Nonlinear interaction of MHD waves and solar corona heating

Details Nonlinear interaction of MHD waves and solar corona heating Nonlinear interaction of MHD waves and solar corona heating

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..477y&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 477-480

Physics

Scientific paper

The nonlinear parametric interaction of Alfvén waves with magnetosonic and ion-acoustic waves is considered on the basis of two-fluid magnetohydrodynamics. A nonlinear dispersion relation describing three-wave interaction, instability growth rate have been calculated and estimated. The analysis of theoretical results shows that kinetic effects in the Alfvén waves (the finite ion Larmour radius) are essential for the parametric interactions of waves. Nonlinear parametric processes studied in the paper could take place in the solar coronal loops, where plasma parameter is small. The products of the decay - magnetosonic and ion-acoustic waves, can effectively heat the coronal plasma owing to rapid dissipation.

Affiliated with

Also associated with

No associations

Rating

Nonlinear interaction of MHD waves and solar corona 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 Nonlinear interaction of MHD waves and solar corona heating, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear interaction of MHD waves and solar corona heating will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1386921