Analyzing observations of multiple small center of solar flares at a wavelength of 195 Å

Details Analyzing observations of multiple small center of solar flares at a wavelength of 195 Å Analyzing observations of multiple small center of solar flares at a wavelength of 195 Å

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ge%26ae..48..709s&link_type=abstract

Geomagnetism and Aeronomy, Volume 48, Issue 6, pp.709-712

Physics

96.60.Rd

Scientific paper

The duration of elementary eruption process and intervals between them for flares of different importance have been determined based on the photometric data for flares, observed by a TRACE spacecraft at a wavelength of 195 Å. It has been revealed that the values of these parameters increase with increasing flare importance. It is assumed that the appearance of elementary nonstationary flare centers correlates with the origination of solitons at self-organized criticality.

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