On high brightness temperature of pulsar giant pulses

Details On high brightness temperature of pulsar giant pulses On high brightness temperature of pulsar giant pulses

2009-11-17

arxiv.org/abs/0911.3272v3

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

19 pages, 2 Postscript figures; added and corrected references, corrected misprints and abbreviation. The 8th International Co

Scientific paper

Giant pulses (GP) observed in a number of pulsars show a record brightness temperature. Comparable energy densities in the radio-frequency region are attainable in a cavity-resonator being the pulsar internal vacuum gap. A wide range of events observed at GP (intensity, localization, circular polarization, duration, power low, correlation with hard emission) can be explained from the viewpoint that the internal vacuum gap is a cavity stimulated by discharges and radiating through the breaks in the magnetosphere. Superimposed separate discharges form the fine structure of GP.

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