Results 71 to 80 of about 1,200 (139)
Geophysical Research LettersThe 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
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The Astrophysical JournalHow 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]
Sci Rep, 2020 Sabri S, Farahani SV, Ebadi H, Poedts S.
europepmc +1 more source
Driven Phase-mixed Alfvén Waves in a Partially Ionized Solar Plasma
The Astrophysical JournalPhase 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
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Annales GeophysicaeThe 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]
Sci Rep, 2019 Escande DF, Gondret V, Sattin F.
europepmc +1 more source
High-frequency torsional Alfvén waves as an energy source for coronal heating. [PDF]
Sci Rep, 2017 Srivastava AK +8 more
europepmc +1 more source
Alfvén waves as a solar-interplanetary driver of the thermospheric disturbances. [PDF]
Sci Rep, 2016 Guo J +7 more
europepmc +1 more source
Alfvén Waves in Partially Ionised Solar Steady-State Plasmas. [PDF]
Sol PhysAlshehri NF, Ballai I, Verth G, Fedun V.
europepmc +1 more source