{"id":135415,"date":"1997-01-01T00:00:00","date_gmt":"1997-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/aplicacion-de-una-nueva-tecnica-observacional-al-estudio-de-modos-gravitatorios-solares\/"},"modified":"1997-01-01T00:00:00","modified_gmt":"1997-01-01T00:00:00","slug":"aplicacion-de-una-nueva-tecnica-observacional-al-estudio-de-modos-gravitatorios-solares","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/aplicacion-de-una-nueva-tecnica-observacional-al-estudio-de-modos-gravitatorios-solares\/","title":{"rendered":"Aplicacion de una nueva tecnica observacional al estudio de modos gravitatorios solares."},"content":{"rendered":"<h2>Tesis doctoral de <strong>  Martin Mateos Isabel Teresa <\/strong><\/h2>\n<p>El trabajo recogido en la presente memoria describe un experimento encaminado hacia la deteccion de modos gravitatorios solares. Los datos tomados en el observatorio del teide entre los a\u00f1os 1991 y 1993, consisten en medidas diarias de velocidad solar obtenidas secuencialmente en seis posiciones diferentes y simetricas sobre el disco solar. El analisis conjunto de las series de cada apertura y sus combinaciones lineales permite obtener los espectros de potencia con el menor ruido de todos aquellos que existen en la actualidad.  combinando parejas de espectros se estudio la relacion entre las fases de picos que superaban ciertos limites establecidos en potencia y que eran comunes a los espectros considerados. Finalmente se llego a una seleccion con la identificacion de 18 picos, considerados se\u00f1ales estables, probablemente modo gravitatorio.  la comparacion de estos picos con los predichos por algunos modelos solares dan mayores semejanzas con un modelo estandar que incluye difusion de he. En este caso, se alcanza un 72% de los picos identificados con un margen de error de 0.5 microhertzios.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Aplicacion de una nueva tecnica observacional al estudio de modos gravitatorios solares.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Aplicacion de una nueva tecnica observacional al estudio de modos gravitatorios solares. <\/li>\n<li><strong>Autor:<\/strong>\u00a0  Martin Mateos Isabel Teresa <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 La laguna<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1997<\/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> Palle Manzano Pere LLuis<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Teodoro Roca Cortes <\/li>\n<li>Bernard Gelly (vocal)<\/li>\n<li>Manuel Vazquez Abeledo (vocal)<\/li>\n<li>Miguel Angel Aballe Villero (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Martin Mateos Isabel Teresa El trabajo recogido en la presente memoria describe un experimento encaminado hacia la [&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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