Solar cycle variations of the soft X-ray background flux and its relation to flare occurrence

Details Solar cycle variations of the soft X-ray background flux and its relation to flare occurrence Solar cycle variations of the soft X-ray background flux and its relation to flare occurrence

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..259v&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Physics

Solar Cycles: Variations, Soft X-Ray Background

Scientific paper

The X-ray background flux (XBF) based on GOES 1-8 Å measurements for the period 1975-2000 is studied. We come to the conclusion that in the XBF the flare contribution is not eliminated but the XBF is dominated by flare and post-flare emission of intense events. Furthermore, we suggest that the characteristic lag of the X-ray background flux with regard to Sunspot Numbers reported for cycle 21 is a secondary effect related to the substantial contribution of large flares to the XBF.

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