On the Nature of the Inhomogenous Structure of Interplanetary Plasma
Inhomogenous structure of interplanetary plasma
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Inhomogenous structure of interplanetary plasma
Harrison baryon inhomogeneity postulate of galactic evolution critically analyzed for universality of cosmic rays
Holographic method for measurements of ray deviations in optically inhomogeneous field
Radiation from vertical electric dipole in inhomogeneous half space, discussing far field energy propagation
Statistical effects of inhomogeneities in universe on light propagation, noting low intergalactic medium density effect at all red shifts
Matter excess over antimatter in early high density high temperature universe, discussing baryon inhomogeneity
Supraluminous longitudinal plasma wave scattering by localized inhomogeneity in thermal plasma density, calculating far field electromagnetic radiation production
Winds and inhomogeneous atmosphere effects on sonic boom strength and propagation, using model based on shock wave/vortex sheet interaction concept
Kinetic equation for inhomogeneous fully ionized plasma in quasi-equilibrium in magnetic field
Input admittance of waveguide-fed rectangular aperture under flowing and stationary inhomogeneous plasmas, noting dependence on various plasma properties
Admittance of inhomogeneously sheathed infinite cylindrical antenna immersed in istropic compressible plasma
Anisotropic solar cosmic ray propagation in inhomogeneous medium
Statistical theory of inhomogeneous gas
Propagation in planar inhomogeneous plasma medium
Radiative transfer equation solution for spectral line formed in two dimensionally varying atmosphere extended to continuum radiation in inhomogeneous atmospheres
Dynamical model for spherical inhomogeneity in mean mass density of universe to predict velocity dispersion observed for Coma Cluster
Normal mode representation of HF properties of inhomogeneous plasma, analyzing Vlasov equation for free oscillations under external driving field
Coupled kinetic equations for inhomogeneous systems treated as simultaneous equations in time, obtaining solutions by successive approximation