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

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dc.creatorSlowikowska, A.
dc.creatorJessner, A.
dc.creatorKlein, B.
dc.creatorKanbach, G.
dc.date2005-11-20
dc.date2005-11-21
dc.date.accessioned2026-07-07T12:29:04Z
dc.date.available2026-07-07T12:29:04Z
dc.descriptionWe 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.
dc.descriptionAIP Conference Proceedings "Astrophysical Sources of High Energy Particles and Radiation", eds. T. Bulik et al. (NY:AIP), Volume 801, 2005, pp. 324-329
dc.identifierhttps://arxiv.org/abs/astro-ph/0511599
dc.identifierhttp://arxiv.org/abs/astro-ph/0511599
dc.identifierAstrophysical Sources Of High Energy Particles And Radiation. AIP Conference Proceedings, Volume 801, pp. 324-329 (2005)
dc.identifierdoi:10.1063/1.2141893
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215752
dc.subjectAstrophysics
dc.titlePolarization characteristics of the Crab pulsar's giant radio pulses at HFCs phases
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