Nonlinear development of Langmuir turbulence in inhomogeneous solar coronal plasma

Details Nonlinear development of Langmuir turbulence in inhomogeneous solar coronal plasma Nonlinear development of Langmuir turbulence in inhomogeneous solar coronal plasma

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..315k&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Corona: Langmuir Wave Turbulence

Scientific paper

The Langmuir wave turbulence is a key issue in the theory of solar plasma emission. The self-consistent description of Langmuir wave and ion-sound wave turbulence in the presence of an electron beam is presented for inhomogeneous non-isothermal plasma. The results show that the presence of inhomogeneity significantly changes the overall evolution in the system. The inhomogeneity is very effective in shifting the wave numbers of the Langmuir waves, and thus can switch between different nonlinear processes.

Affiliated with

Also associated with

No associations

Rating

Nonlinear development of Langmuir turbulence in inhomogeneous solar coronal plasma 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 development of Langmuir turbulence in inhomogeneous solar coronal plasma, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear development of Langmuir turbulence in inhomogeneous solar coronal plasma will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-963778