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New turbulent effects of reconstruction of solar magnetism

Вісник астрономічної школи

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Field Value
 
Title New turbulent effects of reconstruction of solar magnetism
 
Creator Krivodubskij V.N.
 
Date 2014
 
Source Astronomical School’s Report, 2014, Volume 10, Issue 2, P. 85-89
2411-6602
 
Identifier http://astro.nau.edu.ua/papers/AstSR_2014_Vol_10_Iss_2_P_85.pdf
10.18372/2411-6602.10.2085
 
Language uk
 
Description Two effects of turbulent transfer of magnetic field in the convective zone of the Sun, the topological pumping and “turbulent buoyancy”, are investigated. It is shown that the topological pumping contributes to the vertical stratification of the magnetic fields into the magnetic tubes. While the “turbulent buoyancy” near the bottom of the solar convection zone is able to compensate the classical magnetic buoyancy of strong magnetic fields.
 
Publisher National Aviation University
 
Format application/pdf
 

Технічна підтримка: НДІІТТ НАУ