Formation of filament-like structures in the pulsar magnetosphere and the short-term variability of pulsar emission
V. UrpinA.F. Ioffe Institute of Physics and Technology and Isaac Newton Institute of Chile, Branch in St. Petersburg, 194021 St. Petersburg, Russia
2014en
ABI
Аннотация
Context. Magnetohydrodynamic (MHD) instabilities can play an important role in the dynamics of the pulsar magnetosphere and can be responsible for the formation of various structures.
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