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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