Перевод: с русского на английский

с английского на русский

hydrodynamics instability

См. также в других словарях:

  • Richtmyer-Meshkov instability — The Richtmyer Meshkov instability (RMI) occurs when an interface between fluids of differing density is impulsively accelerated, e.g. by the passage of a shock wave. The development of the instability begins with small amplitude perturbations… …   Wikipedia

  • гидродинамическая неустойчивость в ионосфере — Неустойчивость ионосферной плазмы, связанная с неравномерностью ее макроскопических параметров. [ГОСТ 25645.113 84] Тематики ионосфера земли Обобщающие термины волны и неустойчивости ионосферной плазмы EN hydrodynamics instability FR instabilite… …   Справочник технического переводчика

  • Fluid dynamics — Continuum mechanics …   Wikipedia

  • D'Alembert's paradox — In fluid dynamics, d Alembert s paradox (or the hydrodynamic paradox) is a contradiction reached in 1752 by French mathematician Jean le Rond d Alembert.[1] D Alembert proved that – for incompressible and inviscid potential flow – the drag force… …   Wikipedia

  • GERSHUNI — RUSSIA (see also List of Individuals) 15.2.1929 Yartsevo/RU 5.1.1999 Saint Petersburg/RU Grigory Zinovevich Gershuni was born in the Smolenskaya Oblast. During World War II, his family moved to the Perm Oblast, and it was there where he made… …   Hydraulicians in Europe 1800-2000

  • Magnetosphere of Jupiter — Discovery[1] Discovered by …   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

  • John Henry Michell — (26 October 1863 – 3 February 1940) was an Australian mathematician, Professor of Mathematics at the University of Melbourne.Early lifeMichell was the son of John Michell (pronounced Mitchell), a miner, and his wife Grace, née Rowse and was born… …   Wikipedia

  • Stellar evolution — Life cycle of a Sun like star Stellar evolution is the process by which a star undergoes a sequence of radical changes during its lifetime. Depending on the mass of the star, this lifetime ranges from only a few million years (for the most… …   Wikipedia

  • Vortex ring — A vortex ring, also called a toroidal vortex, is a region of rotating fluid moving through the same or different fluid where the flow pattern takes on a doughnut shape. The movement of the fluid is about the poloidal or circular axis of the… …   Wikipedia

  • Electrohydrodynamics — (EHD), also known as electro fluid dynamics (EFD) or electrokinetics, is the study of the dynamics of electrically conducting fluid. It is the study of the motions of ionised particles or molecules and their interactions with electric fields and… …   Wikipedia

Поделиться ссылкой на выделенное

Прямая ссылка:
Нажмите правой клавишей мыши и выберите «Копировать ссылку»