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THE
PROPELLER REGIME OF DISK ACCRETION TO A RAPIDLY ROTATING MAGNETIZED STAR PROPELLER-DRIVEN OUTFLOWS AND DISK OSCILLATIONS [return] |
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THE
PROPELLER REGIME OF DISK ACCRETION TO A RAPIDLY ROTATING MAGNETIZED STAR PROPELLER-DRIVEN OUTFLOWS AND DISK OSCILLATIONS [return] |
| Quasi-periodic accretion and
outflows in propeller regime. Parameters: avis=0.3, adif=0.2.
Color background shows density, lines are magnetic field lines.
Evolution is shown for time interval from 800 to 1000 rotations. Time is
measured in units of Keplerian rotation at R=1. [video] (.avi, 6.6 MBt)
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| Quasi-periodic accretion and
outflows in propeller regime. Parameters: avis=0.3, adif=0.2.
Color background shows density, lines are magnetic field lines, Evolution is
shown for 1500 rotations. [video] (.avi, 50 MBt)
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Density distribution and streamlines of matter flow for T=924 rotations. Vectors are proportional to velocity. Parameters: avis=0.3, adif=0.2. [video] (.avi, 4.7 MBt)
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| Quasi-periodic accretion and outflows
in case of larger viscosity, (avis=0.6, adif=0.2).
Evolution is shown for time interval from 450 to 600 rotations. In this case the QPOs are
well-tuned. [video] (.avi, 4.8 MBt)
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| Quasi-periodic accretion and outflows
in case of larger viscosity, (avis=0.6, adif=0.2).
Evolution is shown for time interval from 500 to 700 rotations. In this case the QPOs are
well-tuned. [video] (.avi, 5.4 MBt) [return]
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