Please use this identifier to cite or link to this item: http://dx.doi.org/10.18419/opus-8044
Authors: Herold, Heinz
Ertl, Thomas
Finkbeiner, Bernd
Ruder, Hanns
Title: Towards a self-consistent modelling of pulsar magnetospheres
Issue Date: 1987
metadata.ubs.publikation.typ: Konferenzbeitrag
metadata.ubs.publikation.source: Williams, William Terry (Hrsg.): XVIII. International Conference on Phenomena in Ionized Gases : Swansea 13th - 17th July 1987. Bristol, UK : Hilger, 1987. - ISBN 0-9511848-0-6, S. 234-235
URI: http://nbn-resolving.de/urn:nbn:de:bsz:93-opus-77208
http://elib.uni-stuttgart.de/handle/11682/8061
http://dx.doi.org/10.18419/opus-8044
Abstract: The numerical modelling of the general case of an oblique rotator is a very complicated time-dependent 3-dimensional problem and in its full extent probably outside the capicity of present.day computers. A considerable simplification occurs if one can assume that the essential effects may be understood by modelling the magnetosphere of an aligned rotator (where the rotation axis is parallel to the magnetic axis of the neutron star). This assumption is only reasonable for small obliqueness, since by this approach all electromagnetic wave effects are not taken into account.
Appears in Collections:15 Fakultätsübergreifend / Sonstige Einrichtung

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