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图片展示了太阳表面成群的太阳黑子,这些黑斑呈带状分布在太阳赤道的上方和下方

太阳黑子

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图注: 在这张图片中,太阳在2012年7月至8月的近九天里布满了成群的太阳黑子。这张图片中看到的太阳黑子是太阳耀斑和日冕物质抛射(CME)的源头。特别是,在这张图片中,太阳正接近其周期(太阳周期)中的太阳活动最大值,我们可以看到许多黑子沿着太阳赤道形成。这些太阳黑子和活动出现在太阳的南半球,在此之前,大部分活动都发生在北半球。
来源: NASA/SDO/HMI
来源链接

词汇表: 太阳 , 太阳黑子 , 恒星活动
分类: 太阳

授权许可: 公共领域 公共领域 图标

文件 ( 图像 153.32 kB)


A poster including a giant scale illustrating equality when day and night have the same length

Equal Day 2026 Poster

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图注: The Poster for Equal Day 2026


文件 ( 图像 540.62 kB)


A poster with an hourglass with the moon and sun in it and a dove. The text reads 'equal day'

Equal Day 2025 poster

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图注: The poster for Equal Day 2025
来源: OAE Center Italy/NAEC Lebanon


文件 ( 图像 1.63 MB)


The Sun as red disk with bright patches and long dark strands. Several small wispy features protrude from the disk's edge

H-alpha image of the Sun's chromosphere

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图注: This false-color image was captured with a 10-cm telescope at the Big Bear Solar Observatory (BBSO) in the United States in July 2002. It depicts the full disk of the Sun using the H-alpha emission line of hydrogen. When observed in this spectral line, the Sun's chromosphere appears particularly prominent due to hydrogen atoms emitting light at the specific wavelength. This emission produces a distinctive red color, making features such as spicules (jets of plasma that look hair-like) and plage (bright patches in the chromosphere) highly visible. Several small solar prominences can be seen protruding from the edge of the solar disk. When prominences (also known as filaments) cross the face of the disk they appear as dark threads caused by the cooler material in the prominence absorbing light. The chromosphere is also visible in the violet part of the solar spectrum due to ionized calcium showing emissions in these wavelengths.
来源: Big Bear Solar Observatory (BBSO)/New Jersey Institut of Technology (NJIT)
来源链接

词汇表: 色球 , 日珥 , 太阳 , 光谱线
分类: 太阳

授权许可: 公共领域 公共领域 图标

文件 ( 图像 2.82 MB)


A dark, roughly circular, black sunspot sends dark fingers out into the bright orange surroundings

Close-up view of a sunspot

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图注: This image of a sunspot was taken by the Daniel K Inouye Solar Telescope (DKIST), operated by the U.S. National Science Foundation. It was taken only in light with a wavelength of 530 nanometers, within the greenish-yellow part of the visible spectrum. The picture reveals the detail of the spot's structure and the Sun’s photosphere. The dark central region, known as the umbra, is surrounded by a lighter area called the penumbra with radially elongated features stretching towards the umbra. Note that the umbra and penumbra here are not the same as the umbra and penumbra that occur during an eclipse. The sunspot measures approximately 5000 kilometres in diameter, roughly equivalent to the east-west span of China. While the umbra appears black, it is actually hot and bright. It only appears dark because it is a few thousand kelvin cooler than the surrounding solar photosphere. Surrounding the sunspot, granulation patterns of plasma are visible on the photospheric surface of the Sun.
来源: NSO/NSF/AURA
来源链接

词汇表: 光球 , 太阳 , 太阳黑子 , 米粒组织

授权许可: 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 知识共享许可协议 署名 4.0 国际 (CC BY 4.0) 图标

文件 ( 图像 5.23 MB)


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