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Tertiary modes in electrostatic drift-wave turbulence are localized near extrema of the zonal velocity $U(x)$ with respect to the radial coordinate $x$.
1905
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Y. Zhou, H. Zhu, and I. Y. Dodin, arXiv:1909.10479
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2019
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C.-B. Kim, B. Min, and C.-Y. An, Plasma Phys. Control. Fusion 61
2019
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Actually, due to nonzero N N , the long-time dynamics within the mHWE model can be very different from that in the Terry–Horton or Hasegawa–Mima models even at large α \alpha . See A. J. Majda, D. Qi, and A. J. Cerfon, Phys. Plasmas 25
2019
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Y. Lang, Z. B. Guo, X. G. Wang, and B. Li, Phys. Rev. E 100
2019
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Y. Zhou, H. Zhu, and I. Y. Dodin, Plasma Phys. Control. Fusion 61
2019
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