{"version":3,"sources":["webpack:///./src/data/phenomena/en/earth-magnetosphere.md"],"names":["module","exports","body","html","attributes","vue","render","staticRenderFns","component","data","templateRender","createElement","this","created","_vm","_h","$createElement","_self","_c","_m","$options","staticClass","_v","attrs","src","alt","href","controls","type"],"mappings":"mGAAAA,EAAAC,QAAA,CACAC,KAAA,qzCACAC,KAAA,06CACAC,WAAA,GACAC,IAAA,CACAC,OAAA,+GACAC,gBAAA,65DACAC,UAAA,CACAC,KAAA,WACA,OACAC,eAAA,OAGAJ,OAAA,SAAAK,GACA,OAAAC,KAAAF,eAAAE,KAAAF,iBAAAC,EAAA,oBAEAE,QAAA,WACAD,KAAAF,eAAA,WAAqD,IAAAI,EAAAF,KAAcG,EAAAD,EAAAE,eAA0BF,EAAAG,MAAAC,GAAwB,OAAAJ,EAAAK,GAAA,IACrHP,KAAAQ,SAAAb,gBAAA,YAA0D,IAAAO,EAAAF,KAAcG,EAAAD,EAAAE,eAA0BE,EAAAJ,EAAAG,MAAAC,IAAAH,EAAwB,OAAAG,EAAA,OAAiBG,YAAA,iBAA4B,CAAAH,EAAA,MAAAJ,EAAAQ,GAAA,2BAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,OAA2EK,MAAA,CAAOC,IAAA,4BAAAC,IAAA,mBAAyDX,EAAAQ,GAAA,KAAAJ,EAAA,MAAAJ,EAAAQ,GAAA,sBAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAJ,EAAAQ,GAAA,kGAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,oBAAAR,EAAAQ,GAAA,oCAAAJ,EAAA,KAA4QK,MAAA,CAAOG,KAAA,6BAAmC,CAAAZ,EAAAQ,GAAA,gBAAAR,EAAAQ,GAAA,4HAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,2BAAAR,EAAAQ,GAAA,kEAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,sBAAAR,EAAAQ,GAAA,4KAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,qBAAAR,EAAAQ,GAAA,sEAAAJ,EAAA,UAAAJ,EAAAQ,GAAA,mBAAAR,EAAAQ,GAAA,OAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAJ,EAAAQ,GAAA,sKAAAR,EAAAQ,GAAA,KAAAJ,EAAA,SAAq3BK,MAAA,CAAOI,SAAA,KAAe,CAAAT,EAAA,UAAeK,MAAA,CAAOC,IAAA,8BAAAI,KAAA,eAAwDd,EAAAQ,GAAA,sDAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,MAAAJ,EAAAQ,GAAA","file":"js/chunk-2d0b327e.f991cb4a.js","sourcesContent":["module.exports = { \n    body: \"# Earth's Magnetosphere\\n\\n![Magnetosphere](./static/earth_mag_en.png)\\n*(Source: NASA)*\\n\\nThe flow of molten iron in Earth’s core generates electric currents, which in turn produces a **magnetic field**.  Through interaction with the <a href=\\\"#/en/phenomena/solarwind\\\">solar wind</a>, this magnetic field forms a shield for Earth known as the magnetosphere. The magnetosphere protects us from the Sun’s **ultraviolet radiation**, as well as energetic particles everywhere in space known as **cosmic radiation**.  Instead of penetrating directly into Earth’s surface, the charged particles hitting the shield (magnetosphere) mostly flow around and get trapped in a region called **radiation belts**. A portion of them follow the magnetic field to move down to the **polar regions**.\\n\\nThe pressure of the solar wind on Earth’s magnetic field compresses the field on the dayside of Earth and stretches the field into a long tail on the nightside.\\n\\n<video controls>\\n  <source src=\\\"./videos/magnetic_field.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n\\n*This animation shows how coronal mass ejections can blow out from the Sun, interfere with Earth’s magnetic fields (the curved purple lines), and cause auroras (the blue rings of light circling the North and South poles). (Credit: NASA)*\\n\",\n    html: \"<h1>Earth’s Magnetosphere</h1>\\n<p><img src=\\\"./static/earth_mag_en.png\\\" alt=\\\"Magnetosphere\\\">\\n<em>(Source: NASA)</em></p>\\n<p>The flow of molten iron in Earth’s core generates electric currents, which in turn produces a <strong>magnetic field</strong>.  Through interaction with the <a href=\\\"#/en/phenomena/solarwind\\\">solar wind</a>, this magnetic field forms a shield for Earth known as the magnetosphere. The magnetosphere protects us from the Sun’s <strong>ultraviolet radiation</strong>, as well as energetic particles everywhere in space known as <strong>cosmic radiation</strong>.  Instead of penetrating directly into Earth’s surface, the charged particles hitting the shield (magnetosphere) mostly flow around and get trapped in a region called <strong>radiation belts</strong>. A portion of them follow the magnetic field to move down to the <strong>polar regions</strong>.</p>\\n<p>The pressure of the solar wind on Earth’s magnetic field compresses the field on the dayside of Earth and stretches the field into a long tail on the nightside.</p>\\n<video controls>\\n  <source src=\\\"./videos/magnetic_field.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n<p><em>This animation shows how coronal mass ejections can blow out from the Sun, interfere with Earth’s magnetic fields (the curved purple lines), and cause auroras (the blue rings of light circling the North and South poles). (Credit: NASA)</em></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(\\\"Earth’s Magnetosphere\\\")]),_vm._v(\\\" \\\"),_c('p',[_c('img',{attrs:{\\\"src\\\":\\\"./static/earth_mag_en.png\\\",\\\"alt\\\":\\\"Magnetosphere\\\"}}),_vm._v(\\\" \\\"),_c('em',[_vm._v(\\\"(Source: NASA)\\\")])]),_vm._v(\\\" \\\"),_c('p',[_vm._v(\\\"The flow of molten iron in Earth’s core generates electric currents, which in turn produces a \\\"),_c('strong',[_vm._v(\\\"magnetic field\\\")]),_vm._v(\\\".  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