A concise review is given of astrophysically motivated experimental and theoretical research
on Taylor–Couette flow. The flows of interest rotate differentially with the inner cylinder faster …

Abstract Decades ago S. Lundquist, S. Chandrasekhar, PH Roberts and RJ Tayler first
posed questions about the stability of Taylor–Couette flows of conducting material under the …

This updated revision gives a complete and topical overview on Nonconservative Stability
which is essential for many areas of science and technology ranging from particles trapping …

Protoplanetary discs are made of gas and dust orbiting a young star. They are also the birth
place of planetary systems, which motivates a large amount of observational and theoretical …

We investigate sustenance and dependence on magnetic Prandtl number (Pm) for
magnetorotational instability (MRI)-driven turbulence in Keplerian disks with zero net …

Context. Surface magnetic fields have been detected in 5–10% of isolated massive stars,
hosting outer radiative envelopes. They are often thought to have a fossil origin, resulting …

Magnetic fields of planets, stars and galaxies are generated by self-excitation in moving
electrically conducting fluids. Once produced, magnetic fields can play an active role in …

We conduct a linear analysis of axisymmetric magnetorotational instability (MRI) in a
magnetized cylindrical Taylor-Couette (TC) flow for its standard version (SMRI) with a purely …

It has recently been shown that a significant slowdown of many stars can be attributed to the
emergence of a strong magnetic field within the radiative region, where heat is transferred …

The most ambitious project within the DREsden Sodium facility for DYNamo and
thermohydraulic studies (DRESDYN) at Helmholtz-Zentrum Dresden-Rossendorf (HZDR) is …