Markov property of the Super-MAG auroral electrojet indices. (November 2022)

• Record Type: Journal Article
• Authors: Benella, Simone; Consolini, Giuseppe; Stumpo, Mirko; Alberti, Tommaso; Gjerloev, Jesper W.
• Is Part Of: Chaos, solitons and fractals. Volume 164(2022)
• Publication Date: 2022-11
• Subjects: Near-earth electromagnetic environment dynamics -- Geomagnetic indices -- Markov processes -- Complex timeseries analysis; Chaotic behavior in systems -- Periodicals; Solitons -- Periodicals; Fractals -- Periodicals; Chaotic behavior in systems; Fractals; Solitons; Periodicals; 003.7
• DOI: 10.1016/j.chaos.2022.112736
• Languages: English
• ISSNs: 0960-0779

Abstract

Abstract: The dynamics of the Earth's magnetosphere exhibits strongly fluctuating patterns as well as non-stationary and non-linear interactions, more pronounced during magnetospheric substorms and magnetic storms. This complex dynamics comprises both stochastic and deterministic features occurring at different time scales. Here we investigate the stochastic nature of the magnetospheric substorm dynamics by analyzing the Markovian character of SuperMAG SME and SML geomagnetic indices. By performing the Chapman–Kolmogorov test, the SME/SML dynamics appears to satisfy the Markov condition at scales below 60 min. The Kramers–Moyal analysis instead highlights that a purely diffusive process is not representative of the magnetospheric dynamics, thus a model that includes both diffusion and Poisson-jump processes is used to reproduce the SME dynamical features at small scales. A discussion of the similarities and differences between this model and the SME properties is provided with a special emphasis on the metastability of the Earth's magnetospheric dynamics. Finally, the relevance of our results in the framework of Space Weather is also addressed. Highlights: The statistics of the SME index satisfies the Markov property below 60 min. The small scale magnetospheric dynamics is modeled in terms of jump–diffusion process. The SME non-Markovian nature can be related to the metastability of the magnetosphere.