Cosmic magnetic fields are produced, on a wide range of spatial scales, by the homogeneous dynamo effect in electrically conducting fluids [1]. The Earth’s magnetic field is generated in its outer core, most likely by spiral flow structures which result from the combined action of Coriolis forces and thermal and/or compositional buoyancy [2]. The magnetic field of the Sun is generated in the convection zone and in the tachocline, very likely under the influence of differential rotation and helical turbulence [3]. A similar mechanism is probably at the root of large scale galactic magnetic fields [4], while inter-galactic magnetic fields are thought to be a product of the so-called fluctuation dynamo [5].
Magnetic fields play an active role in cosmic structure formation. It was in 1991 that Balbus and Hawley [6] highlighted the importance of the magnetorotational instability (MRI, or Velikhov-Chandrasekhar instability [7, 8]) for the angular momentum transport in accretion disks around stars and black holes. In MRI, the externally applied magnetic field serves only as a trigger for the instability that actually taps into the rotational energy of the flow. This is quite in contrast to another magnetic instability in which prevailing currents in the fluid can become unstable by themselves. This latter, so-called Tayler instability [9] is held responsible for parts of the dynamo mechanism in stars [10], and for some observed helical structures in jets and outflows [11].
3D MHD Simulations of Instabilities
Wang & Robertson 1985, Rastätter & Schindler 1999, … Nonlinear development of the magnetic Rayleigh-Taylor instability
(Stone & Gardiner 2007)

An argon plasma jet forms a rapidly growing corkscrew, known as a kink instability. This instability causes an even faster-developing behavior called a Rayleigh-Taylor instability, in which ripples grow and tear the jet apart. This phenomenon, the Caltech researchers say, has never been seen before and could be important in understanding solar flares and in developing nuclear fusion as a future energy source. Watch the plasma in action here.
[Credit: A. L. Moser and P. M. Bellan, Caltech ]
So then nuclear fusion is taking place on the surface of the Sun? Where have we heard that before?An argon plasma jet forms a rapidly growing corkscrew, known as a kink instability. This instability causes an even faster-developing behavior called a Rayleigh-Taylor instability, in which ripples grow and tear the jet apart. This phenomenon, the Caltech researchers say, has never been seen before and could be important in understanding solar flares and in developing nuclear fusion as a future energy source. Watch the plasma in action here.
[Credit: A. L. Moser and P. M. Bellan, Caltech ]

... rotating black hole by astronomers -quantaverse

The falling magnetic field generates a huge electrical field which shoots two high-energy beams out of the plasmoid, the electrons one way, the protons in the opposite direction. The beam consists of many dense helical filaments (one micron across). Some ions are heated to such high temperatures that they fuse.
There are two types of kinetic Alfv ́en waves. For relatively large beta (β > me/mi), e.g., at the magnetospheric boundary, the mode is called the oblique kinetic Alfv ́en wave with the phase velocity
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