{"id":87254,"date":"2000-09-11T00:00:00","date_gmt":"2000-09-11T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/dinamica-de-las-tormentas-de-gran-escala-en-las-atmosferas-de-los-gigantes-gaseosos\/"},"modified":"2000-09-11T00:00:00","modified_gmt":"2000-09-11T00:00:00","slug":"dinamica-de-las-tormentas-de-gran-escala-en-las-atmosferas-de-los-gigantes-gaseosos","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/ciencias-de-la-tierra-y-del-espacio\/dinamica-de-las-tormentas-de-gran-escala-en-las-atmosferas-de-los-gigantes-gaseosos\/","title":{"rendered":"Din\u00e1mica de las tormentas de gran escala en las atm\u00f3sferas de los gigantes gaseosos"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Ricardo Hueso Alonso <\/strong><\/h2>\n<p>En esta tesis se estudia el desarrollo de las grandes tormentas convectivas que se han observado en los planetas gigantes gaseosos, j\u00fapiter, saturno, urano y neptuno. Las propiedades observadas de estas tormentas se resumen y comentan y se aplica un modelo de simulaci\u00f3n num\u00e9rica tridimensional para estudiar las condiciones en que las grandes tormentas convectivas pueden formarse y las propiedades que estas tormentas poseen. Los resultados del modelo est\u00e1n de acuerdo con las propiedades observadas y es posible establecer reg\u00edmenes convectivos distintos para las tormentas de agua y amon\u00edaco.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Din\u00e1mica de las tormentas de gran escala en las atm\u00f3sferas de los gigantes gaseosos<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Din\u00e1mica de las tormentas de gran escala en las atm\u00f3sferas de los gigantes gaseosos <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Ricardo Hueso Alonso <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Pa\u00eds vasco\/euskal herriko unibertsitatea<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 09\/11\/2000<\/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>Agust\u00edn S\u00e1nchez Lavega<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: manuel Tello le\u00f3n <\/li>\n<li>ram\u00f3n Enrique viloria (vocal)<\/li>\n<li>pierre Drossart (vocal)<\/li>\n<li>agust\u00edn Ezcurra taleg\u00f3n (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Ricardo Hueso Alonso En esta tesis se estudia el desarrollo de las grandes tormentas convectivas que se [&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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