Why is the corona hot? Micro- and nano-flares and the solar corona.

Details Why is the corona hot? Micro- and nano-flares and the solar corona. Why is the corona hot? Micro- and nano-flares and the solar corona.

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998asthe..91..399s&link_type=abstract

Astronomical Herald, Vol. 91, No. 9, p. 399 - 405

Astronomy and Astrophysics

Astrophysics

Solar Corona: Temperatures, Solar Corona: Solar Flares

Scientific paper

The solar corona is the upper atmosphere which consists of faint, hot (>2 million K degree) plasma. Why is the corona so hot? This is one of fundamental questions in astrophysics. Micro- and nano-flares have been recently considered as a mechanism for energy dissipation in the corona. The soft X-ray telescope on board the Yohkoh satellite enables one for the first time to investigate micro- and nano-flares. This article introduces some observational results of micro- and nano-flares, and discusses their implications for heating of the corona.

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