{"id":2408,"date":"1994-01-01T00:00:00","date_gmt":"1994-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/1994\/01\/01\/dinamica-de-la-fotosfera-solar-en-regiones-en-calma-y-faculares\/"},"modified":"1994-01-01T00:00:00","modified_gmt":"1994-01-01T00:00:00","slug":"dinamica-de-la-fotosfera-solar-en-regiones-en-calma-y-faculares","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/dinamica-de-la-fotosfera-solar-en-regiones-en-calma-y-faculares\/","title":{"rendered":"Dinamica de la fotosfera solar en regiones en calma y faculares."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Ines Marquez Rodriguez <\/strong><\/h2>\n<p>En el trabajo se presentan, en primer lugar, datos observacionales de tres lineas fotosfericas seleccionadas, obteniendose valores de los parametros de las lineas (estudiadas sin resolucion espacial), en distintas posiciones sobre el disco solar y a lo largo de secuencias temporales. La autora encuentra diferencias significativas entre los resultados en regiones en calma y faculares.  en segundo lugar se expone el desarrollo de un codigo numerico que, utilizando como atmosfera media la del modelo val-c (vernazza et al., 1981) y como fluctuaciones asociadas a la granulacion solar las del modelo de nelson (1978). El codigo permite la inclusion de diversas influencias: estructuras convectivas de tama\u00f1o mayor al de la granulacion, distintos tipos de ondas y presencia de tubos de flujo magneticos, que pueden ser estudiadas por separado o en conjunto. En ultimo lugar se comparan los resultados simulados para el continuo en regiones faculares con datos observacionales.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Dinamica de la fotosfera solar en regiones en calma y faculares.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Dinamica de la fotosfera solar en regiones en calma y faculares. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Ines Marquez Rodriguez <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 La laguna<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1994<\/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>Jos\u00e9 Antonio Bonet Navarro<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Teodoro Roca Cortes <\/li>\n<li>Manuel Vazquez Abeledo (vocal)<\/li>\n<li>Felix Herrera Cabello (vocal)<\/li>\n<li>Benjam\u00edn Montesinos Comino (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Ines Marquez Rodriguez En el trabajo se presentan, en primer lugar, datos observacionales de tres lineas fotosfericas [&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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