{"id":50268,"date":"2021-06-07T21:49:57","date_gmt":"2021-06-07T21:49:57","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/estudio-de-la-componente-vh-de-la-radiacion-cosmica-mediante-detector-plastico-lexan\/"},"modified":"2021-06-07T21:49:57","modified_gmt":"2021-06-07T21:49:57","slug":"estudio-de-la-componente-vh-de-la-radiacion-cosmica-mediante-detector-plastico-lexan","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/estudio-de-la-componente-vh-de-la-radiacion-cosmica-mediante-detector-plastico-lexan\/","title":{"rendered":"Estudio de la componente vh de la radiacion cosmica mediante detector plastico lexan."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Montserrat Casas Ametller <\/strong><\/h2>\n<p>Estudio de la componente vh de la radiacion cosmica (20 menor o igual que z menor o igual que 28) mediante el detector inerte policarbonato lexan. El montaje experimental del apilamiento ha permitido la explotacion en zonas correspondientes a distintos intervalos de energia: a) 235 menor o igual que e menor o igual que 355 b) 365 menor o igual que e menor o igual que 455      c) 465 menor o igual que  e menor o igual que 555. La comparacion de los resultados se ha llevado a cabo en lo alto de la atmosfera  para lo cual ha sido necesario el uso de la ecuacion de propagacion  siendo el modelo regular  una vez corregido mediante el termino de perdida de energia el mas idoneo para su resolucion en este caso.  se han calculado       asimismo los parametros de fragmentacion en lexan y aire a distintas ene rgias; y se ha realizado un estudio de la fiabilidad de respuesta del detector en cuanto a discriminacion en carga  y de su sensibilidad en cuantoa discriminacion en masa.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Estudio de la componente vh de la radiacion cosmica mediante detector plastico lexan.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Estudio de la componente vh de la radiacion cosmica mediante detector plastico lexan. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Montserrat Casas Ametller <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Aut\u00f3noma de barcelona<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1982<\/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>quadras Roca Vidal<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Vicente Gandia Gomar <\/li>\n<li>Agustin Alonso Santos (vocal)<\/li>\n<li>Luis Pueyo Panduro (vocal)<\/li>\n<li>Pierre Massue Jean (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Montserrat Casas Ametller Estudio de la componente vh de la radiacion cosmica (20 menor o igual que [&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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