Scientists study the Sun's chromosphere for solar activity insights.
科学家研究太阳的色球层以了解太阳活动。
The chromosphere is located above the Sun's photosphere layer.
色球层位于太阳光球层之上。
A solar flare often originates in the chromosphere region.
太阳耀斑通常起源于色球层区域。
The chromosphere appears reddish due to hydrogen emissions.
色球层由于氢发射而呈现红色。
During an eclipse, the chromosphere can be briefly observed.
在日食期间，可以短暂观察到色球层。
Temperature in the chromosphere rises with altitude increase.
色球层的温度随着高度增加而升高。
The chromosphere is key to understanding solar magnetic fields.
色球层是理解太阳磁场的关键。
Scientists use spectroscopy to study the chromosphere.
科学家使用光谱学来研究色球层。
The chromosphere plays a role in solar wind generation.
色球层在太阳风的产生中起作用。
The chromosphere can be a dynamic and turbulent layer.
色球层可能是一个动态和湍流的层。
chromosphere temperature 色球层温度
chromosphere activity 色球层活动
chromosphere emission 色球层辐射
chromosphere observation 色球层观测
chromosphere structure 色球层结构
chromosphere dynamics 色球层动力学
chromosphere heating 色球层加热
