Results 81 to 90 of about 1,162 (146)
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
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
Alfvén Waves in Partially Ionised Solar Steady-State Plasmas. [PDF]
Alshehri NF, Ballai I, Verth G, Fedun V.
europepmc +1 more source
Riemann solvers and Alfven waves in black hole magnetospheres. [PDF]
Punsly B, Balsara D, Kim J, Garain S.
europepmc +1 more source
Evidence for Alfvén waves powering auroral arc via a static electric potential drop. [PDF]
Tian S +10 more
europepmc +1 more source
Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]
Morton RJ +5 more
europepmc +1 more source

