Amazing properties of giant pulses and the nature of pulsar's radio emission
| dc.creator | Soglasnov, V. | |
| dc.date | 2007-01-08 | |
| dc.date.accessioned | 2026-07-07T07:38:57Z | |
| dc.date.available | 2026-07-07T07:38:57Z | |
| dc.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. | |
| dc.description | 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 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701190 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701190 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/121280 | |
| dc.subject | Astrophysics | |
| dc.title | Amazing properties of giant pulses and the nature of pulsar's radio emission | |
| dc.type | text |