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Alfven waves as a driving mechanism in stellar winds
(ELSEVIER SCI LTD, 2010)
Alfven waves have been invoked as an important mechanism of particle acceleration in stellar winds of cool stars. After their identification in the solar wind they started to be studied in winds of stars located in different ...
Kinetic ion effect on geodesic acoustic Alfven modes in tokamaks
(AMER INST PHYSICS, 2009)
Using a quasitoroidal set of coordinates with coaxial circular magnetic surfaces, the Vlasov equation is solved for collisionless plasmas, and the dielectric tensor is found for large aspect ratio tokamaks in a low frequency ...
Chaos and Intermittency in the DNLS Equation Describing the Parallel Alfvén Wave Propagation
(Hindawi Publishing Corporation, 2014-04)
When the Hall effect is included in the magnetohydrodynamics equations (Hall-MHD model) the wave propagation modes become coupled, but for propagation parallel to the ambient magnetic field the Alfvén mode decouples from ...
Wolf-Rayet optically thick winds with Alfven waves
(ELSEVIER SCI LTD, 2010)
The Wolf-Rayet (WR) stars are hot luminous objects which are suffering an extreme mass loss via a continuous stellar wind. The high values of mass loss rates and high terminal velocities of the WR stellar winds constitute ...
CORONAL LOOP HEATING BY DISCRETE ALFVEN WAVES
(Kluwer Academic PublDordrechtHolanda, 1991)
Interplay between Alfvén and magnetosonic waves in compressible magnetohydrodynamics turbulence
(American Institute of Physics, 2017-10)
Using spatio-temporal spectra, we show direct evidence of excitation of magnetosonic and Alfvén waves in three-dimensional compressible magnetohydrodynamic turbulence at small Mach numbers. For the plasma pressure dominated ...