A physical mechanism of solar corona heating

Details A physical mechanism of solar corona heating A physical mechanism of solar corona heating

2011-06-15

arxiv.org/abs/1106.2941v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

e-mail: colombo2006@mail.ru

Scientific paper

Time profiles of solar soft X-ray microflares and structure soft X-ray solar
corona thermal background are studied on RHESSI data. The observations of 2003
year are analyzed. Decrease fluxe of solar soft X-ray microflares and thermal
background of solar corona in the X-ray range 2-15 kev are revealed. The new
model of solar corona heating in based on this new data are suggested.

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