Amazing properties of giant pulses and the nature of pulsar's radio emission
Abstract
Description
For comprehensive studying of giant pulses (GPs) from the Crab pulsar and the original millisecond pulsar (MSP) B1937+21 (J1939+2134), we conducted multifrequency observations over the last few years. They show that giant pulses may be improbably bright, 10^5, 10^6 Jy and more, they have extra ordinal spectra and polarization. EM energy concentrated in such strong pulse is high enough to accelerate particles up to Lorenz factor gamma ~ 10^4 - 10^6, since giant pulses may play an important role in physics of pulsar's magnetosphere.
Proceedings of the 363. WE-Heraeus Seminar on: Neutron Stars and Pulsars (Posters and contributed talks) Physikzentrum Bad Honnef, Germany, May.14-19, 2006, eds. W.Becker, H.H.Huang, MPE Report 291, pp.68-71
Proceedings of the 363. WE-Heraeus Seminar on: Neutron Stars and Pulsars (Posters and contributed talks) Physikzentrum Bad Honnef, Germany, May.14-19, 2006, eds. W.Becker, H.H.Huang, MPE Report 291, pp.68-71