Temporal regularities of changing magnetic field generation modes in the model of the αω-dynamo

  1. Institute of Cosmophysical Researches and RadioWave Propagation Far-Eastern Branch, Russian Academy of Sciences
  2. Vitus Bering Kamchatka State University
  3. Municipal budgetary institution of supplementary education «Center «Luch»»

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.

Sheremetieva О.V., Godomskaya A.N. Temporal regularities of changing magnetic field generation modes in the model of the αω-dynamo // E3S WEB OF CONFERENCES XI International Conference “Solar-Terrestrial Relations and Physics of Earthquake Precursors”. 2020 P. 02030