The helioseismological results about the Solar law of rotation pose some serious problems for dynamo theory. However, if the magnetic flux is bounded in the lower part of the convection zone and the a-effect is concentrated at the equator, it is possible to obtain correct butterfly diagrams. ...
convection zone Wikipedia convection zone n. A region of turbulent plasma located within a star, through which energy is transported outward by convection. In a convection zone, hot plasma rises, cools as it recedes from the hot stellar center, and then falls to be heated and rise again. ...
convection zone. and finally the core.(从太阳外部开始进入内部这些区域为:光环带、色球带、光球带、对流带,最终为核心带。) Evaluation results show that the turbulence in convection zone is capable of generating enough wave energy to supply coronal energy lose due to convection and radiation.(利用...
The convection zone of a star is the range of radii in which energy is transported primarily by convection. In the radiation zone, energy is transported by radiation. 以上来源于:Wikipedia 学习怎么用 双语例句 用作名词(n.) This confirms the idea that the mechanical waves generated from the conv...
We conclude that the extremely rich and complicated dynamics of the upper convection zone reveal remarkable organization on the large scale, which can be correlated with the magnetic activity zones. 展开 关键词: Sun : activity Sun : helioseismology Sun : interior Sun : oscillations Sun : rotation...
Application of digital image correlation technique to dynamic measurement of the velocity field in the deformation zone in cold rolling 热度: Using the stress relaxation and dynamic tests to evaluate the viscoelastic properties of dough from soft wheat cultivars ...
convection theory of cyclones Convection zone Convection, Rotation and Planetary Transits Convection, Rotation and Planetary Transits convectional convectional convectional convectional stability convections convections convections convective convective convective convective convective activity Convective and Orographic...
Dynamics of Emerging Flux Tubes in the Sun This paper is intended to study the evolution of a magnetic flux tube that rises from the upper convection zone to the solar atmosphere by means of a 2.5-d... Magara,T. - 《Astrophysical Journal》 被引量: 68发表: 2008年 ...
The process of emergence of magnetic flux from the depths of the convection zone to the surface is presented in the framework of self-consistent model for the storage of field in the lower overshoot regions and as the mechanism responsible for some of the regularities observed in active regions...
The intensity of the non-equilibrium zone inside the cavity is increased with an increase in modified Rayleigh numberThe temperature fields are significantly affected by the effective thermal conductivity ratio than the scaled heat transfer coefficient of the fluid Zemach et al. [105] with permission...