TWO-FLUID MODEL OF THE MAGNETOSPHERE AS A BASIS FOR DESCRIPTION OF PULSAR EMISSION
Purpose: The self-consistent two-fluid model for the stationary axisymmetric magnetosphere of a pulsar is considered. Design/methodology/approach: Taking into account infinitesimal inertial effects, the zero- and first-order equations are solved. The general results are applied to the case of a s...
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| Format: | Article |
| Language: | English |
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National Academy of Sciences of Ukraine, Institute of Radio Astronomy
2016-12-01
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| Series: | Radio Physics and Radio Astronomy |
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| Online Access: | http://rpra-journal.org.ua/index.php/ra/article/view/1246/pdf |