Loading...

This page describes an image A Coronal Mass Ejection

下载文件 ( 图像 596.22 kB)

图片说明 A burst of solar material can be seen erupting from the Sun in this view, illustrating a coronal mass ejection (CME)—a large eruption of plasma and magnetic field from the Sun’s outer atmosphere, or corona. These CMEs are caused by magnetic explosions in the Sun's corona. During a CME, huge amounts of electrically charged particles are launched into space at great speeds, carrying part of the Sun’s magnetic field with them. These events are driven by changes in the Sun’s magnetic structure and release vast clouds of hot gas that travel outward into the solar system. When a CME moves through space, it can interact with a planet’s magnetic field and atmosphere, sometimes creating spectacular auroras or, in strong cases, interfering with artificial satellites and power systems.

CMEs are often associated with a temporary brightening of the region of the Sun where the CME originated. This is known as a solar flare. Stars other than the Sun can also have CMEs and flares.

This image was taken by NASA's Solar Dynamics Observatory (SDO). This is a space mission to monitor the Sun. The image here is taken at a special wavelength which partially ionised helium emits strongly at.
滚动查看其他语言的字幕


图片来源 NASA/Goddard/SDO 来源链接

相关术语表词条: 太阳 , 日冕物质抛射(CME)

图片许可: 公共领域 公共领域 图标

OAE 网站上展示的媒体文件说明文字是由 OAE、OAE 各中心与节点、OAE 的 国家天文教育协调员(NAECs) 和其他志愿者共同撰写、翻译与审核的。您可以在 这里 查看我们翻译项目的完整致谢名单。所有媒体文件说明均遵循 Creative Commons CC BY-4.0 许可协议进行发布,应注明来源为“IAU OAE”。媒体文件本身可能有不同的许可协议(见上文),请根据“来源”部分注明相应来源。

如果您发现此词汇术语或定义中的事实或翻译错误, 请向 发邮件 联系.

其他语言版本的图注

英语
图片说明 A burst of solar material can be seen erupting from the Sun in this view, illustrating a coronal mass ejection (CME)—a large eruption of plasma and magnetic field from the Sun’s outer atmosphere, or corona. These CMEs are caused by magnetic explosions in the Sun's corona. During a CME, huge amounts of electrically charged particles are launched into space at great speeds, carrying part of the Sun’s magnetic field with them. These events are driven by changes in the Sun’s magnetic structure and release vast clouds of hot gas that travel outward into the solar system. When a CME moves through space, it can interact with a planet’s magnetic field and atmosphere, sometimes creating spectacular auroras or, in strong cases, interfering with artificial satellites and power systems.

CMEs are often associated with a temporary brightening of the region of the Sun where the CME originated. This is known as a solar flare. Stars other than the Sun can also have CMEs and flares.

This image was taken by NASA's Solar Dynamics Observatory (SDO). This is a space mission to monitor the Sun. The image here is taken at a special wavelength which partially ionised helium emits strongly at.
图片来源 NASA/Goddard/SDO
相关术语表词条: Coronal Mass Ejection (CME) , Sun