Magnetically-driven jets and winds from weakly magnetized accretion disks

14 Oct 2019 Jacquemin-Ide J. Ferreira J. Lesur G.

Semi-analytical models of disk outflows have successfully described magnetically-driven, self-confined super-Alfv\'enic jets from near Keplerian accretion disks. These Jet Emitting Disks are possible for high levels of disk magnetization $\mu$ defined as $\mu=2/\beta$ where beta is the usual plasma parameter... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • SOLAR AND STELLAR ASTROPHYSICS