Results 321 to 330 of about 258,872 (345)
Some of the next articles are maybe not open access.

Modelling of MHD Turbulence

2007
SCOPUS: ar.k ; info:eu-repo/semantics ...
Knaepen, Bernard   +2 more
openaire   +2 more sources

Investigation on TiO2–Cu/H2O hybrid nanofluid with slip conditions in MHD peristaltic flow of Jeffrey material

Journal of Thermal Analysis and Calorimetry, 2020
Aamir Ali   +5 more
semanticscholar   +1 more source

Numerical and analytical solutions for Falkner-Skan flow of MHD Oldroyd-B fluid

, 2014
Purpose – In this paper, analysis is presented to investigate the Falkner-Skan flow of magnetohydrodynamic (MHD) Oldroyd-B fluid. The paper aims to discuss these issues.
S. Abbasbandy   +3 more
semanticscholar   +1 more source

MHD linear generator modelling

IEEE Transactions on Appiled Superconductivity, 1995
The performance of typical magnetohydrodynamic (MHD) linear generators are evaluated as function of the excitation magnetic field profile. Using a three dimensional (3D) lumped parameter model, able to simulate all major physical MHD energy conversion phenomena, a parametric analysis has been pointed out for various saddle shaped superconducting (SC ...
GERI, Alberto   +2 more
openaire   +4 more sources

MHD spectroscopy

2004
Experiments are conducted on the JET tokamak to demonstrate the diagnostic potential of Magneto-Hydro-Dynamics (MHD) spectroscopy, for the plasma bulk and its suprathennal components, using Alfven eigenmodes (AEs) excited by external antennas and by energetic particles.
Heeter, R. F.   +7 more
openaire   +1 more source

Practice with MHD

1987
The subject of magnetohydrodynamics (MHD) is important for astrophysics because magnetic fields pervade cosmic phenomena. The mathematical solution to most MHD problems is complicated, even for modern computers. Therefore, a lore of physical intuition has evolved which permits ‘solution’ of MHD problems by ‘hand-waving’ arguments based on a few simple ...
openaire   +2 more sources

SLAU2-MHD for Low Mach Magnetohydrodynamics (MHD) Simulations [PDF]

open access: possibleAIAA AVIATION 2021 FORUM, 2021
Takashi Minoshima   +2 more
openaire   +1 more source

MHD and the Solar Dynamo

2007
In this chapter we will explain the basic MHD equations which are needed to understand solar active phenomena such as spots, prominences, flares etc.
openaire   +2 more sources

MHD stagnation point flow of viscoelastic nanofluid with non-linear radiation effects

, 2016
M. Farooq   +5 more
semanticscholar   +1 more source

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