The CKF solution of pulsar magnetospheres

Details The CKF solution of pulsar magnetospheres The CKF solution of pulsar magnetospheres

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..312b&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 312-313 (2005).

Computer Science

Numerical Analysis

Pulsars, Stellar Atmospheres, Numerical Analysis, Pulsars, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

We continue the pulsar magnetosphere calculations of Contopoulos, Kazanas and Fendt. The assumptions of the model are listed and illustrated. Different grids from 30×30 up to 150×150 are used, though high resolution is not so important for determining the source function if only an appropriate convergence scheme is used (substantially different from the approach, to be published elsewhere). We compactify the physical space to carry out integration on a finite grid.

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