{"id":95703,"date":"2018-03-11T10:15:45","date_gmt":"2018-03-11T10:15:45","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/decaimiento-de-flujo-magnetico-en-el-sol-manchas-mmfs-y-ers\/"},"modified":"2018-03-11T10:15:45","modified_gmt":"2018-03-11T10:15:45","slug":"decaimiento-de-flujo-magnetico-en-el-sol-manchas-mmfs-y-ers","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/la-laguna\/decaimiento-de-flujo-magnetico-en-el-sol-manchas-mmfs-y-ers\/","title":{"rendered":"Decaimiento de flujo magnetico en el sol: manchas, mmfs y ers"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Alberto Sainz Dalda <\/strong><\/h2>\n<p>El decaimiento de las regiones activas en en sol muestran dos fases, a saber: una fase linieal de p\u00e9rdida de flujo local, y otra fase plana. A partir de los datos del instrumento soho\/mdi hemos estudiado la evoluci\u00f3n de tres regiones activas, cuantificando por primera vez estos ritmos de decaimiento, as\u00ed como las cancdelacioones y p\u00e9rdidas de flujo in situ que se producen en ellas. Se ha descubierto por primera vez la estructura superpeenumbral en las manchas solares, en la que las estructruas magn\u00e9tcias en movimiento realizan trayectorias radiales. Asimismo, se han descubierto movimientos serpentinos en los filamentos penumbrales, que a pesar de haber sido presdichos te\u00f3ricamente nunca hab\u00edan sido obaservados.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Decaimiento de flujo magnetico en el sol: manchas, mmfs y ers<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Decaimiento de flujo magnetico en el sol: manchas, mmfs y ers <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Alberto Sainz Dalda <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 La laguna<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 29\/07\/2009<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n<h3>Direcci\u00f3n y tribunal<\/h3>\n<ul>\n<li><strong>Director de la tesis<\/strong>\n<ul>\n<li>Valent\u00edn Mart\u00ednez Pillet<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: teodoro Roca cort\u00e9s <\/li>\n<li>arturo Lopez ariste (vocal)<\/li>\n<li>Jos\u00e9 Carlos del Toro iniesta (vocal)<\/li>\n<li>Andr\u00e9s Asensio ramos (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Alberto Sainz Dalda El decaimiento de las regiones activas en en sol muestran dos fases, a saber: [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center 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