THE MAGNETIC FIELD IMPACT ON ACCRETION RATE IN A PROTOPLANETARY DISK
Recent observations are the evidence of a large-scale magnetic field in discs around classical T Tauri stars. A model of the axisymmetric thin protoplanetary disk in a global magnetic field is considered. A compressible magnetohydrodynamic set of equations is solved by using the explicit numerical m...
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| Format: | Article |
| Language: | English |
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Odessa I. I. Mechnykov National University
2012-11-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/83348 |