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MHD SIMULATIONS OF DISK - MAGNETIZED STAR INTERACTIONS IN QUIESCENT REGIME: FUNNEL FLOWS AND ANGULAR MOMENTUM TRANSPORT 2D MHD (axisymmetric) numerical simulations of disk accretion to a star with a dipole magnetic field
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MHD SIMULATIONS OF DISK - MAGNETIZED STAR INTERACTIONS IN QUIESCENT REGIME: FUNNEL FLOWS AND ANGULAR MOMENTUM TRANSPORT 2D MHD (axisymmetric) numerical simulations of disk accretion to a star with a dipole magnetic field
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| Disk
accretion to a slowly rotating star (r_cor = 3). Viscosity parameter
a =
0.02. Initially, inner radius of the disk located at the magnetosphere
radius, r_m = 1. [video] (.avi, approx. 1.7 MBt)
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| Disk
accretion to a slowly rotating star (r_cor = 3). Viscosity parameter
a =
0.02. Initially, inner radius of the disk is at co-rotation radius,
r_cor = 3. [video] (.avi, approx. 1.9 MBt)
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| Disk
accretion to a slowly rotating star (r_cor = 3). Viscosity parameter
a =0.
Initially, inner radius of the disk is at co-rotation radius, r_co r=
3. [video] (.avi, approx. 1.1 MBt)
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| Disk
accretion to a slowly rotating star (r_cor = 3). Viscosity parameter
a =0.
Initially, inner radius of the disk is at co-rotation radius, r_co r=
3. Smaller
region is shown. [video] (.avi, approx. 1.3 MBt)
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| Torqueless
accretion which is realized at co-rotation radius r_cor = 1.5 (see Paper).
Viscosity parameter is
a
=0.02. Initially, inner radius of the disk located at the magnetosphere radius, r_m = 1. [video] (.avi, approx. 1.5 MBt)
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