Stochastic electron heating and hydromagnetic wave damping.
Collisionless damping of fast hydromagnetic waves by stochastic electron heating, discussing method for obtaining damping decrements
SEARCH · Search NASA
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Collisionless damping of fast hydromagnetic waves by stochastic electron heating, discussing method for obtaining damping decrements
Hydromagnetic disturbances on magnetopause from IMP 2 satellite data noting relation to energetic electron bow shock spikes
Criticism of work by Lerche regarding hydromagnetic analysis of Kelvin-Helmholtz configuration at boundary between solar wind and magnetosphere
Hydromagnetic surface waves propagating on finitely conducting fluid using alternating magnetic field, including electromagnetic skin depth effects in computing theoretical wave dispersion
Hydromagnetic tangential discontinuities in solar wind from Pioneer 6
Adiabatic motion of hydromagnetic fluid behind spherical fast shock wave for Parker solar wind model
Quasi-linear theory of hydromagnetic waves in nonrelativistic collisionless plasma, noting resonant diffusion effect on plasma heating mode
Hydromagnetic wave-charged particle resonant interaction described by diffusion equation in momentum space, deriving diffusion coefficients and time evolution ultrarelativistic particle energy spectrum
Hydromagnetic waves equations of motion for nonrelativistic case, discussing particle and fluid flow models
Hydromagnetic radiation characteristics of electric and magnetic dipoles in homogeneous anisotropic cold plasma, obtaining field components and wave propagation modes
Reverse hydromagnetic shock in solar wind
Hydromagnetic forces effects on tidal period hydrodynamic waves, explaining ionospheric tidal motion behavior
Hydromagnetic wave interaction with magnetopause and bow shock, considering solar wind turbulence and magnetopause tail stability
Hydromagnetic self gravitating galactic slab embedded in halo, deriving stability criteria using models of magnetic field
Hydromagnetic fluid model of solar wind for interpreting discontinuities in plasma and magnetic field, interaction with atmosphere, heating mechanism and chemical composition
Bow shock associated hydromagnetic waves generation in upstream interplanetary medium, constructing model in terms of ion cyclotron resonance
Hydromagnetic shock waves structure, investigating resistive, viscous and thermal conduction dissipation effects on discontinuities
Current sheet structure of hydromagnetic boundary layer formed by mixing two conducting fluid streams containing oppositely directed magnetic fields