Space-climatic feedback of the magnetic solar cycle through the interplanetary space.

Autor: Carbone V; Department of Physics, University of Calabria, 87036, Rende, Italy., Alberti T; Istituto Nazionale di Geofisica e Vulcanologia, 00143, Rome, Italy. tommaso.alberti@ingv.it.; INAF-Istituto di Astrofisica e Planetologia Spaziali, 00133, Rome, Italy. tommaso.alberti@ingv.it., Reda R; Department of Physics, University of Rome Tor Vergata, 00133, Rome, Italy., Giovannelli L; Department of Physics, University of Rome Tor Vergata, 00133, Rome, Italy.
Jazyk: angličtina
Zdroj: Scientific reports [Sci Rep] 2024 Aug 27; Vol. 14 (1), pp. 19850. Date of Electronic Publication: 2024 Aug 27.
DOI: 10.1038/s41598-024-70583-4
Abstrakt: The relationship between solar magnetic activity and solar wind parameters, with observed time-delayed mutual coupling, is an outstanding challenge in space physics. In this study, drawing inspiration from recent observations, we propose a reconciliation framework whose fundamentals stand in the Parker model for solar wind expansion. We investigate the effects on fluctuations in solar wind speed when linearly sustained by an oscillating magnetic solar dynamo described via a modified Van der Pol nonlinear oscillator mimicking the magnetic activity at different timescales. Our findings reveal the presence of a "space-climatic feedback" that, in absence of the driving magnetic activity, slows down solar wind velocity fluctuations. The combined action of the slowing down of fluctuations and a periodic driving is the responsible for the time-delay between solar magnetic activity and solar wind dynamics. Furthermore, we also demonstrate how the space-climatic feedback controls the value of the time-delay which depends on the different periodicities of the driving magnetic activity. This holistic approach provides a formal link at the interplay between solar magnetic activity and solar wind dynamics through the interplanetary space which can advance our understanding of long-term effects of solar activity on solar wind variations, and consequently on interactions with planetary environments.
(© 2024. The Author(s).)
Databáze: MEDLINE
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