MHD Simulations of Magnetospheric Accretion, Ejection and Plasma-field Interaction
arXiv:1311.4597 · doi:10.1051/epjconf/20136405001
Abstract
We review recent axisymmetric and three-dimensional (3D) magnetohydrodynamic (MHD) numerical simulations of magnetospheric accretion, plasma-field interaction and outflows from the disk-magnetosphere boundary.
11 pages, 8 figures, conference proceedings: "Physics at the Magnetospheric Boundary", Geneva, Switzerland, 25-28 June, 2013
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Cited by in corpus (8)
- CSI 2264: Probing the inner disks of AA Tau-like systems in NGC 2264
- Physics in Very Strong Magnetic Fields: Introduction and Overview
- The magnetospheric radius of an inclined rotator in the magnetically threaded disk model
- Trapping of Low-Mass Planets Outside the Truncated Inner Edges of Protoplanetary Discs
- On the area of accretion curtains from fast aperiodic time variability of the intermediate polar EX Hya
- Swift J1734.5-3027: a new long type-I X-ray bursting source
- Observing Rayleigh-Taylor stable and unstable accretion through a Kalman filter analysis of X-ray pulsars in the Small Magellanic Cloud
- Measuring the magnetic dipole moment and magnetospheric fluctuations of accretion-powered pulsars in the Small Magellanic Cloud with an unscented Kalman filter