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- W1669423310 abstract "Aims. We present the results of the numerical simulations of the interaction between a magnetized star and an imperfectly conducting accretion disk. Methods. To analyze the ”star‐disk” interaction we numerically investigate the MHD equations used Godunov-type high resolution numerical method. Results. It was found that the ”star ‐ disk” interaction occurs with quasi-periodic reconnection of the magnetic field coronal loo ps and plasmoid ejections. In the case of the perfect disk conductivity the evolution of the coronal magnetic field leads to the p eriodic outflow of angular momentum from the disk. In the case of an imperfectly conducting disk the configuration of the magnetic field is for med such that the disk angular momentum carried by magnetic field gets balance d by angular momentum carried by matter." @default.
- W1669423310 created "2016-06-24" @default.
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- W1669423310 date "2006-03-31" @default.
- W1669423310 modified "2023-09-27" @default.
- W1669423310 title "Numerical simulations of coronal magnetic field loop evolut ion" @default.
- W1669423310 cites W1639168386 @default.
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