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  5. THE TRANSPORT OF LOW-FREQUENCY TURBULENCE IN ASTROPHYSICAL FLOWS

THE TRANSPORT OF LOW-FREQUENCY TURBULENCE IN ASTROPHYSICAL FLOWS

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：liutongyang123
【摘 要】
：
Zank et al.2012 developed a turbulence transport model for low-frequency incompressible magnetohydrodynamic(MHD) turbulence in inhomogeneous flows in terms of the energy corresponding to the forward a
【作 者】
：
L.Adhikari G.P.Zank R.Bruno D.Telloni P.Hunana A.Dosch R.Marino Q.Hu 
【机 构】
：
Center for Space Plasma and Aeronomic Research(CSPAR),University of Alabama in Huntsville,Huntsville
【出 处】
：
The Fourteenth International Solar Wind Conference (第十四届国际太阳
【发表日期】
：
2015年5期
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Zank et al.2012 developed a turbulence transport model for low-frequency incompressible magnetohydrodynamic(MHD) turbulence in inhomogeneous flows in terms of the energy corresponding to the forward and backward propagating modes,the residual energy,the correlation lengths corresponding to the forward and backward propagating modes,and the correlation length of the residual energy.
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