n.（太阳的）色球层

The chromosphere is the outermost layer of the Sun, just above the photosphere where we can see sunspots.
色球层是太阳的最外层，就在我们可以看到太阳黑子的光球层之上。
Astronomers study the chromosphere's dynamic behavior during solar flares to understand the Sun's magnetic activity.
天文学家研究色球层在太阳耀斑期间的动态行为，以了解太阳的磁活动。
The chromosphere exhibits a beautiful rosy glow during sunrise and sunset, known as the "corona.
日出和日落时，色球呈现出美丽的粉红色光芒，这就是我们所说的"日冕"。
The temperature in the chromosphere increases with height, reaching up to 5,000 degrees Celsius.
色球层的温度随高度升高而增加，最高可达5000摄氏度。
Solar astronomers use spectrometers to analyze the light emitted from the chromosphere, revealing information about its composition.
太阳天文学家使用光谱仪分析从色球层发出的光线，揭示其组成信息。
Chromospheric material occasionally erupts in coronal mass ejections, posing potential hazards to Earth's space environment.
色球物质偶尔会爆发形成日冕物质抛射，对地球的空间环境构成潜在威胁。
The chromosphere plays a role in the formation of solar prominences, which are large, filamentary structures suspended above the Sun's surface.
色球层参与太阳黑子的形成，这些是悬挂在太阳表面的巨大丝状结构。
Observations of the chromosphere help scientists track solar magnetic reconnection events, a critical process in energy release on the Sun.
对色球层的观察有助于科学家追踪太阳磁场的重新连接事件，这是太阳能量释放的关键过程。
The chromosphere's intricate dynamics and colorful appearance make it a popular subject for amateur astronomers with telescopes.
色球层复杂多变的动态和多彩的外观使其成为业余天文爱好者用望远镜观测的热门对象。
In recent years, advanced imaging techniques have enabled us to observe the chromosphere with unprecedented detail, revealing previously unseen features.
近年来，先进的成像技术使我们能够以前所未有的细节观察色球层，揭示了新的特征。