Bitte benutzen Sie diese Kennung, um auf die Ressource zu verweisen:
http://dx.doi.org/10.18419/opus-8030
| Autor(en): | Herold, Heinz Ertl, Thomas Finkbeiner, Bernd Ruder, Hanns |
| Titel: | Self-consistent numerical modelling of pulsar magnetospheres |
| Erscheinungsdatum: | 1992 |
| Dokumentart: | Konferenzbeitrag |
| Erschienen in: | Hankins, Timothy H. (Hrsg.): The magnetospheric structure and emission mechanisms of radio pulsars. Zielona Góra : Pedagogical Univ. Pr., 1992 (Proceedings of the … colloquium of the International Astronomical Union 128). - ISBN 83-00-03596-6, S. 105-108 |
| URI: | http://nbn-resolving.de/urn:nbn:de:bsz:93-opus-76870 http://elib.uni-stuttgart.de/handle/11682/8047 http://dx.doi.org/10.18419/opus-8030 |
| Zusammenfassung: | 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 self-consistent 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. |
| Enthalten in den Sammlungen: | 15 Fakultätsübergreifend / Sonstige Einrichtung |
Dateien zu dieser Ressource:
| Datei | Beschreibung | Größe | Format | |
|---|---|---|---|---|
| ert6.pdf | 951,45 kB | Adobe PDF | Öffnen/Anzeigen |
Alle Ressourcen in diesem Repositorium sind urheberrechtlich geschützt.