Physics
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aujph..32...71e&link_type=abstract
(Joint Australia-USSR-USA Symposium on Pulsars and Supernova Remnants, Sydney, Australia, Apr. 1978.) Australian Journal of Phys
Physics
1
Atmospheric Models, Neutron Stars, Stellar Atmospheres, Stellar Magnetospheres, Stellar Models, Magnetic Field Configurations, Pulsar Magnetospheres, Stellar Radiation
Scientific paper
The problem of modeling a rotating neutron star magnetosphere is discussed. Attention is drawn to the possibility of qualitative modeling of this cosmic object without conforming to the similarity laws. Two models, one simulating an aligned magnetic rotator and the other an oblique rotator, are suggested. Preliminary results from such modeling of pulsar magnetospheres in the oblique rotator case are reported.
Eremin B. G.
Kostrov Alexander V.
Slutsker Ia. Z.
Suvorov E. V.
Zhelezniakov Vladimir V.
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