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Thorough numerical studies of the characters of maserinstability driven by a b eam of weak relativistic electrons are performed on the basis of the theoretical model of Chen et al due to its important applicatio n in the solar radio emission. It enriches the f undamental content of the plasma instabilities. And it is expected to be applica ble widely in the study of solar and celestial emission mechanism.
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Keywords:
- maserinstability /
- weak relativistic e lectron beam /
- growth rate
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