Recent YOHKOH solar gamma-ray observations

Physics

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Scientific paper

Yohkoh observed two γ-ray flares in 2000, a X5.7 flare at 10:20 UT on 14 July and a X2.3 flare at 15:08 UT on November 24, with the hard X/γ-ray spectrometers and hard X-ray imager. The two flares emitted several nuclear γ-ray lines and hard X-ray images indicate two sources which are located at both footpoints of the magnetic loop. At the beginning of the peak phase of the July 14 flare, the temporal evolution of the hard X-ray sources suggests that a change in the magnetic loop structure from high-shearing to low-shearing states is associated with magnetic reconnection. Particle accleration is discussed based on the Yohkoh spectroscopic and imaging data.

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