2016
DOI: 10.3367/ufnr.2016.02.037727
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Current results on the asymptotics of dynamo models

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Cited by 4 publications
(2 citation statements)
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“…The set of P,T V 2 4 , P,T V 3 4 and P,T B 0 1 is two disk dynamo [2] and so on. In thin convective layer as on the Sun, number of modes in the Dynamo wave is large and WKB approximation may be used [3]. Fist the solar activity was considered as the Van der Pol oscillator [4].…”
Section: Magnetic Dynamo As Atom In the Resonatormentioning
confidence: 99%
“…The set of P,T V 2 4 , P,T V 3 4 and P,T B 0 1 is two disk dynamo [2] and so on. In thin convective layer as on the Sun, number of modes in the Dynamo wave is large and WKB approximation may be used [3]. Fist the solar activity was considered as the Van der Pol oscillator [4].…”
Section: Magnetic Dynamo As Atom In the Resonatormentioning
confidence: 99%
“…The idea of a relaxation generator in one form or another was used to create the theory of a magnetic dynamo [7][8][9][10][11][12][13][14][15][16][17][18][19][20][21][22] and see additionally the reviews [23][24][25], but there is no convection in the early models. The low-mode models with convection have a particular place in this theory [26][27][28][29], but only the representation of the dynamo in the form of the multidimensional Lienard oscillator [1] defines correctly the symmetry of the system and opens up new ways in the development of nonlinear physics thanks to the universality and productivity of the new dynamo paradigm and the specificity of relaxation oscillations.…”
Section: Introductionmentioning
confidence: 99%