EGU22-8782
https://doi.org/10.5194/egusphere-egu22-8782
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Chaos and Predictability in vTEC time series

Massimo Materassi1, Yenca Migoya-Orue2, Tommaso Alberti3, Sandro Radicella4, and Giuseppe Consolini3
Massimo Materassi et al.
  • 1Istituto dei Sistemi Complessi CNR, Sesto Fiorentino, Italy (massimo.materassi@isc.cnr.it)
  • 2International Center for Theoretical Physics (ICTP), Trieste, Italy
  • 3INAF-Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy
  • 4Boston College Institute of Scientific Research, Boston, USA

Modeling the Earth’s ionosphere is a big challenge, due to the complexity of the system. Any ionospheric model misses the behavior of the real system for some fluctuating component, that appears almost impossible to predict, and is particularly threatening for the human technologies (e.g., GNSS navigation). While producing models extremely rich, including many physical agents acting on the Earth’s ionosphere, it is necessary to understand whether the residual, non-modeled component is predictable in principle as a “simple" dynamical system, or is conversely so chaotic to be practically stochastic, and should be treated probabilistically.

The question of how chaotic and how predictable the time series of vertical total electron content (vTEC) are, depending on the different locations and solar activity conditions, is dealt with by employing tools of dynamical system theory.

In particular, we calculate the correlation dimension D2 and the Kolmogorov entropy rate K2 for the vTEC time series at different latitudes in both northern and southern hemispheres and during both high and low solar activity periods.

The quantity D2 is a proxy of the degree of chaos and dynamical complexity: the larger D2 is, the higher the number of dynamical variables needed to describe the phenomenon is. Instead, K2 measures the speed of destruction of the mutual information between the signal and a delayed copy of it, so that (K2)-1 is a sort of maximum time horizon for predictability.

The analysis of the D2 and K2 for the vTEC time series will then allow to give a measure of chaos and predictability of the Earth ionosphere. Being such analysis performed for different locations and different solar activity conditions, these characteristics will indicate possible differences depending on location.

How to cite: Materassi, M., Migoya-Orue, Y., Alberti, T., Radicella, S., and Consolini, G.: Chaos and Predictability in vTEC time series, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-8782, https://doi.org/10.5194/egusphere-egu22-8782, 2022.

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