Results 121 to 130 of about 9,578 (225)
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
Damping of high frequency waves in the solar wind [PDF]
Cyclotron damping by suprathermal fluxes of protons and electrons in the interplanetary medium will greatly attenuate high frequency Alfven waves and whistler waves within distances 1 AU of the sun.
Fisk, L. A., Goldstein, M. L.
core +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
Relevant heating of the quiet solar corona by Alfvén waves: a result of adiabaticity breakdown. [PDF]
Escande DF, Gondret V, Sattin F.
europepmc +1 more source
High-frequency torsional Alfvén waves as an energy source for coronal heating. [PDF]
Srivastava AK +8 more
europepmc +1 more source
Alfvén waves as a solar-interplanetary driver of the thermospheric disturbances. [PDF]
Guo J +7 more
europepmc +1 more source

