associated with the nanoflare model of coronal
heating are computed. It is shown that the reconnection jets associated
with this heating model lead to Doppler shifts or line broadening of
coronal spectral lines in excess of those observed. Some possible
resolutions of the problem are suggested.

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