Abstract:
Spectral observations of the Sun in the frequency range of 54 to
78 MHz in the November 24, 2000 solar flare showed quasi - periodic pulsations
with periods in the range of 11 - 19 seconds. YOHKOH images of this flare in
the active region AR 9236 showed loop structures. Assuming an impulsively
generated propagating MHD wave for the pulsations, the coronal magnetic field
at 1.6 R0 height is derived as '" 8 Gauss.