{"id":24023,"date":"2021-08-12T09:47:30","date_gmt":"2021-08-12T15:47:30","guid":{"rendered":"https:\/\/otech.uaeh.edu.mx\/noti\/?p=24023"},"modified":"2021-08-12T09:47:40","modified_gmt":"2021-08-12T15:47:40","slug":"el-sol-esta-oscilando-a-5-kilometros-por-hora","status":"publish","type":"post","link":"https:\/\/otech.uaeh.edu.mx\/noti\/ciencia\/el-sol-esta-oscilando-a-5-kilometros-por-hora\/","title":{"rendered":"El Sol est\u00e1 oscilando a 5 kil\u00f3metros por hora"},"content":{"rendered":"<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">El Sol registra oscilaciones que se manifiestan en la superficie global como movimientos giratorios, con velocidades del orden de 5 kil\u00f3metros por hora. <\/span><span style=\"vertical-align: inherit;\">Un grupo de investigadores liderado por cient\u00edficos del\u00a0 <\/span><\/span><a style=\"color: #000000;\" href=\"https:\/\/www.mpg.de\/institutes\" target=\"_blank\" rel=\"noopener noreferrer\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Instituto Max Planck<\/span><\/span><\/a><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\"> \u00a0para la Investigaci\u00f3n del Sistema Solar y la\u00a0 <\/span><\/span><a style=\"color: #000000;\" href=\"https:\/\/www.uni-goettingen.de\/en\/1.html\" target=\"_blank\" rel=\"noopener noreferrer\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Universidad de G\u00f6ttingen<\/span><\/span><\/a><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\"> , en Alemania, ha concluido que las oscilaciones tienen su propia m\u00fasica: son modos resonantes y deben su existencia a la rotaci\u00f3n diferencial del Sol.<\/span><\/span><!--more--><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">De acuerdo a una nota de prensa, las oscilaciones ayudar\u00e1n a establecer formas novedosas de sondear el interior del Sol y obtener informaci\u00f3n sobre la estructura y la din\u00e1mica de nuestra estrella. <\/span><span style=\"vertical-align: inherit;\">Las oscilaciones descubiertas pertenecen a ciclos largos, similares al per\u00edodo de rotaci\u00f3n solar de 27 d\u00edas, y se diferencian de las oscilaciones ac\u00fasticas cortas, de alrededor de 5 minutos, que ya se hab\u00eda identificado seis d\u00e9cadas atr\u00e1s.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">El nuevo estudio, que ha sido publicado recientemente en la revista\u00a0 <\/span><\/span><a style=\"color: #000000;\" href=\"https:\/\/www.aanda.org\/\" target=\"_blank\" rel=\"noopener noreferrer\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Astronomy &amp; Astrophysics<\/span><\/span><\/a><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\"> , recoge diez a\u00f1os de datos obtenidos por el Observatorio de Din\u00e1mica Solar (SDO) de la\u00a0 <\/span><\/span><a style=\"color: #000000;\" href=\"https:\/\/www.nasa.gov\/\" target=\"_blank\" rel=\"noopener noreferrer\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">NASA<\/span><\/span><\/a><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\"> . <\/span><span style=\"vertical-align: inherit;\">Las observaciones permitieron medir los movimientos giratorios descubiertos en el Sol, una informaci\u00f3n que fue combinada con modelos num\u00e9ricos para caracterizar con mayor precisi\u00f3n el fen\u00f3meno.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><strong><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Notas graves y agudas<\/span><\/span><\/strong><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">La \u00abm\u00fasica\u00bb del Sol se expresa en diferentes tonalidades. <\/span><span style=\"vertical-align: inherit;\">Sobre la d\u00e9cada de 1960, los especialistas identificaron las \u00abnotas agudas\u00bb, relacionadas con oscilaciones cortas de alrededor de 5 minutos: aparecen a partir de turbulencias en la superficie solar y su energ\u00eda queda \u00abatrapada\u00bb en el interior de la estrella.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Estas vibraciones ac\u00fasticas, que han sido observadas en los \u00faltimos 30 a\u00f1os con diversos instrumentos, han permitido avanzar notablemente en el conocimiento de la estructura interna del Sol y en su din\u00e1mica. <\/span><span style=\"vertical-align: inherit;\">Sin embargo, al mismo tiempo se hab\u00eda postulado la existencia de oscilaciones que responden a ciclos m\u00e1s largos, y cuyo sonido evidencia las \u00abnotas m\u00e1s graves\u00bb del Sol.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Son precisamente las oscilaciones descubiertas en el nuevo estudio: se trata de movimientos de largo per\u00edodo que dependen de la rotaci\u00f3n del sol. <\/span><span style=\"vertical-align: inherit;\">No son de naturaleza ac\u00fastica, pero s\u00ed resonantes: al ser desplazadas al espectro audible, las variaciones de sonido en las oscilaciones informan sobre la activaci\u00f3n o cese de los movimientos.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><strong><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">En per\u00edodos prolongados<\/span><\/span><\/strong><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Como sucede al analizar los terremotos en la Tierra, los cient\u00edficos contar\u00e1n ahora con una nueva herramienta para descubrir m\u00e1s sobre el interior del Sol. <\/span><span style=\"vertical-align: inherit;\">Sin embargo, las oscilaciones durante per\u00edodos prolongados requieren la medici\u00f3n de los movimientos horizontales en la superficie del Sol a lo largo de muchos a\u00f1os. <\/span><span style=\"vertical-align: inherit;\">Esa informaci\u00f3n es la que obtuvo el SDO de la NASA, concretamente a trav\u00e9s del generador de im\u00e1genes magn\u00e9ticas y helios\u00edsmicas (HMI).<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Las oscilaciones en ciclos largos se manifiestan como movimientos de \u00abremolino\u00bb en la superficie del Sol, con velocidades m\u00e1s lentas con relaci\u00f3n a las oscilaciones cortas, que pueden asemejarse a la velocidad con la cual camina una persona promedio. <\/span><span style=\"vertical-align: inherit;\">Algunas de estas oscilaciones son m\u00e1s intensas en los polos solares, otras en latitudes medias y un tercer grupo alcanza un ritmo m\u00e1s pronunciado cerca del ecuador solar.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">En cuanto al impacto de este descubrimiento, los investigadores destacaron que el nuevo tipo de oscilaciones solares que se ha identificado y caracterizar pueden precisar al detalle la magnitud de algunas fuerzas y fen\u00f3menos, que parecen controlar la din\u00e1mica interna del Sol.<\/span><\/span><\/span><\/p>\n<p style=\"text-align: justify;\"><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">Fuente:\u00a0<\/span><\/span><\/span><\/p>\n<p><span style=\"color: #000000;\"><span style=\"vertical-align: inherit;\"><span style=\"vertical-align: inherit;\">M. (sf-d). <\/span><span style=\"vertical-align: inherit;\">El Sol est\u00e1 oscilando a 5 kil\u00f3metros por hora | <\/span><span style=\"vertical-align: inherit;\">madrimasd. <\/span><span style=\"vertical-align: inherit;\">Recuperado 12 de agosto de 2021, de http:\/\/www.madrimasd.org\/notiweb\/noticias\/sol-esta-oscilando-5-kilometros-por-hora<\/span><\/span><\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>El Sol registra oscilaciones que se manifiestan en la superficie global como movimientos giratorios, con velocidades del orden de 5 kil\u00f3metros por hora. Un grupo de investigadores liderado por cient\u00edficos del\u00a0 Instituto Max Planck \u00a0para la Investigaci\u00f3n del Sistema Solar y la\u00a0 Universidad de G\u00f6ttingen , en Alemania, ha concluido que las oscilaciones tienen su [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":24024,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[56],"tags":[],"class_list":["post-24023","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-ciencia"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v26.7 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>El Sol est\u00e1 oscilando a 5 kil\u00f3metros por hora - Observatorio Tecnol\u00f3gico de Hidalgo<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/otech.uaeh.edu.mx\/noti\/ciencia\/el-sol-esta-oscilando-a-5-kilometros-por-hora\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"El Sol est\u00e1 oscilando a 5 kil\u00f3metros por hora - Observatorio Tecnol\u00f3gico de Hidalgo\" \/>\n<meta property=\"og:description\" content=\"El Sol registra oscilaciones que se manifiestan en la superficie global como movimientos giratorios, con velocidades del orden de 5 kil\u00f3metros por hora. 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