Effects of wave damping and finite perpendicular scale on three-dimensional Alfven wave parametric decay in low-beta plasmas (2403.08179v2)
Abstract: Shear Alfven wave parametric decay instability (PDI) provides a potential path toward significant wave dissipation and plasma heating. However, fundamental questions regarding how PDI is excited in a realistic three-dimensional (3D) open system and how critically the finite perpendicular wave scale--as found in both laboratory and space plasmas--affects the excitation remain poorly understood. Here, we present the first 3D, open-boundary, hybrid kinetic-fluid simulations of kinetic Alfven wave PDI in low-beta plasmas. Key findings are that the PDI excitation is strongly limited by the wave damping present, including electron-ion collisional damping (represented by a constant resistivity) and geometrical attenuation associated with the finite-scale Alfven wave, and ion Landau damping of the child acoustic wave. The perpendicular wave scale alone, however, plays no discernible role: waves of different perpendicular scales exhibit similar instability growth as long as the magnitude of the parallel ponderomotive force remains unchanged. These findings are corroborated by theoretical analysis and estimates. The new understanding of 3D kinetic Alfv\'en wave PDI physics is essential for laboratory study of the basic plasma process and may also help evaluate the relevance/role of PDI in low-beta space plasmas.
- L. Chen and F. Zonca, Reviews of Modern Physics 88, 015008 (2016).
- L. Del Zanna and M. Velli, Advances in Space Research 30, 471 (2002).
- B. Inhester, Journal of Geophysical Research: Space Physics 95, 10525 (1990).
- P. H. Yoon and T.-M. Fang, Plasma Physics and Controlled Fusion 50, 085007 (2008).
- R. Z. Sagdeev and A. A. Galeev, Nonlinear Plasma Theory (1969).
- N. Derby Jr, The Astrophysical Journal 224, 1013 (1978).
- M. L. Goldstein, The Astrophysical Journal 219, 700 (1978).
- A. Hasegawa and L. Chen, Physical Review Letters 36, 1362 (1976).
- H. Wong and M. Goldstein, Journal of Geophysical Research: Space Physics 91, 5617 (1986).
- M. Longtin and B. Ö. Sonnerup, Journal of Geophysical Research: Space Physics 91, 6816 (1986).
- J. V. Hollweg, Journal of Geophysical Research: Space Physics 99, 23431 (1994).
- B. D. Chandran, Journal of plasma physics 84 (2018).
- K. H. Kiyani, K. T. Osman, and S. C. Chapman, “Dissipation and heating in solar wind turbulence: from the macro to the micro and back again,” (2015).
- G. G. Howes, Physics of plasmas 25 (2018).
- W. Gekelman, Journal of Geophysical Research: Space Physics 104, 14417 (1999).
- J. Maggs and G. Morales, Physical review letters 91, 035004 (2003).
- S. Vincena and W. Gekelman, Physics of plasmas 13, 064503 (2006).
- S. Dorfman and T. Carter, Physical Review Letters 110, 195001 (2013).
- S. Dorfman and T. Carter, Physical Review Letters 116, 195002 (2016).
- B. J. Vasquez, Journal of Geophysical Research: Space Physics 100, 1779 (1995).
- L. Ofman and J. Davila, Journal of Geophysical Research: Space Physics 100, 23413 (1995).
- J. V. Hollweg, Journal of Geophysical Research: Space Physics 104, 14811 (1999).
- G. Morales and J. Maggs, Physics of Plasmas 4, 4118 (1997).
- A. F. Viñas and M. L. Goldstein, Journal of plasma physics 46, 129 (1991).
- Y. Shi, Physical Review E 99, 063212 (2019).
- D. Winske and N. Omidi, Presented at the 4th International School for Space Simulation , 1 (1991).
- D. S. Montgomery, Physics of Plasmas 23 (2016).
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