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Self-Organization of Parallel Propagating Alfven Wave Turbulence

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Self-Organization of Parallel Propagating Alfven Wave Turbulence Proceedings of ISSS-7, 26-31, March, 2005 Self-organization of parallel propagating Alfven wave turbulence Yasuhiro NARIYUKI and Tohru HADA ESST ,Kyushu Univ, 6-1,Kasuga-Kouen, Kasuga City, Fukuoka 816-8580, Japan Nonlinear evolution of Alfven wave turbulence is discussed within the context of the derivative nonlinear Schroedinger equation (DNLS), a subset of the hall-MHD equation set, which includes quasi-parallel propagating right- and left-hand polarized Alfven wave modes. Via numerical time integration of the equation under periodic boundary conditions, we discuss self-organization of solitary waves, evolution of tri-coherence, synchronization of the wave phases, among others. Finite amplitude magnetohydrodynamics (MHD) waves k-space(Fig.2). Around t~300, a series of solitary waves are evolve nonlinearly via wave-particle and wave-wave born (Fig.1), corresponding to broading of the spectrum in interactions. Nonlinear evolution of the waves has been an Fig.2. These solitary waves repeatedly appear and vanish, while attracting subject for nonlinear wave research. Also, these interacting with each other. It is also noted that the almost all waves are considered as an essential ingredient for Fermi the solitary waves disappear at certain time intervals like t~900, acceleration of cosmic rays. Among various nonlinear which is indicative of the presence of (near) recursion of the processes triggered by the presence of the finite amplitude DNLS system with periodic boundary conditions. Alfven waves, we concentrate in this presentation on nonlinear The nonlinearity of the DNLS is cubic, i.e., the four wave evolution and self-organization of Alfven waves caused by resonance is the basic nonlinear interaction, self-coupling among Alfven waves which are parallel and uni-directional. By using this particularity, the hall-MHD k1=－k2+k3+k4 (2) equation set can be reduced using the method of averaging to yield the so-called DNLS equation, where similar relation is held for frequencies as well. Since it turned out that the power of the parent wave (k0=－11) remains 2 to be the most dominant one throughout the run, we evaluate ∂b ∂ 2 ∂ b (1) the tri-coherence among the wave modes with k3=k4=k0 above. + α ( b b ) + iµ 2 = 0 ∂t ∂x ∂x Then it is now clear that the modulational instability generates 2 two side band waves around the parent wave, since we can 1 C 1 b = b + ib α = A µ = ± write k1=k0-kd, k2=k0+kd, with arbitrary kd. Using these y z 4 C 2 - C 2 2 A s specifications of the wave numbers, we plot time evolution of sine of the relative phase among the four waves in Fig.3. As we will discuss in the presentation in detail, this parameter gives where b is the complex transverse magnetic field normalized to indication of energy (quanta) flow among the wave modes, the static field in the x direction, CA is the Alfven speed, Cs is which explains generation and decay of the solitary wave rows the sound speed, and time and space are normalized using the observed in the simulation. ion gyrofrequency and CA . The DNLS is integrable under In the presentation, we also discuss wave turbulence in the various boundary conditions. In the present study, we discuss driven-damped DNLS system. We show results of numerical nonlinear evolution of Alfven waves in (1), with particular runs with various parameters. attention to correlation of wave phases. In Fig.1 we show an example of time integration of (1), where |b| (envelope) is plotted in the phase space of time (t) and space (x). Evolution of the power spectrum of the same run is given in Fig.2, in which the vertical axis is the wave number k, with k positive (negative) corresponds to right- (left-) hand polarized waves. Initial conditions are given as a superposition of finite amplitude monochromatic waves (the parent) and a very small amplitude white noise. Boundary conditions are periodic. Until t~200, the parent wave energy is gradually transferred to daughter waves through modulational instability, which can be seen as a gradual spreading of the power spectrum in the Fig 1 Time evolution of envelope, |b|. Acknowledgments We thank S. Matsukiyo and D. Koga for useful discussions and comments. References Rogister, A. , Parallel propagation of nonlinear low-frequency waves in high-β plasma, Phys.Fluids, 14, 2733-2739, 1971. Mjolhus, E, J. , On the modulational instability of hydromagnetic waves parallel to the magnetic field, Plasma. Phys, 16, 321-334, 1974. Mio, K et al., Modified Nonlinear Schrodinger Equation for Alfven Waves Propagating along the Magnetic Field in Cold Plasma, J. Phys. Soc. Jpn, 41, 265-271, 1976. Mjolhus. E, and Hada. T, Nonlinear waves and chaos in space plasmas, edited by Hada.T and Matsumoto.H (Terrapub, Tokyo, p.121,1997. Kaup, D, J. , Newell, A, C. , An exact solution for a derivative Fig 2 Time evolution of power spectrum. nonlinear Schrodinger equation, J. Math. Phys, 19, 798-801,1978. Chen, X. , Lam, W, K. , Inverse scattaring transform for the derivative nonlinear Schrodinger equations with nonvanishing boundary conditions, Phys. Rev. E, 69, 066604, 2004. Hada,T., et al, Phase coherence of MHD waves in the solar wind, Space.Sci.Rev, 107, 463-466 ,2003. Sakai, j. , Sonneruo, B, J., Modulational instability of finite amplitude dispersive Alfven waves, J. Geophys. Res, 88, 9069-9078,1983. Machida, A. , et al , Simulation of amplitude-modulated circularly polarized Alfven waves for Beta less than 1 , J. Geophys. Res, 92, 7413-7422, 1987. Fig 3 Time evolution of sine of the relative phase(θk) among the four waves satisfying :k1+k2=2k0. Fig 4 Relation between the “flow of quana” among the resonant wave modes (horizontal axis) and the rate of which th erelative phase among the resonant wave modes varies (vertical axis). The flow of quanta among the sites is enhanced(suppressed) when the relative phase is almost constant (varies rapidly) in time. .
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