Results 11 to 20 of about 128,351 (288)

MHD. ENTVESTENEN VERLOBEN. [PDF]

open access: greenBeiträge zur Geschichte der deutschen Sprache und Literatur (PBB), 1918
n ...
O. BEHAGHEL
openalex   +4 more sources

BEITRÄGE ZUM MHD. WORTSCHATZ. [PDF]

open access: greenBeiträge zur Geschichte der deutschen Sprache und Literatur (PBB), 1899
n ...
G. EHRISMANN
openalex   +5 more sources

Simulating solar MHD [PDF]

open access: yesAnnales Geophysicae, 1999
Abstract. Two aspects of solar MHD are discussed in relation to the work of the MHD simulation group at KIS. Photospheric magneto-convection, the nonlinear interaction of magnetic field and convection in a strongly stratified, radiating fluid, is a key process of general astrophysical relevance.
M. Schüssler, M. Schüssler
openaire   +7 more sources

The tamed MHD equations [PDF]

open access: yesJournal of Evolution Equations, 2020
AbstractWe study a regularised version of the magnetohydrodynamics (MHD) equations, the tamed MHD (TMHD) equations. They are a model for the flow of electrically conducting fluids through porous media. We prove existence and uniqueness of TMHD on the whole space $${\mathbb {R}}^{3}$$ R
openaire   +3 more sources

Anisotropic MHD turbulence [PDF]

open access: yesAIP Conference Proceedings, 2007
The solar wind and the interstellar medium are permeated by large-scale magnetic fields that render magnetohydrodynamic (MHD) turbulence anisotropic. In the weak-turbulence limit in which three-wave interactions dominate, analytical and high-resolution numerical results based on random scattering of shear-Alfv n waves propagating parallel to a large ...
C. S. Ng, Amitava Bhattacharjee
openaire   +3 more sources

MHD. POYTWIN. [PDF]

open access: yesBeiträge zur Geschichte der deutschen Sprache und Literatur (PBB), 1909
n ...
openaire   +2 more sources

On wave turbulence in MHD [PDF]

open access: yesNonlinear Processes in Geophysics, 2001
Abstract. We describe the fundamental differences between weak (wave) turbulence in incompressible and weakly compressible MHD at the level of three-wave interactions. The main difference is in the structure of the resonant manifolds and the mechanisms of redistribution of spectral densities along the applied magnetic field B0.
Sébastien Galtier   +3 more
openaire   +5 more sources

MHD Boundary Layers Theory in Sobolev Spaces Without Monotonicity I: Well‐Posedness Theory [PDF]

open access: yesCommunications on Pure and Applied Mathematics, 2016
We study the well‐posedness theory for the MHD boundary layer. The boundary layer equations are governed by the Prandtl‐type equations that are derived from the incompressible MHD system with non‐slip boundary condition on the velocity and perfectly ...
Cheng-Jie Liu, Feng Xie, Tong Yang
semanticscholar   +1 more source

Causal and pathogenetic therapy of pain in oropharynx

open access: yesМедицинский совет, 2015
Sore throat is one of the most common complaint with which patients seek the aid of doctors specializing in different areas. Sore throat may be associated with abnormalities of various organs and systems due to topographical proximity of various ...
A. I. Кryukov   +4 more
doaj   +1 more source

MHD Instabilities in Tokamaks [PDF]

open access: yesFusion Science and Technology, 2006
A general introduction to ideal magnetohydrodynamic (MHD) stability of tokamak plasmas is given, using linear perturbations of the ideal MHD equations.
openaire   +3 more sources

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