Disentangling the solar activity-solar wind predictive causality at Space Climate scales
Raffaele Reda, Mirko Stumpo, Luca Giovannelli, Tommaso Alberti and, Giuseppe Consolini

TL;DR
This study investigates the causal relationship between solar activity and solar wind at decadal scales, revealing a delayed response and significant information flow, which could improve space climate predictions.
Contribution
It introduces a novel application of Hilbert-Huang Transform and Transfer Entropy to analyze solar activity and wind causality at long time scales.
Findings
Confirmed delayed response of solar wind to solar activity (~3.1-3.4 years)
Identified significant information flow from solar activity to solar wind (~3.6 years lag)
Demonstrated potential for improved space climate predictive models
Abstract
The variability in the magnetic activity of the Sun is the main source of the observed changes in the plasma and electromagnetic environments within the heliosphere. The primary way in which solar activity affects the Earth's environment is via the solar wind and its transients. However, the relationship between solar activity and solar wind is not the same at the Space Weather and Space Climate time scales. In this work, we investigate this relationship exploiting five solar cycles data of Ca II K index and solar wind parameters, by taking advantage of the Hilbert-Huang Transform, which allows to separate the contribution at the different time scales. By filtering out the high frequency components and looking at decennial time scales, we confirm the presence of a delayed response of solar wind to Ca II K index variations, with a time lag of ~ 3.1-year for the speed and ~ 3.4-year for…
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Taxonomy
TopicsMarket Dynamics and Volatility · Solar and Space Plasma Dynamics · Global Energy and Sustainability Research
