Modeling Solar Wind Activity Using a Physical Second-Order Oscillator Approach

Please use this identifier to cite or link to this item: http://openlibrary.ge/handle/123456789/10731

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DC Field	Value	Language
dc.contributor	Mikheil Nodia Institute of Geophysics of Ivane Javakhishvili Tbilisi State University, Tbilisi, Georgia	en
dc.contributor.author	Kiria, T.	en
dc.contributor.author	Nikolaishvili, M.	en
dc.contributor.author	Chkhaidze, T.	en
dc.date.accessioned	2025-11-21T17:21:54Z	-
dc.date.available	2025-11-21T17:21:54Z	-
dc.date.issued	2025	-
dc.identifier.citation	1st International Scientific Conference “Modern problems in Geophysics”. Proceedings, ISBN 978-9941-36-434-1, ISSN 3088-4349, Tbilisi, Georgia, November 6-8, 2025. Publish House of Iv. Javakhishvili Tbilisi State University, Tbilisi, 2025, pp. 258-260.	en
dc.identifier.uri	http://openlibrary.ge/handle/123456789/10731	-
dc.description.abstract	This paper presents a second-order differential equation model describing the dynamics of solar wind activity. The model captures the system’s oscillatory nature by incorporating lunar illumination and daily periodic forcing as external drivers. Parameter calibration shows the model’s capacity to forecast activity trends with physical interpretability	en
dc.language.iso	en	en
dc.subject	Modern problems in Geophysics	en
dc.subject	Proceedings	en
dc.subject	geomagnetism	en
dc.subject	geophysics	en
dc.subject	modeling	en
dc.title	Modeling Solar Wind Activity Using a Physical Second-Order Oscillator Approach	en
dc.type	Article	en
Appears in Collections:	1st International Scientific Conference “Modern problems in Geophysics”. Proceedings, Tbilisi, Georgia, November 6-8, 2025

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