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本節目深入探討了太陽黑子的奧秘，將其比作太陽表面的「雀斑」，並解釋了它們之所以看起來暗淡，是因為其溫度遠低於周圍的光球層。文中詳細闡述了太陽黑子的形成與演化，指出它們是太陽內部強烈磁活動的直接體現，由扭曲纏繞的磁力線「刺穿」表面並抑制熱傳導所致。此外，節目還介紹了太陽黑子的物理特性、結構以及令人著迷的11年活動週期，並提及了觀測歷史、蒙德極小期及其與地球氣候的可能聯繫，展現了對這些太陽現象的全面理解。 -- Hosting provided by SoundOn
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