- MHD stability
- Макаров: (magnetohydrodynamic stability) магнитогидродинамическая устойчивость
Универсальный англо-русский словарь. Академик.ру. 2011.
MHD stability
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Plasma stability — An important field of plasma physics is the stability of the plasma. It usually only makes sense to analyze the stability of a plasma once it has been established that the plasma is in equilibrium. Equilibrium asks whether there are net forces… … Wikipedia
Electrothermal instability — NOTOC The electrothermal instability (also known as the ionization instability or Velikhov instability in the literature) is a magnetohydrodynamic (MHD) instability appearing in magnetized non thermal plasmas used in MHD converters. It was first… … Wikipedia
Pinch (plasma physics) — For other uses, see Pinch (disambiguation). Lightning bolts illustrating electromagnetically pinched plasma filaments … Wikipedia
Magnetohydrodynamics — For the academic journal, see Magnetohydrodynamics (journal). Magnetohydrodynamics (MHD) (magneto fluid dynamics or hydromagnetics) is an academic discipline which studies the dynamics of electrically conducting fluids. Examples of such fluids… … Wikipedia
Fusion power — The Sun is a natural fusion reactor. Fusion power is the power generated by nuclear fusion processes. In fusion reactions two light atomic nuclei fuse together to form a heavier nucleus (in contrast with fission power). In doing so they release a … Wikipedia
Shocks and discontinuities (magnetohydrodynamics) — Shocks and discontinuities are transition layers where the plasma properties change from one equilibrium state to another. The relation between the plasma properties on both sides of a shock or a discontinuity can be obtained from the… … Wikipedia
Rayleigh–Taylor instability — The Rayleigh–Taylor instability, or RT instability (after Lord Rayleigh and G. I. Taylor), is an instability of an interface between two fluids of different densities, which occurs when the lighter fluid is pushing the heavier fluid. [citation… … Wikipedia
Magnetorotational instability — The magnetorotational instability or MRI is a fluid instability that arises when the angular velocity of a magnetized fluid decreases as the distance from the rotation center increases. It can also be known as the Velikhov Chandrasekhar… … Wikipedia
Balbus-Hawley-Instabilität — Kleine Magnetfelder sorgen in rotierenden Fluiden unter bestimmten Voraussetzungen dafür, dass die Rotation instabil wird und Materie ins Zentrum fällt. Dieses Phänomen wird als Magnetorotationsinstabilität (MRI, magnetische… … Deutsch Wikipedia
Magnetorotationsinstabilität — Kleine Magnetfelder sorgen in rotierenden Fluiden unter bestimmten Voraussetzungen dafür, dass die Rotation instabil wird und Materie ins Zentrum fällt. Dieses Phänomen wird als Magnetorotationsinstabilität (MRI, magnetische… … Deutsch Wikipedia
Corona — This article is about the astronomical term. For other uses, see Corona (disambiguation). During a total solar eclipse, the solar corona can be seen with the naked eye. A corona is a type of plasma atmosphere of the Sun or other celestial body,… … Wikipedia
