Modelling Fast-Alfvén Mode Conversion Using SPARC
作者: H MoradiP S Cally
作者单位: 1Monash Centre for Astrophysics, School of Mathematical Sciences, Monash University, Victoria 3800, Australia
刊名: Journal of Physics: Conference Series, 2013, Vol.440 (1)
来源数据库: Institute of Physics Journal
DOI: 10.1088/1742-6596/440/1/012047
原始语种摘要: We successfully utilise the SPARC code to model fast-Alfvén mode conversion in the region cA >> cs via 3-D MHD numerical simulations of helioseismic waves within constant inclined magnetic field configurations. This was achieved only after empirically modifying the background density and gravitational stratifications in the upper layers of our computational box, as opposed to imposing a traditional Lorentz Force limiter, to ensure a manageable timestep. We found that the latter approach inhibits the fast-Alfvén mode conversion process by severely damping the magnetic flux above the surface.
全文获取路径: IOP 

  • successfully 成功地
  • ensure 担保
  • process 过程
  • SPARC Scalable Processor ARChitecture
  • limiter 限幅器
  • Force 
  • above 在上面
  • approach 
  • computational 计算的
  • Conversion 变换