Axisymmetric Magnetic Fields Can Be Stably Generated by Simple Convection
DOI:
https://doi.org/10.51094/jxiv.520Keywords:
Cowling’s theorem, dynamo theory, simple convection, neutral pointAbstract
Researchers have struggled to understand the mechanism underlying the formation of celestial magnetic fields. In some studies, the conception of this mechanism, such as Cowling's theorem, which posits that complex convection is necessary to generate a magnetic field, constrains research. Research in this field could progress through the discovery of a simple mechanism. To reveal a possible simple mechanism, this paper addresses generating a magnetic field by convection, which is a simple concept. Whether an axisymmetric poloidal magnetic field can be stably generated by the axisymmetric poloidal convection of a conductive fluid depends on whether the induction term contains a source of power generation. This problem can be solved by decomposing and examining the induction term in detail. Cowling's theory omits certain components (terms) from this term; however, in this study, these components are found to be essential for axisymmetric magnetic field generation on the basis of calculations and examination of the total amount of energy. This approach is a novel concept. In addition, another claim of Cowling's theorem concerning the neutral point is also disputed. Consequently, even under simple axisymmetric convection, the possibility of generating axisymmetric magnetic fields is demonstrated. These findings will contribute to further elucidation of the mechanism of magnetic field formation. However, in this work, unresolved points are found in the maintenance of the magnetic field and the deformation of the formula.
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References
Levy, E.H.: Generation of planetary magnetic fields. Annu. Rev. Earth Planet. Sci. 4, 159–185 (1976)
Parker, E.N.: Hydromagnetic dynamo models. Astrophysical J. 122, 293–314 (1955)
Cowling, T.G.: The magnetic field of sunspots. Monthly Notices Roy. Astronomical Soc. 94(1), 39–48 (1933)
Cardin, P., Cugliandolo, L.G.: Dynamos: Lecture Notes of the Les Houches Summer School 2007. Les Houches. Elsevier Science, Oxford (2011). https://books. google.co.jp/books?id=OVgaews3C1IC
Moffatt, K., Dormy, E.: Self-Exciting Fluid Dynamos. Cambridge Texts in Applied Mathematics. Cambridge University Press, Cambridge (2019)
Davidson, P.A.: Introduction to Magnetohydrodynamics. Cambridge Texts in Applied Mathematics. Cambridge University Press, Cambridge (2017). https: //books.google.co.jp/books?id=TtocDgAAQBAJ
Pollack, G.L., Stump, D.R.: Electromagnetism. Addison Wesley, San Francisco (2002). https://books.google.co.jp/books?id=wes9AQAAIAAJ
Otsuki, M.: Boosting the Magnetic Field of a Toroidal Conductive Fluid by a Poloidal Flow. Preprint at https://doi.org/10.51094/jxiv.284 (2023)
Alfv´en, H.: On the Existence of Electromagnetic-Hydrodynamic Waves. Arkiv for Matematik, Astronomi och Fysik 29B, 1–7 (1943)
Fitzpatrick, R.: Cowling Anti-Dynamo Theorem. Available from https://farside. ph.utexas.edu/teaching/plasma/lectures1/node115.html Accesses 10/12/2024
(2019)
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Submitted: 2023-10-03 22:05:46 UTC
Published: 2023-10-16 02:08:10 UTC — Updated on 2025-02-06 02:09:06 UTC
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Mamoru Otsuki

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