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Glossary term: 太陽黑子

Description: 太陽黑子是由於太陽光球層中的強磁場引起的暫時性冷區。太陽黑子是磁通管從太陽深處湧出的區域。強磁場增加了這些區域的磁壓力。為了保持與周圍環境相同的壓力,太陽黑子中的氣體和等離子體壓力必須下降,這就使其溫度低於周圍環境。由於太陽黑子比周圍的光球溫度低,因此可以通過望遠鏡看到太陽黑子,是太陽表面的暗斑/斑點。太陽黑子的大小從幾十公里到十幾萬公裡不等。持續時間從幾天到幾個月不等。太陽黑子的數量和位置隨太陽週期而變化。其他恆星也被認為有由其磁場引起的黑子。

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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

This is an automated transliteration of the simplified Chinese translation of this term

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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圖片展示了太陽表面成群的太陽黑子,這些黑斑呈帶狀分布在太陽赤道的上方和下方

太陽黑子

Caption: 在這張圖片中,太陽在2012年7月至8月的近九天里布滿了成群的太陽黑子。這張圖片中看到的太陽黑子是太陽耀斑和日冕物質拋射(CME)的源頭。特別是,在這張圖片中,太陽正接近其週期(太陽週期)中的太陽活動最大值,我們可以看到許多黑子沿著太陽赤道形成。這些太陽黑子和活動出現在太陽的南半球,在此之前,大部分活動都發生在北半球。
Credit: NASA/SDO/HMI credit link

License: PD Public Domain icons

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