Transverse waves in a relativistic plasma.
Linearized equations describing transverse waves in relativistic plasma embedded in magnetic field and in presence of nonrelativistic plasma
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Linearized equations describing transverse waves in relativistic plasma embedded in magnetic field and in presence of nonrelativistic plasma
Transverse wave instabilities in collisionless hydrogen plasmas under magnetic field
Transverse electromagnetic wave propagation in cold plasma by external electric field oscillation
Transverse waves in a cylindrical chamber
Transverse waves instability in relativistic plasma, noting condition of isotropy and existence of electromagnetic waves
Interaction of longitudinal, surface, and transverse waves on plasma boundary
Transverse waves in a plasma in a magnetic field
Unstable transverse waves in anisotropic multicomponent plasma, establishing stability criteria, noting role of electron distribution
Transverse wave instability of unmagnetized collisionless plasma subjected to shear flow
Externally imposed oscillating electric field excites transverse electromagnetic waves propagating perpendicular to it in cold plasma
Pulsed laser double exposure holographic interferometry for measuring transverse wave propagation in beams
Double exposure pulsed laser holographic interferometry application to transverse wave propagation in Al plate
A method of making a composite panel having subsonic transverse wave speed characteristics which has first and second sheets sandwiching a core with at least one of the sheets being attached to the core at first regions thereof and unattached to the core at second regions thereof.
Investigation of the properties of low-frequency transverse waves in an expanding plasma. The wave vector, the background magnetic field, and the streaming velocity of the plasma are all assumed to lie along the radial direction. Expressions are presented for the radial dependence of the amplitude and phase of left and right circularly polarized waves, correct to first order in the wave frequency divided by the proton cyclotron frequency. Differences in the phase velocities of these two circular polarizations result in a Faraday rotation that can be substantial for typical interplanetary conditions near 1 AU. The implications of these results for a realistic solar wind model with the interplanetary magnetic field along the spiral direction are also considered.
We have investigated the Landau damping of transverse waves propagating in the thermal exospheric plasma, by fast particle fluxes which also exist in these regions. The most intense non-thermal fluxes so far detected are those of the auroral producing electrons and protons measured by McIlwain. We find that these fluxes may considerably damp the propagation of whistler modes through some regions. The damping of hydromagnetic waves in the exosphere by this mechanism is negligible.
Determination of the instability of a collisionless plasma in a uniform magnetic field with respect to transverse waves
The solution was obtained without approximating the dispersion relation. This was made possible by the use of a computer method for carrying out the extremely large number of algebraic manipulations involved. The three-fluid model employed accounts for the interaction of the electron, ion, and neutral species. The solution for the e-folding distance describes the damping characteristics of each wave mode. Each of the e-folding solutions corresponds to one of the phase velocity solutions.
Breakup of water jet by transverse shock wave