Physics
Scientist
Beijing Astronomical Observatory, Chinese Academy of Sciences
Beijing Observatory, Academia Sinica
A 2.84 GHz ms-resolution receiver and the question about the reliability of the 205 solar UFFS data taken with it
On the interpretation of the 2.84 GHz solar UFFS data of May 16, 1981
The Energetic Spectrum of Non-Thermal Electrons in an Acceleration Region Calculated From a Solar Microwave Type III Burst with both Positive and Negative Frequency Drifts
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