{"version":3,"sources":["webpack:///./src/data/phenomena/en/sunspots.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","target","rel","controls","type"],"mappings":"iGAAAA,EAAAC,QAAA,CACAC,KAAA,ktCACAC,KAAA,85CACAC,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,cAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAJ,EAAAQ,GAAA,iVAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,OAA0aK,MAAA,CAAOC,IAAA,4BAAAC,IAAA,kBAAwDX,EAAAQ,GAAA,KAAAJ,EAAA,MAAAJ,EAAAQ,GAAA,wGAAAJ,EAAA,KAA8IK,MAAA,CAAOG,KAAA,mCAAAC,OAAA,SAAAC,IAAA,iCAAkG,CAAAd,EAAAQ,GAAA,UAAAR,EAAAQ,GAAA,SAAAR,EAAAQ,GAAA,KAAAJ,EAAA,MAAAJ,EAAAQ,GAAA,iBAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAJ,EAAAQ,GAAA,2NAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,OAAoWK,MAAA,CAAOC,IAAA,0BAAAC,IAAA,sBAA0DX,EAAAQ,GAAA,KAAAJ,EAAA,MAAAJ,EAAAQ,GAAA,yBAAAJ,EAAA,KAA+DK,MAAA,CAAOG,KAAA,uBAAAC,OAAA,SAAAC,IAAA,iCAAsF,CAAAd,EAAAQ,GAAA,uDAAAR,EAAAQ,GAAA,KAAAJ,EAAA,SAAwFK,MAAA,CAAOM,SAAA,KAAe,CAAAX,EAAA,UAAeK,MAAA,CAAOC,IAAA,uCAAAM,KAAA,eAAiEhB,EAAAQ,GAAA,sDAAAR,EAAAQ,GAAA,KAAAJ,EAAA,KAAAA,EAAA,MAAAJ,EAAAQ,GAAA","file":"js/chunk-2d0ab538.04ab4349.js","sourcesContent":["module.exports = { \n    body: \"# Sunspots\\n\\nSunspots are dark areas on the Sun's surface with relatively low temperatures (compared with other parts of the sun) and strong magnetic fields. They normally appear in groups. The number of sunspots is usually taken as an indicator of solar activity. It increases significantly and can reach hundreds at the peak of a solar cycle.\\n\\n![0319_sunspot](./static/0319_sunspot.png)\\n*A huge sunspot group may cover an area 13 times or more the Earth's entire surface (Source/Credits: [SOHO](https://sohowww.nascom.nasa.gov/))*\\n\\n# Solar Cycle\\n\\nSolar activity is periodic. A solar cycle (also called a sunspot cycle) is an approximately 11-year period with increasing and decreasing sunspot numbers. Each cycle starts from the time of minimum solar activity. \\n\\n![0319_solar_cycle](./static/0319_cycle.png)\\n*Solar cycle (Source: [SILSO, Royal Observatory of Belgium, Brussels](http://sidc.be/silso)*\\n\\n<video controls>\\n  <source src=\\\"./videos/sun_magnetic_field@nasa.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n\\n*This visualization represents the constant changing of the sun’s magnetic field over the course of four years. (Credit: NASA's Scientific Visualization Studio)*\\n\",\n    html: \"<h1>Sunspots</h1>\\n<p>Sunspots are dark areas on the Sun’s surface with relatively low temperatures (compared with other parts of the sun) and strong magnetic fields. They normally appear in groups. The number of sunspots is usually taken as an indicator of solar activity. It increases significantly and can reach hundreds at the peak of a solar cycle.</p>\\n<p><img src=\\\"./static/0319_sunspot.png\\\" alt=\\\"0319_sunspot\\\">\\n<em>A huge sunspot group may cover an area 13 times or more the Earth’s entire surface (Source/Credits: <a href=\\\"https://sohowww.nascom.nasa.gov/\\\" target=\\\"_blank\\\" rel=\\\"noopener noreferrer nofollow\\\">SOHO</a>)</em></p>\\n<h1>Solar Cycle</h1>\\n<p>Solar activity is periodic. A solar cycle (also called a sunspot cycle) is an approximately 11-year period with increasing and decreasing sunspot numbers. Each cycle starts from the time of minimum solar activity.</p>\\n<p><img src=\\\"./static/0319_cycle.png\\\" alt=\\\"0319_solar_cycle\\\">\\n<em>Solar cycle (Source: <a href=\\\"http://sidc.be/silso\\\" target=\\\"_blank\\\" rel=\\\"noopener noreferrer nofollow\\\">SILSO, Royal Observatory of Belgium, Brussels</a></em></p>\\n<video controls>\\n  <source src=\\\"./videos/sun_magnetic_field@nasa.mp4\\\" type=\\\"video/mp4\\\">\\n  Your browser does not support HTML5 video.\\n</video>\\n<p><em>This visualization represents the constant changing of the sun’s magnetic field over the course of four years. (Credit: NASA’s Scientific Visualization Studio)</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(\\\"Sunspots\\\")]),_vm._v(\\\" \\\"),_c('p',[_vm._v(\\\"Sunspots are dark areas on the Sun’s surface with relatively low temperatures (compared with other parts of the sun) and strong magnetic fields. They normally appear in groups. The number of sunspots is usually taken as an indicator of solar activity. It increases significantly and can reach hundreds at the peak of a solar cycle.\\\")]),_vm._v(\\\" \\\"),_c('p',[_c('img',{attrs:{\\\"src\\\":\\\"./static/0319_sunspot.png\\\",\\\"alt\\\":\\\"0319_sunspot\\\"}}),_vm._v(\\\" \\\"),_c('em',[_vm._v(\\\"A huge sunspot group may cover an area 13 times or more the Earth’s entire surface (Source/Credits: \\\"),_c('a',{attrs:{\\\"href\\\":\\\"https://sohowww.nascom.nasa.gov/\\\",\\\"target\\\":\\\"_blank\\\",\\\"rel\\\":\\\"noopener noreferrer nofollow\\\"}},[_vm._v(\\\"SOHO\\\")]),_vm._v(\\\")\\\")])]),_vm._v(\\\" \\\"),_c('h1',[_vm._v(\\\"Solar Cycle\\\")]),_vm._v(\\\" \\\"),_c('p',[_vm._v(\\\"Solar activity is periodic. A solar cycle (also called a sunspot cycle) is an approximately 11-year period with increasing and decreasing sunspot numbers. Each cycle starts from the time of minimum solar activity.\\\")]),_vm._v(\\\" \\\"),_c('p',[_c('img',{attrs:{\\\"src\\\":\\\"./static/0319_cycle.png\\\",\\\"alt\\\":\\\"0319_solar_cycle\\\"}}),_vm._v(\\\" \\\"),_c('em',[_vm._v(\\\"Solar cycle (Source: \\\"),_c('a',{attrs:{\\\"href\\\":\\\"http://sidc.be/silso\\\",\\\"target\\\":\\\"_blank\\\",\\\"rel\\\":\\\"noopener noreferrer nofollow\\\"}},[_vm._v(\\\"SILSO, Royal Observatory of Belgium, Brussels\\\")])])]),_vm._v(\\\" \\\"),_c('video',{attrs:{\\\"controls\\\":\\\"\\\"}},[_c('source',{attrs:{\\\"src\\\":\\\"./videos/sun_magnetic_field@nasa.mp4\\\",\\\"type\\\":\\\"video/mp4\\\"}}),_vm._v(\\\"\\\\n  Your browser does not support HTML5 video.\\\\n\\\")]),_vm._v(\\\" \\\"),_c('p',[_c('em',[_vm._v(\\\"This visualization represents the constant changing of the sun’s magnetic field over the course of four years. (Credit: NASA’s Scientific Visualization Studio)\\\")])])]) }]\",\n        component: {\n          data: function () {\n            return {\n              templateRender: null\n            }\n          },\n          render: function (createElement) {\n            return this.templateRender ? this.templateRender() : createElement(\"div\", \"Rendering\");\n          },\n          created: function () {\n            this.templateRender = function render() { var _vm=this;var _h=_vm.$createElement;var _c=_vm._self._c||_h;return _vm._m(0) };\n            this.$options.staticRenderFns = [function () { var _vm=this;var _h=_vm.$createElement;var _c=_vm._self._c||_h;return _c('div',{staticClass:\"markdown-body\"},[_c('h1',[_vm._v(\"Sunspots\")]),_vm._v(\" \"),_c('p',[_vm._v(\"Sunspots are dark areas on the Sun’s surface with relatively low temperatures (compared with other parts of the sun) and strong magnetic fields. They normally appear in groups. The number of sunspots is usually taken as an indicator of solar activity. It increases significantly and can reach hundreds at the peak of a solar cycle.\")]),_vm._v(\" \"),_c('p',[_c('img',{attrs:{\"src\":\"./static/0319_sunspot.png\",\"alt\":\"0319_sunspot\"}}),_vm._v(\" \"),_c('em',[_vm._v(\"A huge sunspot group may cover an area 13 times or more the Earth’s entire surface (Source/Credits: \"),_c('a',{attrs:{\"href\":\"https://sohowww.nascom.nasa.gov/\",\"target\":\"_blank\",\"rel\":\"noopener noreferrer nofollow\"}},[_vm._v(\"SOHO\")]),_vm._v(\")\")])]),_vm._v(\" \"),_c('h1',[_vm._v(\"Solar Cycle\")]),_vm._v(\" \"),_c('p',[_vm._v(\"Solar activity is periodic. A solar cycle (also called a sunspot cycle) is an approximately 11-year period with increasing and decreasing sunspot numbers. Each cycle starts from the time of minimum solar activity.\")]),_vm._v(\" \"),_c('p',[_c('img',{attrs:{\"src\":\"./static/0319_cycle.png\",\"alt\":\"0319_solar_cycle\"}}),_vm._v(\" \"),_c('em',[_vm._v(\"Solar cycle (Source: \"),_c('a',{attrs:{\"href\":\"http://sidc.be/silso\",\"target\":\"_blank\",\"rel\":\"noopener noreferrer nofollow\"}},[_vm._v(\"SILSO, Royal Observatory of Belgium, Brussels\")])])]),_vm._v(\" \"),_c('video',{attrs:{\"controls\":\"\"}},[_c('source',{attrs:{\"src\":\"./videos/sun_magnetic_field@nasa.mp4\",\"type\":\"video/mp4\"}}),_vm._v(\"\\n  Your browser does not support HTML5 video.\\n\")]),_vm._v(\" \"),_c('p',[_c('em',[_vm._v(\"This visualization represents the constant changing of the sun’s magnetic field over the course of four years. (Credit: NASA’s Scientific Visualization Studio)\")])])]) }];\n          }\n        }\n      }\n     }"],"sourceRoot":""}