Towards a self-consistent modelling of pulsar magnetospheres

dc.contributor.authorHerold, Heinzde
dc.contributor.authorErtl, Thomasde
dc.contributor.authorFinkbeiner, Berndde
dc.contributor.authorRuder, Hannsde
dc.date.accessioned2012-09-17de
dc.date.accessioned2016-03-31T11:45:00Z
dc.date.available2012-09-17de
dc.date.available2016-03-31T11:45:00Z
dc.date.issued1987de
dc.description.abstractThe 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.en
dc.identifier.other372015077de
dc.identifier.urihttp://nbn-resolving.de/urn:nbn:de:bsz:93-opus-77208de
dc.identifier.urihttp://elib.uni-stuttgart.de/handle/11682/8061
dc.identifier.urihttp://dx.doi.org/10.18419/opus-8044
dc.language.isoende
dc.rightsinfo:eu-repo/semantics/openAccessde
dc.subject.classificationRöntgenpulsar , Magnetosphäre , Mathematische Modellierungde
dc.subject.ddc520de
dc.titleTowards a self-consistent modelling of pulsar magnetospheresen
dc.typeconferenceObjectde
ubs.fakultaetFakultätsübergreifend / Sonstige Einrichtungde
ubs.institutSonstige Einrichtungde
ubs.opusid7720de
ubs.publikation.sourceWilliams, 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. 234-235de
ubs.publikation.typKonferenzbeitragde

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