Results 101 to 110 of about 10,009 (174)
On the role of Alfvén waves as precursors of quasi-static acceleration processes in the Earth auroral zone [PDF]
Proceeding of the SF2A conference in Nice, 2012.In the Earth auroral zone, the electron acceleration by Alfvén waves is sometimes a precursor of the non-propagating acceleration structures.
Mottez, Fabrice
core +2 more sources
Resonant Absorption as Mode Conversion? II. Temporal Ray Bundle
A fast-wave pulse in a simple, cold, inhomogeneous MHD model plasma is constructed by Fourier superposition over frequency of harmonic waves that are singular at their respective Alfven resonances.
Chris S. Hanson +3 more
core +1 more source
How Alfvén waves energize the solar wind: heat vs work. [PDF]
Perez JC +4 more
europepmc +1 more source
MHD WAVES IN THE COLLISIONAL PLASMA OF THE SOLAR CORONA AND TERRESTRIAL IONOSPHERE
We have studied MHD waves (Alfvén and fast compressional modes) in a homogeneous collisional three-component low-β plasma. The three-component plasma consists of electrons, ions, and neutrals with arbitrary ratio between collision frequencies and wave ...
A.K. Nekrasov, V.A. Pilipenko
doaj +1 more source
We perform 1D linear analysis and numerical simulations of the propagation of Alfvén waves in a force-free magnetosphere along magnetic field lines around a spinning black hole.
Shinji Koide +2 more
doaj +1 more source
The electromagnetic interaction between Europa and the plasma sheet in the Jovian magnetosphere generates Alfvén waves, ultimately generating auroral footprints in Jupiter's atmosphere.
Shinnosuke Satoh +7 more
doaj +1 more source
How the plasma in the atmosphere is heated during a solar flare remains inconclusive. Nonthermal electron beams are usually considered as an essential heating source, yet Alfvén waves have also been proposed as a promising heating mechanism.
Jun Tian, Ying Li, Jie Hong, M. D. Ding
doaj +1 more source
How Alfvén waves induce compressive flows in the neighborhood of a 2.5D magnetic null-point. [PDF]
Sabri S, Farahani SV, Ebadi H, Poedts S.
europepmc +1 more source
Driven Phase-mixed Alfvén Waves in a Partially Ionized Solar Plasma
Phase mixing has long been understood to be a viable mechanism for expediting the dissipation of Alfvén wave energy resulting in the subsequent heating of the solar atmosphere.
M. McMurdo +3 more
doaj +1 more source
The problem of boundary conditions for monochromatic Alfvén waves, excited in the magnetosphere by external currents in the ionospheric E-layer, is solved analytically. Waves with large azimuthal wave numbers <i>m</i>»1 are considered. In our
A. S. Leonovich, V. A. Mazur
doaj

