Small‐Scale Energy Cascade of the Solar Wind Turbulence
Small‐Scale Energy Cascade of the Solar Wind Turbulence
Magnetic fluctuations in the solar wind are distributed according to Kolmogorov's power law f−5/3 below the ion cyclotron frequency fci. Above this frequency, the observed steeper power law is usually interpreted in two different ways, as a dissipative range of the solar wind turbulence, or another turbulent cascade, the nature …