convection zone
[kənˈvekʃən zəun]

释义

对流层；

英英释义

Convection zone

• 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

双语例句

用作名词(n.)

1. This confirms the idea that the mechanical waves generated from the convection zone are not very effective in heating the chromosphere and corona.
   这就证实了一些人认为的对流层机械波并不是一个对色球和日冕的有效加热机制的说法。

权威例句

Numerical simulations of stellar convective dynamos. II - Field propagation in the convection zone
Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone
Dynamic variations at the base of the solar convection zone
Emerging flux tubes in the solar convection zone. 1: Asymmetry, tilt, and emergence latitude
The depth of the solar convection zone
Evolving Submerged Meridional Circulation Cells within the Upper Convection Zone Revealed by Ring-Diagram Analysis
Emerging Flux Tubes in the Solar Convection Zone. II. The Influence of Initial Conditions
Torsional Oscillation, Meridional Flows, and Vorticity Inferred in the Upper Convection Zone of the Sun by Time-Distance Helioseismo...
The influence of the Coriolis force on flux tubes rising through the solar convection zone
Motion of magnetic flux tubes in the solar convection zone and chromosphere