Damping of Torsional Modes in the Solar Corona

Details Damping of Torsional Modes in the Solar Corona Damping of Torsional Modes in the Solar Corona

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..895..147c&link_type=abstract

FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP Conference Proceedings, Volume 895, pp. 147-152 (2007).

Astronomy and Astrophysics

Astrophysics

Corona, Mhd Waves, Plasma Waves, Turbulence, Magnetohydrodynamics And Plasmas

Scientific paper

The Alfvén wave is one of the classic waves in magnetoplasma. It is an electromagnetic-hydrodynamic wave, in which the restoring force comes from the magnetic tension, while the ions provide the inertia. We have studied the propagation and dissipation of torsional Alfvén waves in an inhomogeneous cylindrical plasma taking into account the effects due to finite Larmor gyroradius.

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