Multimode Representation of the Magnetic Field for the Analysis of the Nonlinear Behavior of Solar Activity as a Driver of Space Weather
Elena Popova,
Anatoli I. Popov and
Roald Sagdeev
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Elena Popova: Centro de Investigación en Astronomía, Universidad Bernardo O’Higgins, Santiago 8370854, Chile
Anatoli I. Popov: Institute of Solid State Physics, University of Latvia, LV-1063 Riga, Latvia
Roald Sagdeev: Department of Physics, University of Maryland, College Park, MD 20742-4111, USA
Mathematics, 2022, vol. 10, issue 10, 1-10
Abstract:
Estimating and predicting space weather is important to the space industry and space missions. The driver of space weather, especially near the Earth, is solar activity, the study of which is an important task. In particular, there is a direction of problems based on models of solar magnetic field generation that require research. In our work, we build a nonlinear dynamic system of equations that describes the behavior of the solar magnetic field harmonics based on the alpha-omega dynamo model. We found that, at the beginning of the magnetic field generation process, when the dynamo number significantly exceeds the threshold, the most rapidly growing waves are in the lead. Then, over time, these waves stop growing quite quickly. In this case, the initially slowly increasing harmonics of the magnetic field become the leaders, which then make the main contribution to the process of magnetic field generation.
Keywords: space weather; dynamic systems; multimode representation; solar activity; nonlinear system (search for similar items in EconPapers)
JEL-codes: C (search for similar items in EconPapers)
Date: 2022
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Citations: View citations in EconPapers (1)
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