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Numerical and analytical solutions for Falkner-Skan flow of MHD Oldroyd-B fluid
, 2014Purpose – 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, 1995The 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
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
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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
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 ...
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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]
Takashi Minoshima+2 more
openaire +1 more source
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.
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In this chapter we will explain the basic MHD equations which are needed to understand solar active phenomena such as spots, prominences, flares etc.
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MHD stagnation point flow of viscoelastic nanofluid with non-linear radiation effects
, 2016M. Farooq+5 more
semanticscholar +1 more source