{"id":69676,"date":"2007-07-10T02:03:00","date_gmt":"2007-07-10T02:03:00","guid":{"rendered":"http:\/\/weblogs.madrimasd.org\/\/astrofisica\/archive\/2007\/07\/10\/69676.aspx"},"modified":"2014-04-25T08:55:08","modified_gmt":"2014-04-25T07:55:08","slug":"manchas-solares","status":"publish","type":"post","link":"https:\/\/www.madrimasd.org\/blogs\/astrofisica\/2007\/07\/10\/69676","title":{"rendered":"Manchas Solares"},"content":{"rendered":"<div align=\"justify\">David ByNEl Sol, aunque no lo parezca, presenta una fenomenolog\u00eda bastante compleja: desde sus<a href=\"http:\/\/weblogs.madrimasd.org\/astrofisica\/archive\/2007\/05\/17\/65737.aspx\"> propias tormentas<\/a>, que afectan a nuestro planeta, hasta la aparici\u00f3n y desaparici\u00f3n c\u00edclica de caracteristicas superficiales, entre las que destacan las manchas.<\/p>\n<\/div>\n<p><!--more--><\/p>\n<div align=\"justify\">En realidad, el Sol presenta un ciclo de actividad de unos 11 a\u00f1os (22 si se tiene en cuenta el cambio de la polaridad magn\u00e9tica). Hace <a href=\"http:\/\/weblogs.madrimasd.org\/astrofisica\/archive\/2006\/12\/08\/54422.aspx\">un a\u00f1o aproximadamente pasamos por el m\u00ednimo<\/a> y el n\u00famero de manchas se incrementa poco a poco. Recientemente ha aparecido un conjunto de ellas con una estructura muy interesante. A continuaci\u00f3n adjuntamos una foto, junto con <a href=\"http:\/\/spaceweather.com\/swpod2007\/08jul07\/alvarez1_strip.gif\">un video que muestra el limbo solar<\/a>.<\/div>\n<p><img decoding=\"async\" src=\"http:\/\/laeff.cab.inta-csic.es\/users\/barrado\/weblog\/SunSpot0963_GValentini-NOAA.jpg\" alt=\"\" \/><br \/>\n<em>La mancha solar 963. Se aprecia claramente la umbra y la penumbra.<\/em><\/p>\n<p>M\u00e1s im\u00e1genes del Sol se pueden encontrar en <a href=\"http:\/\/umbra.nascom.nasa.gov\/images\/latest.html\">este enlace<\/a> gen\u00e9rico (<a href=\"http:\/\/www.sec.noaa.gov\/solar_sites.html\">m\u00e1s aqu\u00ed<\/a>)\u00a0 o en la <a href=\"http:\/\/sohowww.nascom.nasa.gov\/gallery\/\">p\u00e1gina del sat\u00e9lite SOHO<\/a>.<\/p>\n<p>PD: Recordemos que <span style=\"color: #ff0000;\"><strong>NUNCA<\/strong><\/span> debe mirarse el Sol directamente. Se requiere instrumentaci\u00f3n espec\u00edfica que proteja adecuadamente el ojo. M\u00e1s informaci\u00f3n <a href=\"http:\/\/weblogs.madrimasd.org\/astrofisica\/archive\/2006\/10\/29\/48455.aspx\">aqu\u00ed<\/a>, al final de la entrada.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>David ByNEl Sol, aunque no lo parezca, presenta una fenomenolog\u00eda bastante compleja: desde sus propias tormentas, que afectan a nuestro planeta, hasta la aparici\u00f3n y desaparici\u00f3n c\u00edclica de caracteristicas superficiales, entre las que destacan las manchas.<\/p>\n","protected":false},"author":32,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0},"categories":[64,558,553],"tags":[],"blocksy_meta":{"styles_descriptor":{"styles":{"desktop":"","tablet":"","mobile":""},"google_fonts":[],"version":4}},"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 4.9.9 - aioseo.com -->\n\t<meta name=\"description\" content=\"David ByNEl Sol, aunque no lo parezca, presenta una fenomenolog\u00eda bastante compleja: desde sus propias tormentas, que afectan a nuestro planeta, hasta la aparici\u00f3n y desaparici\u00f3n c\u00edclica de caracteristicas superficiales, entre las que destacan las manchas. 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