HR: 1340h
AN: SH13A-1161    [Abstracts]
TI: Energy Balance in the Corona Over the 22-Year Solar Cycle
AU: * Litvinenko, Y
EM: yuri.litvinenko@unh.edu
AF: University of NH, 39 College Road, Morse Hall, Durham, NH 03824 United States
AB: 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.
DE: 7519 Flares
DE: 7536 Solar activity cycle (2162)
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2004 AGU Fall Meeting