Physics
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phpl...14j2304s&link_type=abstract
Physics of Plasmas, Volume 14, Issue 10, pp. 102304-102304-6 (2007).
Physics
8
Magnetohydrodynamic Waves, Solar Wind Plasma, Sources Of Solar Wind, Particle Acceleration, Corona
Scientific paper
This work presents the numerical simulations to study the filamentation of kinetic Alfvén waves in solar plasmas. Using the modified nonlinear Schrödinger equation model, we study the effect of changing the initial perturbation on filament formation and their nonlinear dynamics. The spectral indices of the power spectrum are calculated with different initial conditions of the simulations. The relevance of the present investigation in coronal heating and solar wind acceleration/turbulence is also pointed out.
Sharma R. P.
Singh Heisnam Dinachandra
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