{"id":64263,"date":"2018-03-09T22:52:15","date_gmt":"2018-03-09T22:52:15","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/near-relativistic-electron-events-monte-carlo-simulatons-of-solar-injection-and-interplanetary-transport\/"},"modified":"2018-03-09T22:52:15","modified_gmt":"2018-03-09T22:52:15","slug":"near-relativistic-electron-events-monte-carlo-simulatons-of-solar-injection-and-interplanetary-transport","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/barcelona\/near-relativistic-electron-events-monte-carlo-simulatons-of-solar-injection-and-interplanetary-transport\/","title":{"rendered":"Near-relativistic electron events. monte carlo simulatons of solar injection and interplanetary transport."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Neus Agueda Costafreda <\/strong><\/h2>\n<p>Hemos desarrollado un modelo monte carlo para simular el transporte de electrones solares casi-relativistas (30-300 kev) en el medio interplanetario que tiene en cuenta los efectos de la focalizaci\u00f3n adiab\u00e1tica, la dispersi\u00f3n en \u00e1ngulo de batida y los efectos del viento solar. Teniendo en cuenta la respuesta angular del telescopio lefs60 del experimento epam a bordo de la sonda interplanetaria ace, hemos construido un algoritmo que, por primera vez, permite transformar las distribuciones angulares de part\u00edculas simuladas en intensidades sectoriales observadas por un detector a bordo de una sonda estabilizada en el giro.  as\u00ed mismo, hemos desarrollado un algoritmo que permite, por primera vez, deconvolucionar los efectos del transporte interplanetario en las intensidades sectoriales observadas, con el objetivo de determinar a partir del mejor ajuste posible de las caracter\u00edsticas del transporte y el perfil de inyecci\u00f3n solar. Hemos aplicado el modelo al estudio de siete sucesos de electrones observados por la sonda ace entre 1998 y 2004. Este estudio ha permitido evaluar los roles de las fulguraciones solares y de los choques conducidos por eyecciones de masa coronal en la inyecci\u00f3n de electrones solares casi-relativistas, as\u00ed como las caracter\u00edsticas del transport  de los electrones a lo largo del campo magn\u00e9tico interplanetario. esta tesis pone de manifiesto que existe un amplio espectro de escenarios posibles que abarca la inyecci\u00f3n de electrones casi-relativistas en procesos fulgurativos, en choques coronales conducidos por eyecciones de masa coronal o en ambos. As\u00ed mismo, pone de manifiesto que el transporte de los electrones casi-relativistas se puede producir tanto en condiciones muy dispersas como en condiciones muy poco dispersivas.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Near-relativistic electron events. monte carlo simulatons of solar injection and interplanetary transport.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Near-relativistic electron events. monte carlo simulatons of solar injection and interplanetary transport. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Neus Agueda Costafreda <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Barcelona<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 28\/04\/2008<\/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>Blas Sanahuja Parera<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: vicente Domingo <\/li>\n<li>Javier Roriguez pachero (vocal)<\/li>\n<li>josep l. Ballester (vocal)<\/li>\n<li>bernd Heber (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Neus Agueda Costafreda Hemos desarrollado un modelo monte carlo para simular el transporte de electrones solares casi-relativistas [&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 center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-gradient":""}},"footnotes":""},"categories":[951,10260,55762,36996,36997],"tags":[141827,1054,141825,141826,141823,141824],"class_list":["post-64263","post","type-post","status-publish","format-standard","hentry","category-barcelona","category-el-sol","category-materia-interplanetaria","category-medio-interplanetario","category-particulas-interplanetarias","tag-bernd-heber","tag-blas-sanahuja-parera","tag-javier-roriguez-pachero","tag-josep-l-ballester","tag-neus-agueda-costafreda","tag-vicente-domingo"],"_links":{"self":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts\/64263","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/comments?post=64263"}],"version-history":[{"count":0,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/posts\/64263\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/media?parent=64263"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/categories?post=64263"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.deberes.net\/tesis\/wp-json\/wp\/v2\/tags?post=64263"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}