Energy Balance in the Corona Over the 22-Year Solar Cycle

Details Energy Balance in the Corona Over the 22-Year Solar Cycle Energy Balance in the Corona Over the 22-Year Solar Cycle

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh13a1161l&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH13A-1161

Physics

7519 Flares, 7536 Solar Activity Cycle (2162)

Scientific paper

A model for dynamic energy balance in the solar corona over the 11-year solar cycle is presented. The model predicts that the flaring rate in the corona should lag behind the solar-cycle related driving because of the coronal response time of order 9 months. This effect may explain hysteresis phenomena between solar activity indices. The model can also incorporate 22-year driving consistent with the Gnevyshev-Ohl rule. The modified model in principle accounts for the observed variation of the flaring time lag for odd and even solar cycles.

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