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Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..314p&link_type=abstract
ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 314-315 (2005).
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Pulsars, Radiative Transfer, Magnetospheric Electromagnetic Wave Propagation, Stellar Atmospheres, Electromagnetic Wave Polarisation, Pulsars, Radiative Transfer, Scattering, Emission, Absorption, And Scattering Of Electromagnetic Radiation, Radiation Mechanisms, Polarization
Scientific paper
Giant radio pulses are explained in terms of induced Compton scattering by the secondary plasma particles in pulsar magnetosphere. This process can account for the energetics and statistics of giant pulses as well as for their substructure at nanosecond timescales. The mechanism suggested predicts strong polarization of giant radiation in the plane of the ambient magnetic field.
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