TY  - CHAP
U1  - Konferenzveröffentlichung
A1  - Słowikowska, A.
A1  - Jessner, A.
A1  - Klein, B.
A1  - Kanbach, G.
T1  - Polarization characteristics of the Crab pulsar’s giant radio pulses at HFCs phases
T2  - Bulik, Rudak et al. (Eds.): Astrophysical Sources of High Energy Particles and Radiation. Torun (Poland), 20-24 June 2005
N2  - 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.
KW  - electromagnetic wave polarisation
KW  - Pulsars
KW  - stellar radiation
SN  - 0-7354-0290-6
SB  - 0-7354-0290-6
U6  - https://doi.org/10.1063/1.2141893
DO  - https://doi.org/10.1063/1.2141893
SP  - 324
EP  - 329
PB  - AIP Publishing
ER  -