Transient filaments formation by nonlinear kinetic Alfvén waves and its effect on solar wind turbulence and coronal heating

Details Transient filaments formation by nonlinear kinetic Alfvén waves and its effect on solar wind turbulence and coronal heating Transient filaments formation by nonlinear kinetic Alfvén waves and its effect on solar wind turbulence and coronal heating

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phpl....8.3759s&link_type=abstract

Physics of Plasmas, Volume 8, Issue 8, pp. 3759-3765 (2001).

Other

20

Magnetohydrodynamic Waves, Nonlinear Phenomena: Waves, Wave Propagation, And Other Interactions, Solar Wind Plasma, Sources Of Solar Wind, Magnetohydrodynamics And Plasmas, Particle Emission, Solar Wind

Scientific paper

The nonlinear dynamical equation for the propagation of kinetic Alfvén waves has been derived in two dimensions using the two-fluid model of the plasma and by taking the adiabatic response for the background density in the presence of nonlinear electron heating and the ponderomotive force. Dynamically evolving filamentary structures are predicted. The effect of these filaments on solar wind turbulence and coronal heating has also been pointed out.

Affiliated with

Also associated with

No associations

Rating

Transient filaments formation by nonlinear kinetic Alfvén waves and its effect on solar wind turbulence and coronal heating does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Transient filaments formation by nonlinear kinetic Alfvén waves and its effect on solar wind turbulence and coronal heating, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transient filaments formation by nonlinear kinetic Alfvén waves and its effect on solar wind turbulence and coronal heating will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-819348