Scale‐free statistics of spatiotemporal auroral emissions as depicted by POLAR UVI images: Dynamic magnetosphere is an avalanching system

By V. Uritsky, A. Klimas, D. Vassiliadis, D. Chua, G. Parks. 2002

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Particle Acceleration in the Magnetotail and Aurora (2012, background): “Similar statistical trends were found by Lund (2010) for FAST auroral observations and Uritsky et al. (2002) for global images of the aurora.”
Geomagnetic storm of 29–31 October 2003: Geomagnetically induced currents and their relation to problems in the Swedish high‐voltage power transmission system (2005, background): “…characteristic temporal or spatial scales in the ionospheric electrodynamics as indicated by statistical studies of auroral phenomena [see, e.g., Uritsky et al., 2002, and references therein] and the fact addressed above that geomagnetic induction can be considered as a high-pass filtering of…”
25 Years of Self-Organized Criticality: Solar and Astrophysics (2014, methodology): “…or size distributions with a powerlaw shape (Table 11), the hallmark of SOC systems, have been measured from auroral blobs in UV (Lui et al. 2000; Uritsky et al. 2002, 2003, 2006) and optical light (Kozelov et al. 2004), from the auroral electron jet index (AE) (Takalo 1993; Consolini 1997,…”