A physical mechanism of solar corona heating
classification
🌌 astro-ph.SR
keywords
solarcoronax-raysoftbackgrounddataheatingmicroflares
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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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