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CMEs are also formed by reorganization of the Sun’s magnetic field lines.  They consist of energetic **charged particles** which travel at high speed, taking about 15-18 hours to several days to reach our planet.\\n\\n<video controls>\\n  <source src=\\\"./videos/CME_eruption.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n\\n*Coronal Mass Ejections (Source: NASA/SDO)*\\n\",\n    html: \"<h1>Coronal Mass Ejections (CME)</h1>\\n<p><img src=\\\"./static/0306_cme.jpg\\\" alt=\\\"0306_cme\\\">\\n<em>Coronal Mass Ejections (Source:  Solar Dynamics Observatory)</em></p>\\n<p>Solar flares are sometimes accompanied by coronal mass ejections (CMEs).  CMEs are also formed by reorganization of the Sun’s magnetic field lines.  They consist of energetic <strong>charged particles</strong> which travel at high speed, taking about 15-18 hours to several days to reach our planet.</p>\\n<video controls>\\n  <source src=\\\"./videos/CME_eruption.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n<p><em>Coronal Mass Ejections (Source: NASA/SDO)</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(\\\"Coronal Mass Ejections (CME)\\\")]),_vm._v(\\\" \\\"),_c('p',[_c('img',{attrs:{\\\"src\\\":\\\"./static/0306_cme.jpg\\\",\\\"alt\\\":\\\"0306_cme\\\"}}),_vm._v(\\\" \\\"),_c('em',[_vm._v(\\\"Coronal Mass Ejections (Source:  Solar Dynamics Observatory)\\\")])]),_vm._v(\\\" \\\"),_c('p',[_vm._v(\\\"Solar flares are sometimes accompanied by coronal mass ejections (CMEs).  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