“…According to Kintner and Seyler (), the range of scales where turbulence plays a relevant role is from few meters up to ∼1000 km in the topside F region of the high‐latitude ionosphere, a range of spatial scales where large magnetic and electric field fluctuations have been observed. In recent years, an extensive literature has demonstrated that high‐latitude magnetic and electric field fluctuations, as well as plasma density variations, show scale‐invariance and intermittent turbulent features (De Michelis et al, ; ; Golovchanskaya et al, , Spicher et al, ; Tam Sunny et al, ). Furthermore, the scale‐invariance nature of magnetic field fluctuations has been shown to be a function of the different polar regions (polar cap, cusp, auroral oval), the magnetic local time, the interplanetary magnetic field conditions and the geomagnetic activity disturbance level (De Michelis et al, , , ).…”