Parametric instability, inverse cascade and the range of solar-wind turbulence
نویسندگان
چکیده
منابع مشابه
Small scale energy cascade of the solar wind turbulence
Magnetic fluctuations in the solar wind are distributed according to Kolmogorov’s power law f below the ion cyclotron frequency fci. Above this frequency, the observed steeper power law is usually interpreted in two different ways: a dissipative range of the solar wind turbulence or another turbulent cascade, the nature of which is still an open question. Using the Cluster magnetic data we show...
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ژورنال
عنوان ژورنال: Journal of Plasma Physics
سال: 2018
ISSN: 0022-3778,1469-7807
DOI: 10.1017/s0022377818000016