Issue |
E3S Web Conf.
Volume 196, 2020
XI International Conference “Solar-Terrestrial Relations and Physics of Earthquake Precursors”
|
|
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Article Number | 02030 | |
Number of page(s) | 9 | |
Section | Geophysical Fields and their Interactions | |
DOI | https://doi.org/10.1051/e3sconf/202019602030 | |
Published online | 16 October 2020 |
Temporal regularities of changing magnetic field generation modes in the model of the αΩ-dynamo
1 Institute of Cosmophysical Research and Radio Wave Propagation FEB RAS, Paratunka, Russia
2 Municipal budgetary institution of supplementary education «Center «Luch»», Yelizovo, Russia
* Corresponding author: olga.v.sheremetyeva@gmail.com
** anna_antonenko@mail.ru
In the dynamic model aΩ-dynamo the change in the intensity of the a-generator under the action of external forces is considered as a result of synchroniza-tion of higher modes of the velocity field and the magnetic field and is regulated by the function Z(t) with an exponential-power kernel J(t). Depending on the choice of the exponent and the scale factor of the kernel determine its temporal characteristics: delay time and waiting time. The question of changing the modes of magnetic field generation depending on the temporal characteristics of the function’s kernel is investigating. In the dynamic model aΩ-dynamo the change of the a-generator intensity under the action of external forces is considered as a result of synchronization of higher modes of the velocity field and the magnetic field and is regulated by the function Z(t) with an exponential-power kernel J(t). Depending on the choice of the exponent and the scale factor of the kernel J(t) determine its temporal characteristics: delay time and waiting time. The question of changing the modes of magnetic field generation depending on the temporal characteristics of the function’s kernel is investigating.
© The Authors, published by EDP Sciences, 2020
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