Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/15619
Authors: Consolini, Giuseppe* 
Quattrociocchi, Virgilio* 
Benella, Simone* 
De Michelis, Paola* 
Alberti, Tommaso* 
Piersanti, Mirko* 
Marcucci, Maria Federica* 
Title: On Turbulent Features of E × B Plasma Motion in the Auroral Topside Ionosphere: Some Results from CSES-01 Satellite
Journal: Remote Sensing 
Series/Report no.: /14 (2022)
Publisher: MDPI
Issue Date: 17-Apr-2022
DOI: 10.3390/rs14081936
Keywords: Turbulence
Auroral ionosphere
ExB plasma motion
Subject Classification01.02. Ionosphere 
Abstract: The recent Chinese Seismo-Electromagnetic Satellite (CSES-01) provides a good opportunity to investigate some features of plasma properties and its motion in the topside ionosphere. Using simultaneous measurements from the electric field detector and the magnetometers onboard CSES-01, we investigate some properties of the plasma ExB drift velocity for a case study during a crossing of the Southern auroral region in the topside ionosphere. In detail, we analyze the spectral and scaling features of the plasma drift velocity and provide evidence of the turbulent character of the ExB drift. Our results provide an evidence of the occurrence of 2D ExB intermittent convective turbulence for the plasma motion in the topside ionospheric F2 auroral region at scales from tens of meters to tens of kilometers. The intermittent character of the observed turbulence suggests that the macro-scale intermittent structure is isomorphic with a quasi-1D fractal structure, as happens, for example, in the case of a filamentary or thin-tube-like structure. Furthermore, in the analyzed range of scales we found that both magnetohydrodynamic and kinetic processes may affect the plasma dynamics at spatial scales below 2 km. The results are discussed and compared with previous results reported in the literature.
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