A physical mechanism of solar corona heating
I. K. Mirzoeva (Space Research Institute, Russian Academy of Sciences,, Moscow)
TL;DR
This paper analyzes RHESSI data from 2003 to study solar soft X-ray microflares and the corona's thermal background, proposing a new physical model for solar corona heating based on observed decreases in X-ray flux.
Contribution
It introduces a new model for solar corona heating derived from analysis of microflare and thermal background data from RHESSI observations.
Findings
Decrease in solar soft X-ray microflare flux observed.
Decrease in thermal background of solar corona detected.
A new physical model for corona heating is proposed.
Abstract
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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Taxonomy
TopicsSolar and Space Plasma Dynamics