2010/08/06 by A. Zajczyk, Anna Zajczykab, B. Rudak +5
Earth and Planetary Sciences · Physics and Astronomy · #FOS: Physical sciences #Geophysics and Gravity Measurements #High Energy Astrophysical Phenomena (astro-ph.HE) #Magnetic confinement fusion research #Pulsars and Gravitational Waves Research #astro-ph.HE
paper · pdf · doi:10.48550/arxiv.1008.1176
6 pages, 2 figures, to be published in proceedings of "HTRA IV - The Era of Extremely Large Telescopes" conference
arxiv created 2010/08/06 · openalex publication_date 2010/08/06 · arxiv updated 2010/08/09 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28
Resluts of 3D numerical simulations in the framework of pair starved polar cap model (PSPC) for millisecond pulsars are presented. In the investigated PSPC model electric field structure highly depends on the pulsar inclination which is clearly visible in the computed spectra of electrons escaping pulsar magnetosphere which become bimodal with the increasing inclination. This is an important result for modelling very high energy radiation from globular clusters where currently the standard power law or monoenergetic electron distributions are used.