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Glossary term: 太阳黑子

Description: 太阳黑子是由于太阳光球层中的强磁场引起的暂时性冷区。太阳黑子是磁通管从太阳深处涌出的区域。强磁场增加了这些区域的磁压力。为了保持与周围环境相同的压力,太阳黑子中的气体和等离子体压力必须下降,这就使其温度低于周围环境。由于太阳黑子比周围的光球温度低,因此可以通过望远镜看到太阳黑子,是太阳表面的暗斑/斑点。太阳黑子的大小从几十公里到十几万公里不等。持续时间从几天到几个月不等。太阳黑子的数量和位置随太阳周期而变化。其他恒星也被认为有由其磁场引起的黑子。

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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

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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

Caption: 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。
Credit: NASA/SDO/HMI credit link

License: PD Public Domain icons

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