Simulations of nonlinear field line resonances

  • Kim, Kyung-Im (Dept. of Astronomy and Space Science, Kyung Hee University) ;
  • Lee, Dong-Hun (Dept. of Astronomy and Space Science, Kyung Hee University) ;
  • Kim, Jong-Soo (Dept. of Astronomy and Space Science, Kyung Hee University)
  • 발행 : 2008.10.22

초록

In this study, the nature of nonlinear field line resonances (FLR) is studied by adopting full MHD simulations. The MHD code used here is based on the total variation diminishing (TVD) scheme and we have performed numerical simulations of FLR with its three-dimensional code. If the source perturbation is strongly impulsive and thus the timescale of the initial variations is sufficiently smaller than the convection timescale, FLRs are easily confirmed in these simulations. When the disturbance is sufficiently small, it is shown that linear properties of MHD wave coupling are well reproduced. In order to examine nonlinear nature of FLR, wave spectra, Poynting flux and energy distribution are studied at resonances as the magnitude of initial disturbance gradually increases.

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