{"id":34204,"date":"1998-01-01T00:00:00","date_gmt":"1998-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/medida-del-espectro-y-la-composicion-de-los-rayos-cosmicos-en-el-rango-de-300-tev-a-30-pev\/"},"modified":"1998-01-01T00:00:00","modified_gmt":"1998-01-01T00:00:00","slug":"medida-del-espectro-y-la-composicion-de-los-rayos-cosmicos-en-el-rango-de-300-tev-a-30-pev","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/fisica\/medida-del-espectro-y-la-composicion-de-los-rayos-cosmicos-en-el-rango-de-300-tev-a-30-pev\/","title":{"rendered":"Medida del espectro y la composicion de los rayos cosmicos en el rango de 300 tev a 30 pev."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Juan Cortina Blanco <\/strong><\/h2>\n<p>Se presentan los resultados de la medici\u00f3n del espectro y la composici\u00f3n qu\u00edmica de los rayos c\u00f3smicos en la regi\u00f3n energ\u00e9tica de 300 tev a 30 pev con el detector hegra.  mediante una simulaci\u00f3n de monte carlo, se han desarrollado nuevos m\u00e9todos para la determinaci\u00f3n de la energ\u00eda primaria de los rayos c\u00f3smicos basados en la medida conjugada del n\u00famero de electrones o la luz cherenkov de la cascada de part\u00edculas producida por el n\u00facleo primario en la \u00e1tmosfera y de la posici\u00f3n del m\u00e1ximo del desarrollo de la cascada. El c\u00e1lculo de la energ\u00eda primaria permite la medida directa del espectro de los rayos c\u00f3smicos y la informaci\u00f3n a\u00f1adida del m\u00e1ximo de la cascada nos permite estimar la proporci\u00f3n de elementos ligeros en el total de los rayos c\u00f3smicos. Los resultados son compatibles con una proporci\u00f3n pr\u00e1cticamente igual de elementos ligeros a pesados en todo el rango de energ\u00edas considerado.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Medida del espectro y la composicion de los rayos cosmicos en el rango de 300 tev a 30 pev.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Medida del espectro y la composicion de los rayos cosmicos en el rango de 300 tev a 30 pev. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Juan Cortina Blanco <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Complutense de Madrid<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1998<\/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>Fernando Arqueros Mart\u00ednez<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Jose Campos Gutierrez <\/li>\n<li>Enrique Zas Arregui (vocal)<\/li>\n<li>Antonio Dorado Gonzalez (vocal)<\/li>\n<li>Miguel Mas Hesse (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Juan Cortina Blanco Se presentan los resultados de la medici\u00f3n del espectro y la composici\u00f3n qu\u00edmica de [&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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