{"id":1503,"date":"2026-08-11T16:00:00","date_gmt":"2026-08-11T14:00:00","guid":{"rendered":"https:\/\/infoimasd.com\/?p=1503"},"modified":"2026-08-12T11:15:41","modified_gmt":"2026-08-12T09:15:41","slug":"eclipse-solar-12-agosto-2026-yebes","status":"publish","type":"post","link":"https:\/\/infoimasd.com\/index.php\/2026\/08\/11\/eclipse-solar-12-agosto-2026-yebes\/","title":{"rendered":"Eclipse solar hist\u00f3rico: tambi\u00e9n puedes verlo con las se\u00f1ales del Observatorio de Yebes"},"content":{"rendered":"\n

El Gobierno de Espa\u00f1a ofrecer\u00e1 a trav\u00e9s de Radiotelevisi\u00f3n Espa\u00f1ola (RTVE) dos se\u00f1ales institucionales de v\u00eddeo del disco solar captadas desde el Observatorio de Yebes (Guadalajara) durante el eclipse total de Sol<\/a>. <\/strong>Las im\u00e1genes estar\u00e1n disponibles para los medios de comunicaci\u00f3n y mostrar\u00e1n distintos fen\u00f3menos solares mediante dos t\u00e9cnicas de observaci\u00f3n complementarias.<\/p>\n\n\n\n

RTVE distribuir\u00e1 adem\u00e1s las dos se\u00f1ales a las televisiones integrantes de la Uni\u00f3n Europea de Radiodifusi\u00f3n (EBU)<\/strong> que agrupa a 69 radiotelevisiones de 57 pa\u00edses. Las emisiones tambi\u00e9n podr\u00e1n seguirse a trav\u00e9s de la web oficial trioeclipses.es<\/a> y del canal de YouTube del Ministerio de Ciencia, Innovaci\u00f3n y Universidades.<\/a><\/p>\n\n\n\n

Las dos se\u00f1ales utilizar\u00e1n filtros espec\u00edficos para reducir la radiaci\u00f3n solar y permitir una observaci\u00f3n segura.<\/strong> Una de ellas emplear\u00e1 un filtro de luz blanca, mientras que la segunda utilizar\u00e1 un filtro H-alfa. Cada sistema permitir\u00e1 observar fen\u00f3menos diferentes de la actividad solar. La observaci\u00f3n directa del Sol mediante telescopios puede provocar da\u00f1os tanto en los ojos como en los equipos. Por ello, los instrumentos deber\u00e1n utilizar filtros adecuados. Durante la fase de totalidad, cuando la Luna cubra por completo el disco solar, la corona podr\u00e1 observarse a simple vista sin filtros.<\/p>\n\n\n\n

La se\u00f1al en luz blanca mostrar\u00e1 las manchas solares y la corona<\/h3>\n\n\n\n

La primera se\u00f1al se obtendr\u00e1 desde la Torre Solar del Observatorio de Yebes mediante un telescopio equipado con un filtro de densidad neutra o de luz blanca. <\/strong>Este sistema bloquea la inmensa mayor\u00eda de la radiaci\u00f3n solar y deja pasar aproximadamente una cienmil\u00e9sima parte de la luz. Esta t\u00e9cnica permitir\u00e1 observar las manchas solares<\/strong>. Son regiones de la superficie del Sol m\u00e1s fr\u00edas que su entorno y est\u00e1n relacionadas con una intensa actividad magn\u00e9tica. Estas estructuras pueden crecer, fragmentarse y desaparecer a lo largo de horas o d\u00edas.<\/p>\n\n\n\n

El filtro podr\u00e1 retirarse durante la totalidad del eclipse. As\u00ed, la se\u00f1al permitir\u00e1 captar la sucesi\u00f3n de fen\u00f3menos que acompa\u00f1a al segundo contacto. Primero aparecer\u00e1 el denominado anillo de diamantes y despu\u00e9s las perlas de Baily. Durante la totalidad ser\u00e1 visible la corona solar, la capa m\u00e1s externa de la atm\u00f3sfera del Sol. Tras el tercer contacto, estos fen\u00f3menos aparecer\u00e1n de nuevo en sentido inverso. La corona desaparecer\u00e1 y volver\u00e1n a observarse las perlas de Baily y el anillo de diamantes. Despu\u00e9s se reinstalar\u00e1 el filtro para continuar la observaci\u00f3n segura del eclipse.<\/p>\n\n\n\n

El canal H-alfa permitir\u00e1 observar las protuberancias solares<\/h3>\n\n\n\n

La segunda se\u00f1al se captar\u00e1 simult\u00e1neamente desde un telescopio Lunt instalado en la azotea del edificio principal del Observatorio de Yebes. <\/strong>En este caso se utilizar\u00e1 un filtro H-alfa, que permite observar una longitud de onda concreta correspondiente al hidr\u00f3geno: 656,3 nan\u00f3metros.<\/p>\n\n\n\n

El resultado ser\u00e1 una imagen dominada por el color rojo<\/strong>. Esta t\u00e9cnica permitir\u00e1 identificar estructuras que no se distinguen de la misma forma mediante luz blanca. Entre ellas destacan las protuberancias solares, grandes estructuras de gas que emergen desde la atm\u00f3sfera del Sol y pueden formar arcos y bucles.<\/p>\n\n\n\n

Durante la totalidad, estas estructuras podr\u00e1n aparecer como peque\u00f1os arcos rojizos alrededor del contorno de la Luna. Algunas pueden alcanzar dimensiones que van desde el tama\u00f1o de la Tierra hasta extensiones comparables al di\u00e1metro de J\u00fapiter. La observaci\u00f3n H-alfa tambi\u00e9n permitir\u00e1 distinguir filamentos, playas solares y la textura granulada de la superficie solar. <\/strong>Sin embargo, su filtro no podr\u00e1 retirarse durante la totalidad. Por ello, la corona tendr\u00e1 una presencia mucho menor en esta segunda se\u00f1al.<\/p>\n\n\n\n

RTVE distribuir\u00e1 la se\u00f1al a medios de todo el mundo<\/h3>\n\n\n\n

Las dos se\u00f1ales estar\u00e1n disponibles en directo para televisiones, medios digitales y agencias de noticias. RTVE realizar\u00e1 la distribuci\u00f3n mediante conmutaci\u00f3n con Torrespa\u00f1a. Los medios digitales dispondr\u00e1n tambi\u00e9n de alternativas mediante c\u00f3digo embebible de rtve.es o YouTube de RTVE. De esta manera, las im\u00e1genes obtenidas desde el Observatorio de Yebes podr\u00e1n incorporarse a las coberturas informativas del eclipse.<\/a> El dispositivo permitir\u00e1 mostrar desde Espa\u00f1a y al p\u00fablico internacional tanto la corona solar durante la totalidad como las diferentes estructuras de la actividad del Sol observadas mediante H-alfa.<\/strong><\/p>\n\n\n\n

<\/p>\n","protected":false},"excerpt":{"rendered":"

El Observatorio de Yebes ofrecer\u00e1 dos se\u00f1ales institucionales del eclipse total de Sol del 12 de agosto de 2026. Las im\u00e1genes permitir\u00e1n observar la corona solar, las manchas y las protuberancias mediante t\u00e9cnicas de luz blanca y H-alfa.<\/p>\n","protected":false},"author":1,"featured_media":1505,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_newsletter_access":"","_jetpack_dont_email_post_to_subs":false,"_jetpack_newsletter_tier_id":0,"_jetpack_memberships_contains_paywalled_content":false,"_jetpack_feature_clip_id":0,"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_post_was_ever_published":false},"categories":[375],"tags":[583,637,635,582,636],"class_list":["post-1503","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-eventos","tag-astronomia","tag-ciencia-solar","tag-eclipse-12-agosto-2026","tag-eclipse-solar","tag-observatorio-de-yebes"],"yoast_head":"\nEclipse solar hist\u00f3rico: tambi\u00e9n puedes verlo con las se\u00f1ales del Observatorio de Yebes - 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