3D MHD SIMULATIONS OF DISK ACCRETION TO AN INCLINED ROTATOR.  MAGNETOSPHERIC FLOW AT DIFFERENT Q

Animation shows rotation of the star around the rotational axis W  at different inclination anlgles Q and different viewing angles i . Red lines show selected magnetic field lines, background - one of density contour levels. All plots are taken for one moment of time: t = 5P0, where P0 is period of rotation at the inner radius of the disk. Only inner part (1/5) of simulation region is shown.

Q - is an  angle between magnetic axis of the dipole m and rotational axis W.
i - is an angle between direction to the observer and rotational axis W.

1.  Q = 30 and Q = 90 at different projections

  Q = 30 Q = 90
X [video, avi] [video, avi]
Z [video, avi] [video, avi]

2.  3D flows at different inclination angles i of the disk

  Q = 15 Q = 30 Q = 45 Q = 60 Q = 75
i = 15 [video, avi] [video, avi] [video, avi] [video, avi] [video, avi]
i = 45 [video, avi] [video, avi] [video, avi] [video, avi] [video, avi]
i = 75 [video, avi] [video, avi] [video, avi] [video, avi] [video, avi]

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created by O. Toropina, 2000-2004Your comments are welcome
2000-2007, last updated on 29.01.07