Tracking Geomagnetic Storms with Dynamical System Approach: Ground-Based Observations

Author:

Alberti Tommaso12ORCID,De Michelis Paola1ORCID,Santarelli Lucia3ORCID,Faranda Davide456,Consolini Giuseppe2ORCID,Marcucci Maria Federica2

Affiliation:

1. Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, I-00143 Rome, Italy

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

3. Istituto Nazionale di Geofisica e Vulcanologia, Viale Francesco Crispi 43/45, I-67100 L’Aquila, Italy

4. Laboratoire des Sciences du Climat et de l’Environnement, CEA Saclay l’Orme des Merisiers, UMR 8212 CEA-CNRS-UVSQ, Université Paris-Saclay & IPSL, 91191 Paris, France

5. London Mathematical Laboratory, 8 Margravine Gardens, London W6 8RH, UK

6. Ecole Normale Superieure, PSL Research University, 75005 Paris, France

Abstract

Using a dynamical systems approach, we examine the persistence and predictability of geomagnetic perturbations across a range of different latitudes and levels of geomagnetic activity. We look at the horizontal components of the magnetic field measured on the ground between 13 and 24 March 2015, at approximately 40 observatories in the Northern Hemisphere. We introduced two dynamical indicators: the extremal index θ, which quantifies the persistence of the system in a particular state and the instantaneous dimension d, which measures the active number of degrees of freedom of the system. The analysis revealed that during disturbed periods, the instantaneous dimension of the horizontal strength of the magnetic field, which depends on latitude, increases, indicating that the geomagnetic response is externally driven. Furthermore, during quiet times, the instantaneous dimension values fluctuate around the state-space dimension, indicating a more stochastic and thus less predictable nature system.

Funder

Italian National Institute for Astrophysics

Italian PNRA

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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