Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-07-09
Astrophys.SpaceSci.308:575-579,2007
Astronomy and Astrophysics
Astrophysics
5 pages, 4 figures. Presented at the conference "Isolated Neutron Stars: from the Interior to the Surface", London, April 24-2
Scientific paper
10.1007/s10509-007-9348-4
Here we briefly report on results of self-consistent numerical modeling of a differentially rotating force-free magnetosphere of an aligned rotator. We show that differential rotation of the open field line zone is significant for adjusting of the global structure of the magnetosphere to the current density flowing through the polar cap cascades. We argue that for most pulsars stationary cascades in the polar cap can not support stationary force-free configurations of the magnetosphere.
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