{"id":8491,"date":"2025-07-31T16:03:06","date_gmt":"2025-07-31T19:03:06","guid":{"rendered":"https:\/\/dicyt.usach.cl\/?p=8491"},"modified":"2025-08-12T18:13:07","modified_gmt":"2025-08-12T21:13:07","slug":"estudio-de-la-magnetosfera-terrestre-frente-a-tormentas-solares-intensas","status":"publish","type":"post","link":"https:\/\/dicyt.usach.cl\/index.php\/estudio-de-la-magnetosfera-terrestre-frente-a-tormentas-solares-intensas\/","title":{"rendered":"Estudio de la magnet\u00f3sfera terrestre frente a tormentas solares intensas"},"content":{"rendered":"\t\t<div data-elementor-type=\"wp-post\" data-elementor-id=\"8491\" class=\"elementor elementor-8491\" data-elementor-post-type=\"post\">\n\t\t\t\t<div class=\"elementor-element elementor-element-5b6f2e0 e-flex e-con-boxed e-con e-parent\" data-id=\"5b6f2e0\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-b1ae17b elementor-widget-divider--view-line elementor-widget elementor-widget-divider\" data-id=\"b1ae17b\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"divider.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-divider\">\n\t\t\t<span class=\"elementor-divider-separator\">\n\t\t\t\t\t\t<\/span>\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-f362043 animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"f362043\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-593b385 e-flex e-con-boxed e-con e-child\" data-id=\"593b385\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-8a7c31d elementor-widget elementor-widget-video\" data-id=\"8a7c31d\" data-element_type=\"widget\" data-e-type=\"widget\" data-settings=\"{&quot;youtube_url&quot;:&quot;https:\\\/\\\/www.youtube.com\\\/watch?v=Lb2WSlwRTjo&amp;list=PLAhmlASb3v1BUJjeL9U--nciebw_y5i8y&amp;index=1&amp;ab_channel=Investigaci%C3%B3n%2CInnovaci%C3%B3nyCreaci%C3%B3nUSACH%28VRIIC%29&quot;,&quot;video_type&quot;:&quot;youtube&quot;,&quot;controls&quot;:&quot;yes&quot;}\" data-widget_type=\"video.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-wrapper elementor-open-inline\">\n\t\t\t<div class=\"elementor-video\"><\/div>\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-cf480d2 elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"cf480d2\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<i aria-hidden=\"true\" class=\"fas fa-check\"><\/i>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tTurbulencia y equilibrio de presi\u00f3n total en la magnetosfera din\u00e1mica interconectada\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-bb696a6 animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"bb696a6\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-45fc0da e-flex e-con-boxed e-con e-child\" data-id=\"45fc0da\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-fc96780 elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"fc96780\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<i aria-hidden=\"true\" class=\"far fa-user\"><\/i>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tDirector del proyecto\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\t\t\t\t\t<p class=\"elementor-icon-box-description\">\n\t\t\t\t\t\tDra. Marina Stepanova, acad\u00e9mica e investigadora Departamento de F\u00edsica, Usach.\t\t\t\t\t<\/p>\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-b672ead animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"b672ead\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-eac44db e-flex e-con-boxed e-con e-child\" data-id=\"eac44db\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-6995526 elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"6995526\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" id=\"Capa_1\" data-name=\"Capa 1\" viewBox=\"0 0 384 382.5\"><path d=\"M0,0H112.27V67.41H67.77V315h44.55V382.5H0ZM22.76,22.64V359.69h67v-22.3H45.27V44.79H89.78V22.64Z\"><\/path><path d=\"M384,382.5H271.73V315.08h44.5V67.55H271.68V0H384Zm-22.74-22.67v-337H294.19V45.06h44.57v292.6H294.2v22.17Z\"><\/path><path d=\"M293.82,90.26v22H90.3v-22Z\"><\/path><path d=\"M293.82,135.25v22.07H90.29V135.25Z\"><\/path><path d=\"M293.83,180.26v22H90.18v-22Z\"><\/path><path d=\"M90.17,247.24V225.19H293.69v22.05Z\"><\/path><path d=\"M293.83,270.25v22.06H90.3V270.25Z\"><\/path><\/svg>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tContexto\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\t\t\t\t\t<p class=\"elementor-icon-box-description\">\n\t\t\t\t\t\tLa magnetosfera terrestre es una regi\u00f3n del espacio dominada por el campo magn\u00e9tico del planeta, que act\u00faa como escudo frente al viento solar. Este entorno est\u00e1 compuesto por plasmas de origen solar e ionosf\u00e9rico, y su din\u00e1mica influye directamente en fen\u00f3menos como las tormentas geomagn\u00e9ticas, capaces de afectar infraestructuras tecnol\u00f3gicas en la Tierra. Estudios recientes han revelado que la cola geomagn\u00e9tica puede comportarse como una estela turbulenta generada por la interacci\u00f3n del viento solar con el campo magn\u00e9tico terrestre, lo que plantea nuevos desaf\u00edos para su comprensi\u00f3n.\t\t\t\t\t<\/p>\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-cb9caa2 animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"cb9caa2\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-24e9ff2 e-flex e-con-boxed e-con e-child\" data-id=\"24e9ff2\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-26255d9 elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"26255d9\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<i aria-hidden=\"true\" class=\"far fa-question-circle\"><\/i>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tProblema\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\t\t\t\t\t<p class=\"elementor-icon-box-description\">\n\t\t\t\t\t\tLos m\u00e9todos tradicionales para estudiar la din\u00e1mica magnetosf\u00e9rica no consideran adecuadamente los efectos de la turbulencia ni las variaciones en la distribuci\u00f3n del plasma. En particular, la falta de un enfoque que integre el equilibrio de presiones \u2013plasm\u00e1tica, magn\u00e9tica y din\u00e1mica\u2013 limita la capacidad de entender y predecir fen\u00f3menos cr\u00edticos como las tormentas y subtormentas geomagn\u00e9ticas.\t\t\t\t\t<\/p>\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-d184e5f animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"d184e5f\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-062081c e-flex e-con-boxed e-con e-child\" data-id=\"062081c\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-aee69af elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"aee69af\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<i aria-hidden=\"true\" class=\"far fa-lightbulb\"><\/i>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tSoluci\u00f3n\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\t\t\t\t\t<p class=\"elementor-icon-box-description\">\n\t\t\t\t\t\tEl proyecto propone estudiar la magnetosfera como un sistema interconectado, compuesto por regiones con diferentes caracter\u00edsticas din\u00e1micas. A trav\u00e9s del an\u00e1lisis de datos obtenidos por misiones satelitales de largo plazo y multiregi\u00f3n, se evaluar\u00e1 c\u00f3mo la conservaci\u00f3n del balance de presi\u00f3n total, incluso en condiciones turbulentas y no-Maxwellianas, influye en la evoluci\u00f3n del plasma y en la generaci\u00f3n de eventos geomagn\u00e9ticos. Este enfoque permite integrar la turbulencia, la presi\u00f3n del plasma y los campos el\u00e9ctricos en una visi\u00f3n coherente del sistema.\t\t\t\t\t<\/p>\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-50c6383 animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"50c6383\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-411c555 e-flex e-con-boxed e-con e-child\" data-id=\"411c555\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-5092028 elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"5092028\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<i aria-hidden=\"true\" class=\"fas fa-chart-line\"><\/i>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tObjetivos\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\t\t\t\t\t<p class=\"elementor-icon-box-description\">\n\t\t\t\t\t\t1. Analizar la estabilidad de la hoja de plasma turbulenta y su relaci\u00f3n con el balance de presi\u00f3n total.<br><br>2. Estudiar la evoluci\u00f3n de la presi\u00f3n del plasma durante tormentas geomagn\u00e9ticas y el rol del transporte turbulento.<br><br>3. Investigar el impacto de la turbulencia intermitente en funciones de distribuci\u00f3n de part\u00edculas no-Maxwellianas y evaluar la aplicabilidad de modelos MHD.\t\t\t\t\t<\/p>\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t<div class=\"elementor-element elementor-element-0ce76ff animated-fast e-flex e-con-boxed elementor-invisible e-con e-parent\" data-id=\"0ce76ff\" data-element_type=\"container\" data-e-type=\"container\" data-settings=\"{&quot;animation&quot;:&quot;zoomIn&quot;}\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t<div class=\"elementor-element elementor-element-8d5ec74 e-flex e-con-boxed e-con e-child\" data-id=\"8d5ec74\" data-element_type=\"container\" data-e-type=\"container\">\n\t\t\t\t\t<div class=\"e-con-inner\">\n\t\t\t\t<div class=\"elementor-element elementor-element-0bec8f1 elementor-position-inline-start elementor-view-default elementor-mobile-position-block-start elementor-widget elementor-widget-icon-box\" data-id=\"0bec8f1\" data-element_type=\"widget\" data-e-type=\"widget\" data-widget_type=\"icon-box.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t<div class=\"elementor-icon-box-wrapper\">\n\n\t\t\t\t\t\t<div class=\"elementor-icon-box-icon\">\n\t\t\t\t<span  class=\"elementor-icon\">\n\t\t\t\t<i aria-hidden=\"true\" class=\"fas fa-chart-line\"><\/i>\t\t\t\t<\/span>\n\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t<div class=\"elementor-icon-box-content\">\n\n\t\t\t\t\t\t\t\t\t<h3 class=\"elementor-icon-box-title\">\n\t\t\t\t\t\t<span  >\n\t\t\t\t\t\t\tBeneficios\t\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/h3>\n\t\t\t\t\n\t\t\t\t\t\t\t\t\t<p class=\"elementor-icon-box-description\">\n\t\t\t\t\t\tEste estudio permitir\u00e1 avanzar en la comprensi\u00f3n de la din\u00e1mica global de la magnetosfera terrestre, con especial foco en los mecanismos de entrada de plasma y en la generaci\u00f3n de eventos geomagn\u00e9ticos. Los resultados contribuir\u00e1n al desarrollo de mejores modelos de predicci\u00f3n del clima espacial, con aplicaciones en la protecci\u00f3n de sat\u00e9lites, comunicaciones y redes el\u00e9ctricas.\t\t\t\t\t<\/p>\n\t\t\t\t\n\t\t\t<\/div>\n\t\t\t\n\t\t<\/div>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t","protected":false},"excerpt":{"rendered":"<p>Turbulencia y equilibrio de presi\u00f3n total en la magnetosfera din\u00e1mica interconectada Director del proyecto Dra. Marina Stepanova, acad\u00e9mica e investigadora Departamento de F\u00edsica, Usach. Contexto La magnetosfera terrestre es una regi\u00f3n del espacio dominada por el campo magn\u00e9tico del planeta, que act\u00faa como escudo frente al viento solar. Este entorno est\u00e1 compuesto por plasmas de [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":8494,"comment_status":"closed","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"inline_featured_image":false,"_mi_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","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":"disabled","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","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":"set","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center 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href=\"https:\/\/dicyt.usach.cl\/index.php\/category\/fisica\/\" rel=\"category tag\">F\u00edsica<\/a>","rttpg_excerpt":"Turbulencia y equilibrio de presi\u00f3n total en la magnetosfera din\u00e1mica interconectada Director del proyecto Dra. Marina Stepanova, acad\u00e9mica e investigadora Departamento de F\u00edsica, Usach. Contexto La magnetosfera terrestre es una regi\u00f3n del espacio dominada por el campo magn\u00e9tico del planeta, que act\u00faa como escudo frente al viento solar. Este entorno est\u00e1 compuesto por plasmas de&hellip;","_links":{"self":[{"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/posts\/8491","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/comments?post=8491"}],"version-history":[{"count":10,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/posts\/8491\/revisions"}],"predecessor-version":[{"id":8639,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/posts\/8491\/revisions\/8639"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/media\/8494"}],"wp:attachment":[{"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/media?parent=8491"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/categories?post=8491"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/dicyt.usach.cl\/index.php\/wp-json\/wp\/v2\/tags?post=8491"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}