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46億年 |\\n\\n\\n\\n*太陽Hα圖像 (來源︰中國氣象局國家衛星氣象中心)*\\n\\n## 日冕\\n\\n我們的太陽由「大氣層」包圍著。日冕就是太陽的大氣層最外圍部分。日冕通常被太陽表面的強光所掩蓋,因此難以觀察,除非利用特別儀器。不過,當有日全蝕時,便可觀察到日冕。\\n\\n\\n*在2017年8月21日的日全蝕,太陽的日冕被觀察到。(來源︰ 美國太空總署/Carla Thomas)*\\n\\n雖然日冕遠離太陽表面,但它溫度極高,並比太陽的表面熱幾百倍。然而,日冕看起來很暗,這是因為日冕的密度比太陽的表面低千萬倍。日冕遠伸至太空。它產生吹過我們太陽系的太陽風。日冕的高溫令它的粒子很高速地移動,使它們能脫離太陽的引力。\\n\\n## 冕洞\\n\\n\\n*(來源︰美國太空總署)*\\n\\n冕洞是**日冕**中**較冷**和**密度較低**的地方,常見於**太陽活動極小期**。我們可以從X射線影像圖中看到它們。\\n\\n## 什麼是太空天氣?\\n\\n太空天氣源自太陽。它普遍是指一切太陽活動,例如太陽黑子、太陽耀斑及太陽風等,以及其為地球帶來的影響。\\n\\n## 太陽怎樣產生太空天氣?\\n\\n要了解太空天氣,我們首先要知道在太陽上發生什麼。太陽有各種現象,都與太空天氣密切相關。讓我們先看看太陽帶來什麼現象 - 現象。\\n\\n---\\n\\n資料來源:\\n\\n- [美國太空總署NASA](
太陽是在太陽系中心的恆星,它驅動地球大氣的循環,亦是地球能源的主要源頭。它源源不絕地給予植物能量以製造食物和氧氣,從而孕育地球上的生命。太陽同時亦會引致大部分的太空天氣現象。
\\n\\n | \\n |
---|---|
半徑 | \\n~ 696,000公里 (約地球半徑的109倍) | \\n
距離地球 | \\n~ 1.5×108公里 (即150百萬公里) | \\n
光度 | \\n~ 3.8 x 1026瓦特 | \\n
平均表面溫度 | \\n~ 5,500攝氏度 (°C) | \\n
質量 | \\n~ 2 x 1030 公斤(kg) (約地球質量的300,000倍) | \\n
化學構造 | \\n氫(~71%),氦(~27%),重元素(~2%) (以質量計) | \\n
年齡 | \\n~ 45 - 46億年 | \\n
\\n太陽Hα圖像 (來源︰中國氣象局國家衛星氣象中心)
我們的太陽由「大氣層」包圍著。日冕就是太陽的大氣層最外圍部分。日冕通常被太陽表面的強光所掩蓋,因此難以觀察,除非利用特別儀器。不過,當有日全蝕時,便可觀察到日冕。
\\n\\n在2017年8月21日的日全蝕,太陽的日冕被觀察到。(來源︰ 美國太空總署/Carla Thomas)
雖然日冕遠離太陽表面,但它溫度極高,並比太陽的表面熱幾百倍。然而,日冕看起來很暗,這是因為日冕的密度比太陽的表面低千萬倍。日冕遠伸至太空。它產生吹過我們太陽系的太陽風。日冕的高溫令它的粒子很高速地移動,使它們能脫離太陽的引力。
\\n\\n(來源︰美國太空總署)
冕洞是日冕中較冷和密度較低的地方,常見於太陽活動極小期。我們可以從X射線影像圖中看到它們。
\\n太空天氣源自太陽。它普遍是指一切太陽活動,例如太陽黑子、太陽耀斑及太陽風等,以及其為地球帶來的影響。
\\n要了解太空天氣,我們首先要知道在太陽上發生什麼。太陽有各種現象,都與太空天氣密切相關。讓我們先看看太陽帶來什麼現象 - 現象。
\\n資料來源:
\\n