{"id":12883,"date":"2018-03-09T08:58:56","date_gmt":"2018-03-09T08:58:56","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/distribucion-espectral-e-cantidades-de-radiacion-total-par-e-uv-a-na-coruna\/"},"modified":"2018-03-09T08:58:56","modified_gmt":"2018-03-09T08:58:56","slug":"distribucion-espectral-e-cantidades-de-radiacion-total-par-e-uv-a-na-coruna","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/ciencias-de-la-tierra-y-del-espacio\/distribucion-espectral-e-cantidades-de-radiacion-total-par-e-uv-a-na-coruna\/","title":{"rendered":"Distribuci\u00f3n espectral e cantidades de radiaci\u00f3n total, par e uv-a na coru\u00f1a"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Antonio Orozco Gonz\u00e1lez <\/strong><\/h2>\n<p>Los procesos que aprovechan la luz solar dependen en gran parte de la longitud de onda de la radiaci\u00f3n incidente, de donde se infiere la necesidad de conocer el espectro solar y establcer la dependencia del mismo de variables como la estaci\u00f3n del a\u00f1o, la hora del d\u00eda la orientaci\u00f3n del sistema receptor y las condiciones atmosf\u00e9ricas. Los datos de irradiancia espectral son necesarios, entre otros, para optimizar la eficiencia de los sistemas colectores de energ\u00eda solar, evaluar la radiacion fotosint\u00e9ticamente activa, cuantificar el efecto eritem\u00e1tico, investigar la degradaci\u00f3n de materiales, etc.  entre 1995 y 1997 se realizaron medidas de irradiancia para longitudes de onda comprendidas entre 300 y 1100 nm a intervalos de 2 nm en a coru\u00f1a, utilizando un espectrorradi\u00f3metro li-1800. El n\u00famero de medidas espectrales efectuadas fue de 8.279 de las cuales 7.249 se llevaron a cabo en posici\u00f3n horizontal y las 1.030 restantes se hicieron con inclinaciones variables. por otra parte, entre los a\u00f1os 1996 y 2000 se registraron diversos componentes de la radiaci\u00f3n solar como la radiaci\u00f3n incidente (mediante piran\u00f3metro kipp y zonnen, tipo cm3),la radiaci\u00f3n fotosint\u00e9ticamente activa o par (sensor skye skp 210) y ultravioleta b o uv-b (sensor sku 420).  se puso a punto un programa espec\u00edfico escrito en lenguaje c para almacenamiento y gesti\u00f3n de los datos obtendios con espectrorradiometro. Se analizaron los espectros de radiaci\u00f3n solar integrados entre 300 y 1100 nm y la dependencia de los mismos de factores como la hora solar, la masa \u00f3ptica, la estaci\u00f3n del a\u00f1o y la claridad. Se comprob\u00f3 que las variables m\u00e1s importantes para explicar la irradiancia y que pueden ser usadas para analizar procesos dependientes del espectro de radiaci\u00f3n eran la masa \u00f3ptica y el \u00edndice de claridad. Se analiz\u00f3 la influencia que estas variables presentaban sobre zonas espec\u00edficas del espectro, en particular la radiaci\u00f3n fotosint\u00e9ticamente<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Distribuci\u00f3n espectral e cantidades de radiaci\u00f3n total, par e uv-a na coru\u00f1a<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Distribuci\u00f3n espectral e cantidades de radiaci\u00f3n total, par e uv-a na coru\u00f1a <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Antonio Orozco Gonz\u00e1lez <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 A coru\u00f1a<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 21\/09\/2001<\/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>Antonio Paz Gonzalez<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Francisco Maseda eimil <\/li>\n<li>benedicto Soto gonz\u00e1lez (vocal)<\/li>\n<li>sidney Rosa vieria (vocal)<\/li>\n<li>Jos\u00e9 Mah\u00eda saavedra (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Antonio Orozco Gonz\u00e1lez Los procesos que aprovechan la luz solar dependen en gran parte de la longitud [&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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