Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-19T22:06:04.801Z Has data issue: false hasContentIssue false
  • English
  • Français

The Locations of the Core and Conal Emission Regions in an Inverse-Compton Scattering Model

Published online by Cambridge University Press:  27 September 2017

G. J. Qiao ,
C. G. Li  and
M. Li
G. J. Qiao
Affiliation:
Center of Astronomy and Astrophysics, CCTS (World Laboratory) and Department of Geophysics, Peking University
C. G. Li
Affiliation:
Department of Geophysics, Peking University
M. Li
Affiliation:
Department of Geophysics, Peking University

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The physical conditions and locations of the emission regions for core and hollow cone emissions are very important in understanding the mechanism of radio pulsars. We present two related methods in an Inverse-Compton Scattering (ICS) model in this paper, which give a clear scenario for determining the location of the emission regions and are consistent with the results given by Cordes et al. (1984) and Rankin (1990).

Type
Part VI Polar cap theories
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 242 - 244
Copyright
Copyright © United States Naval Observatory 1992