Multi-Time-Scale Analysis of Chaos and Predictability in vTEC

Author:

Materassi Massimo1ORCID,Migoya-Orué Yenca2ORCID,Radicella Sandro Maria3ORCID,Alberti Tommaso45ORCID,Consolini Giuseppe5ORCID

Affiliation:

1. Institute for Complex Systems of the National Research Council CNR ISC, Via Madonna del Piano 10, 50019 Sesto Fiorentino, Italy

2. STI Unit, The Abdus Salam International Centre for Theoretical Physics (ICTP), Strada Costiera 11, 34151 Trieste, Italy

3. Visiting Research Scholar, Institute of Scientific Research, Boston College, Newton, MA 02459, USA

4. Istituto Nazionale di Geofisica e Vulcanologia (INGV), Via di Vigna Murata, 605, 00143 Rome, Italy

5. INAF-Istituto di Astrofisica e Planetologia Spaziali, Via del Fosso del Cavaliere 100, 00133 Rome, Italy

Abstract

Theoretical modelling of the local ionospheric medium (LIM) is made difficult by the occurrence of irregular ionospheric behaviours at many space and time scales, making prior hypotheses uncertain. Investigating the LIM from scratch with the tools of dynamical system theory may be an option, using the vertical total electron content (vTEC) as an appropriate tracer of the system variability. An embedding procedure is applied to vTEC time series to obtain the finite dimension (m∈N) of the phase space of an LIM-equivalent dynamical system, as well as its correlation dimension (D2) and Kolmogorov entropy rate (K2). In this paper, the dynamical features (m,D2,K2) are studied for the vTEC on the top of three GNSS stations depending on the time scale (τ) at which the vTEC is observed. First, the vTEC undergoes empirical mode decomposition; then (m,D2,K2) are calculated as functions of τ. This captures the multi-scale structure of the Earth’s ionospheric dynamics, demonstrating a net distinction between the behaviour at τ≤24h and τ≥24h. In particular, sub-diurnal-scale modes are assimilated to much more chaotic systems than over-diurnal-scale modes.

Funder

Italian National Institute for Astrophysics

Publisher

MDPI AG

Reference22 articles.

1. Kelley, M.C. (1989). The Earth’s Ionosphere—Plasma Physics and Electrodynamics, Elsevier Inc.

2. Materassi, M., Forte, B., Coster, A., and Skone, S. (2020). The Dynamical Ionosphere—A Systems Approach to Ionospheric Irregularity, Elsevier Inc.

3. Goodman, J.M. (2005). Space Weather & Telecommunications, Springer.

4. Hunsucker, R.D. (2013). Radio Techniques for Probing the Terrestrial Ionosphere, Springer Science & Business Media.

5. The TEC and F2 parameters as tracers of the ionosphere and thermosphere;Lilensten;J. Atmos. Sol.-Terr. Phys.,2002

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