MAGNETOSPHERIC GAP AND ACCUMULATION OF GIANT PLANETS CLOSE TO THE STAR 

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Animation shows instabilities at the disk-magnetosphere boundary which appear in case of low gamma (g=1.1).  Background shows density distribution in the equatorial plane.

[video] (.avi,  3.3 MBt) 

 

Animation shows instabilities at the disk-magnetosphere boundary. Green background shows one of the density levels. Red lines are sample magnetic field lines.

[video] (.avi,  4.0 MBt) 

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