Physics
Scientist
Institute of High Energy Physics, Academia Sinica, Beijing 100039
A model for enhancement of the flux of very high energy particles during large solar flares.
A very high energy GLE event possibly associated with the X solar flare of 15th June 1991.
Atmospheric Cherenkov telescope.
Correlation between Sun shadows of 10 TeV cosmic rays and solar activity.
Identification of primary cosmic ray particles producing big gamma-families in emulsion chambers.
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