Self-consistent modelling of pulsar magnetospheres

Herold, Heinz; Ertl, Thomas; Finkbeiner, Bernd; Ruder, Hanns

Self-consistent modelling of pulsar magnetospheres

dc.contributor.author	Herold, Heinz	de
dc.contributor.author	Ertl, Thomas	de
dc.contributor.author	Finkbeiner, Bernd	de
dc.contributor.author	Ruder, Hanns	de
dc.date.accessioned	2012-09-05	de
dc.date.accessioned	2016-03-31T11:44:59Z
dc.date.available	2012-09-05	de
dc.date.available	2016-03-31T11:44:59Z
dc.date.issued	1989	de
dc.date.updated	2012-09-25	de
dc.description.abstract	The magnetosphere of a rapidly rotating, strongly magnetized neutron star with aligned magnetic and rotational axes (parallel rotator) is modelled numerically. Including the radiation of the particles accelerated to relativistic energies as an efficient damping mechanism, we obtain a quasi-stationary selfconsistent solution to this classical problem. The numerical simulation, which was started from the well-known vacuum solution, yields a global magnetospheric structure that can be characterized by two regions of oppositely charged particles, which eventually produce a relativistic pulsar wind, separated by a vacuum gap of considerable extent.	en
dc.identifier.other	371589320	de
dc.identifier.uri	http://nbn-resolving.de/urn:nbn:de:bsz:93-opus-76990	de
dc.identifier.uri	http://elib.uni-stuttgart.de/handle/11682/8051
dc.identifier.uri	http://dx.doi.org/10.18419/opus-8034
dc.language.iso	en	de
dc.rights	info:eu-repo/semantics/openAccess	de
dc.subject.classification	Röntgenpulsar , Magnetosphäre , Mathematische Modellierung	de
dc.subject.ddc	530	de
dc.title	Self-consistent modelling of pulsar magnetospheres	en
dc.type	conferenceObject	de
ubs.fakultaet	Fakultätsübergreifend / Sonstige Einrichtung	de
ubs.institut	Sonstige Einrichtung	de
ubs.opusid	7699	de
ubs.publikation.source	Ögelmann, Hakki (Hrsg.): Timing neutron stars. Dordrecht : Kluwer, 1989 (NATO ASI series, C 262). - ISBN 0-7923-0101-3, S. 723-729	de
ubs.publikation.typ	Konferenzbeitrag	de

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