Polarization characteristics of the Crab pulsar's giant radio pulses at HFCs phases

Details Polarization characteristics of the Crab pulsar's giant radio pulses at HFCs phases Polarization characteristics of the Crab pulsar's giant radio pulses at HFCs phases

2005-11-20

arxiv.org/abs/astro-ph/0511599v2

Astrophysical Sources Of High Energy Particles And Radiation. AIP Conference Proceedings, Volume 801, pp. 324-329 (2005)

Astronomy and Astrophysics

Astrophysics

AIP Conference Proceedings "Astrophysical Sources of High Energy Particles and Radiation", eds. T. Bulik et al. (NY:AIP), Volu

Scientific paper

10.1063/1.2141893

We discuss our recent discovery of the giant radio emission from the Crab pulsar at its high frequency components (HFCs) phases and show the polarization characteristic of these pulses. This leads us to a suggestion that there is no difference in the emission mechanism of the main pulse (MP), interpulse (IP) and HFCs. We briefly review the size distributions of the Crab giant radio pulses (GRPs) and discuss general characteristics of the GRP phenomenon in the Crab and other pulsars.

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