chromosphere
英
美
n. （太阳的）色球层
COCA.39512
英英释义
noun
- a gaseous layer of the sun's atmosphere (extending from the photosphere to the corona) that is visible during a total eclipse of the sun
双语例句
- Acoustic waves are a primary candidate for supplying the energy necessary to heat the solar chromosphere and corona.
声波是供给太阳色球和日冕加热所需能量的主要候选能源。 - Starting at the outside and going down into the Sun, the zones are the corona, chromosphere, photosphere. 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。 - Solar spicules are rapidly evolving jets seen on the solar limb, extending from the bottom of the chromosphere to the corona. Spicule is the most common feature observed in the chromosphere.
太阳针状物是日面边缘上快速演化的喷流状结构，它可以从色球底部一直延伸到日冕，是色球层最普遍的观测现象之一。 - Solar-like Activities in Late-type Stars ( ⅱ): Active Chromosphere, Transition Region and Coronal Emissions, and Stellar Flares
晚型恒星中的类太阳活动（Ⅱ）：活动色球、过渡区和冕区发射、耀发活动 - 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。 - No, it was flare eruptions, which are the chromosphere and prominence on the landscape.
不，那是耀斑爆发，它与日珥都是色球层上的景观。 - The results indicate that the heating in the lower chromosphere and the upper photosphere, especially for large flares, can be caused neither by X-ray radiation nor by electron beam bombardment.
耀斑主相时，X线加热更能有效地平衡辐射损失.但是，尤其是对大耀斑来说，色球低层和光球上层的加热既不能用电子束轰击，也不能用X线的作用来解释； - Center to limb observations show that the magnetic structures of small scale magnetic structures have not changed much when they extend from the solar photosphere to the chromosphere.
日面中心到边缘的观测表明，太阳宁静区中的小尺度磁结构在从光球到色球的扩展过程中变化不大。 - It is difficult to photograph the actual chromosphere.
拍摄实际的色球层很困难。 - Beyond the photosphere in the chromosphere and the extremely rarified corona, which extends millions of kilometres into space.
在光球层更外面的色球层以及极其稀薄的电晕，在空中延展几百万千米的范围。