NASA NTRS · 19850003543
Strong Langmuir turbulence
Abstract
Beam-excited Langmuir turbulence in the solar wind is discussed and the criteria for wave-particle, three-wave and strong turbulence interactions are explained. The results of a numerical integration of the Zakharov equations are presented which describe the strong turbulence saturation of a weak (low-density) high energy, bump-on-tail beam instability.
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Goldman, M. V.. 1984-07-01. Strong Langmuir turbulence. https://ntrs.nasa.gov/citations/19850003543
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