Conditions for steady circulation in rotating magnetic stars with finite electrical conductivity
dc.contributor.author | Maheswaran, M. | en_US |
dc.date.accessioned | 2010-07-06T11:08:11Z | |
dc.date.available | 2010-07-06T11:08:11Z | |
dc.date.issued | 1975 | en_US |
dc.identifier.citation | Journal of the National Science Council, 3(1):p.11-17 | en_US |
dc.identifier.uri | https://dl.nsf.gov.lk/handle/1/6435 | |
dc.publisher | NSC:Colombo | en_US |
dc.subject | Magnetohydrodynamics | en_US |
dc.subject | Stellar | en_US |
dc.subject | Physics | en_US |
dc.subject.lcc | Physics | en_US |
dc.title | Conditions for steady circulation in rotating magnetic stars with finite electrical conductivity | en_US |
dc.type | Article | en_US |