Abstract
We briefly introduce our recent work on the spectral evolution of energetic protons, the beam property of accelerated electrons, the gamma-ray flare classification, the temporal features of the annihilation line, the hard X-ray delayed events, the hydrodynamic process, and the continuum emission in solar flares.
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Gan, W., Chang, J., Li, Y. et al. Solar hard X-rays and gamma-rays. Sci. China Ser. A-Math. 45 (Suppl 1), 30–35 (2002). https://doi.org/10.1007/BF02889681
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DOI: https://doi.org/10.1007/BF02889681