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= { \n    body: \"# 極光\\n\\n<video controls loop autoplay>\\n  <source src=\\\"./videos/shunchiming.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n\\n*挪威特羅姆瑟的極光<br>(攝影： 香港天文台台長岑智明)*\\n\\n太空天氣不一定是壞事。它可以製造名為極光的美麗現象!**太陽風**從太陽帶來**帶電粒子**（主要是電子）。它們跟隨地球的磁場向下移至**極地**，並在那裡與地球大氣上層中的**氧**和**氮**的原子和分子碰撞。**氧**會釋出**綠或紅**光，而**氮**則釋出**藍及紫**光。\\n\\n![0306_aurora_2](./static/0306_aurora_2.png)\\n*(來源: 美國太空總署)*\\n\\n我們在約60至75度的高緯度地區最大機會觀賞到極光，例如在北歐和加拿大。當<a href=\\\"#/zh/phenomena/geomagnetic-storms\\\">地磁暴</a>發生時，極光區域向赤道擴展，因此甚至在較低緯度都可以看得到！\\n\",\n    html: \"<h1>極光</h1>\\n<video controls loop autoplay>\\n  <source src=\\\"./videos/shunchiming.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n<p><em>挪威特羅姆瑟的極光<br>(攝影： 香港天文台台長岑智明)</em></p>\\n<p>太空天氣不一定是壞事。它可以製造名為極光的美麗現象!<strong>太陽風</strong>從太陽帶來<strong>帶電粒子</strong>（主要是電子）。它們跟隨地球的磁場向下移至<strong>極地</strong>，並在那裡與地球大氣上層中的<strong>氧</strong>和<strong>氮</strong>的原子和分子碰撞。<strong>氧</strong>會釋出<strong>綠或紅</strong>光，而<strong>氮</strong>則釋出<strong>藍及紫</strong>光。</p>\\n<p><img src=\\\"./static/0306_aurora_2.png\\\" alt=\\\"0306_aurora_2\\\">\\n<em>(來源: 美國太空總署)</em></p>\\n<p>我們在約60至75度的高緯度地區最大機會觀賞到極光，例如在北歐和加拿大。當<a href=\\\"#/zh/phenomena/geomagnetic-storms\\\">地磁暴</a>發生時，極光區域向赤道擴展，因此甚至在較低緯度都可以看得到！</p>\\n\",\n    attributes: {},\n      vue: {\n        render: \"return function render() { var _vm=this;var _h=_vm.$createElement;var _c=_vm._self._c||_h;return _vm._m(0) }\",\n        staticRenderFns: \"return [function () { var _vm=this;var _h=_vm.$createElement;var _c=_vm._self._c||_h;return _c('div',{staticClass:\\\"markdown-body\\\"},[_c('h1',[_vm._v(\\\"極光\\\")]),_vm._v(\\\" 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