1999/11/22 by Vladimir V. Usov, Usov, Vladimir V.
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Earthquake Detection and Analysis #Geophysics and Sensor Technology #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9911403
4 pages, to be published in proceedings of "Pulsar Astronomy - 2000 and Beyond", ASP Conf. Ser
arxiv created 1999/11/22 · arxiv updated 2009/12/01
We discuss plausible locations of radiating regions in the magnetospheres of pulsars and argue that the mechanisms of pulsar radiation at different frequencies are closely connected with the locations of the radiating regions, especially in the radio range. If the region that is responsible for the bulk of the non-thermal radiation at some frequency is localized in the pulsar magnetosphere then the nature of this radiation will be either determined or, at least, restricted significantly.