Numerical modelling of pulsar magnetosph
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M. PetraviΔ
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Article
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1976
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Elsevier Science
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English
β 777 KB
Numerical models used in the study ofthe pulsar magnetosphere are described: a vacuum model based only on Maxwell's equations and a more realistic model employing both Maxwell's and relativistic two-fluid equations. The general approach to solving the chosen Sets of partial differential equations is