
IOSR Journal of Mathematics (IOSR-JM)
... of Laplace transform. More to this, Ram et al (1984) have analyzed Hall effects on heat and mass transfer flow through porous media. Soundelgekar and Abdulla Ali (1986) studied the flow of viscous incompressible electrically conducting fluid past an impulsively started infinite vertical isothermal p ...
... of Laplace transform. More to this, Ram et al (1984) have analyzed Hall effects on heat and mass transfer flow through porous media. Soundelgekar and Abdulla Ali (1986) studied the flow of viscous incompressible electrically conducting fluid past an impulsively started infinite vertical isothermal p ...
6. Solar wind acceleration
... Color contours show the velocity-space density, normalized in each panel to the maximum value at the origin. At left is the initial, isotropic distribution. Adjacent panels show the time development for three later times, where τ is proportional to the normalized wave intensity. ...
... Color contours show the velocity-space density, normalized in each panel to the maximum value at the origin. At left is the initial, isotropic distribution. Adjacent panels show the time development for three later times, where τ is proportional to the normalized wave intensity. ...
study of planetary magnetic fields
... of 24 hours generates enough movement of the liquid to stimulate a magnetic field. The other planets in our solar system, except for Venus and Mars, all have magnetic fields or traces of magnetism that differ from Earth’s in various ways. Mars: Mars does not have a conventional magnetic field--one t ...
... of 24 hours generates enough movement of the liquid to stimulate a magnetic field. The other planets in our solar system, except for Venus and Mars, all have magnetic fields or traces of magnetism that differ from Earth’s in various ways. Mars: Mars does not have a conventional magnetic field--one t ...
M.Sc._Physics_sem_IV.pdf
... Radiations by moving charges: LienardWeinchert potentials and field for a point charge, total power radiated by an accelerated charge (Larmor’s Formula and its relativistic generalization). Angular distribution and frequency spectrum of the radiation power.Covariant formulation of electromagnetic th ...
... Radiations by moving charges: LienardWeinchert potentials and field for a point charge, total power radiated by an accelerated charge (Larmor’s Formula and its relativistic generalization). Angular distribution and frequency spectrum of the radiation power.Covariant formulation of electromagnetic th ...
THE MEAN ELECTROMOTIVE FORCE FOR MHD TURBULENCE
... 1979; Krause and Rädler, 1980; Zeldovich et al., 1983). The crucial point of this approach is the mean electromotive force which is determined by the fluctuations of the fluid velocity and the magnetic field. It describes several physical effects like -effect, turbulent diffusion of the magnetic f ...
... 1979; Krause and Rädler, 1980; Zeldovich et al., 1983). The crucial point of this approach is the mean electromotive force which is determined by the fluctuations of the fluid velocity and the magnetic field. It describes several physical effects like -effect, turbulent diffusion of the magnetic f ...
Lecture 4: Molecular Clouds (1)
... Both HI and diffuse clouds can persist for long periods by means of pressure balance, because of the presence of a surrounding, more rarefied and warmer medium which prevents the internal (thermal) motion from dispersing the cloud. In giant molecular clouds, the main cohesive force is typically the ...
... Both HI and diffuse clouds can persist for long periods by means of pressure balance, because of the presence of a surrounding, more rarefied and warmer medium which prevents the internal (thermal) motion from dispersing the cloud. In giant molecular clouds, the main cohesive force is typically the ...