{"id":41514,"date":"1999-01-01T00:00:00","date_gmt":"1999-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/estructura-vertical-nubosa-en-formaciones-meteorologicas-de-jupiter-y-saturno\/"},"modified":"1999-01-01T00:00:00","modified_gmt":"1999-01-01T00:00:00","slug":"estructura-vertical-nubosa-en-formaciones-meteorologicas-de-jupiter-y-saturno","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/ciencias-de-la-tierra-y-del-espacio\/estructura-vertical-nubosa-en-formaciones-meteorologicas-de-jupiter-y-saturno\/","title":{"rendered":"Estructura vertical nubosa en formaciones meteorologicas de jupiter y saturno."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Juan  Ramon Acarreta Rodriguez <\/strong><\/h2>\n<p>Mediante la aplicaci\u00f3n de t\u00e9cnicas de transporte radiactivo, se ha determinado la estructura vertical nubosa de cuatro estructuras meteorol\u00f3gicas peculiares: la gran tormenta de saturno de 1990, los impactos del cometa shoemaker-levy 9 en j\u00fapiter, la mancha polar norte de saturno y la onda polar sur de j\u00fapiter. Adem\u00e1s de la determinaci\u00f3n de la posici\u00f3n vertical de las nubes y nieblas de las citadas estructuras, se obtuvieron propiedades microf\u00edsicas de subpart\u00edculas constituyentes tales como su tama\u00f1o e \u00edndice de refracci\u00f3n. El trabajo se ha realizado mediante el an\u00e1lisis de im\u00e1genes ccd en el rango \u00f3ptico (0,3 &#8211; 1,0 micras), bajo la aproximaci\u00f3n de la atm\u00f3sfera localmente plano-paralela y de part\u00edculas esf\u00e9ricas. las herramientas num\u00e9ricas utilizadas (algoritmo doubling-apding m\u00e1s la aproximaci\u00f3n de mie) han sido desarrollados al efecto durante la realizaci\u00f3n de esta tesis.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Estructura vertical nubosa en formaciones meteorologicas de jupiter y saturno.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Estructura vertical nubosa en formaciones meteorologicas de jupiter y saturno. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Juan  Ramon Acarreta Rodriguez <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Aut\u00f3noma de Madrid<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1999<\/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>Agustin Sanchez Lavega<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal:  Eiroa de san Francisco Carlos <\/li>\n<li>benjam\u00edn Montesinos comino (vocal)<\/li>\n<li>M\u00aa carmen Recondo gonzalez (vocal)<\/li>\n<li> Rosas palenzuela Jos\u00e9 felix (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Juan Ramon Acarreta Rodriguez Mediante la aplicaci\u00f3n de t\u00e9cnicas de transporte radiactivo, se ha determinado la estructura [&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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