{"id":6853,"date":"2022-07-11T15:47:12","date_gmt":"2022-07-11T15:47:12","guid":{"rendered":"https:\/\/raege-az.pt\/?p=6853"},"modified":"2023-12-14T16:33:26","modified_gmt":"2023-12-14T16:33:26","slug":"high-energy-ions-associated-with-the-sep-event-on-may-22-2013","status":"publish","type":"post","link":"https:\/\/raege-az.pt\/en\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/","title":{"rendered":"High energy ions associated with the SEP event on May 22, 2013"},"content":{"rendered":"<div data-elementor-type=\"wp-post\" data-elementor-id=\"6853\" class=\"elementor elementor-6853\">\n\t\t\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-b750b3b elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"b750b3b\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-074f593\" data-id=\"074f593\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-55c3746 elementor-widget elementor-widget-text-editor\" data-id=\"55c3746\" data-element_type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<p>A Solar Energetic Particle (SEP) was detected by the Electron Proton and Alpha Monitor (EPAM) onboard of the Advanced Composition Explorer (ACE) spacecraft on 2013 May 22 both in the electrons and ion channels. In the electrons channels, it is a prompt fast rising highly isotropic event. There is an evidence in the ion channels of protons with energy above 1 GeV arriving essentially at the same time of the electrons. Although EPAM detected protons at sufficiently high energies, the global network of ground-based neutron monitors did not detected any increase in cosmic ray intensity, hence this event is not part of the list of Ground Level Events (GLEs) and since no significant increase of the count rate of at least two different high altitude stations is seen, it seems to fail even the Sub-GLE classification criteria. Comparing the SEP release time with Soft X-Ray (SXR) data on board of Geostationary Operational Environmental Satellites (GOES) spacecraft, we find that the particles were released after the peak in emission of the SXR, which implies that these particles likely do not have a flare origin. Radio data from ground based observatories show type II and type IV emissions at the time of particle release, therefore these particles could either be accelerated in the magnetic restructuring in the aftermath of a Coronal Mass Ejection (CME) or in an associated shock. We discuss both possibilities.<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-f6ac104 elementor-widget elementor-widget-text-editor\" data-id=\"f6ac104\" data-element_type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<p>Cuambe, Valente<sup>[1]<\/sup>; Chavango, Bivar<sup>[2]<\/sup>; Maia, Dalmiro<sup>[3]<\/sup>; Morgado, Jorge<sup>[3]<\/sup>; Machaieie, Dinelsa<sup>[2]<\/sup>; Bergano, Miguel<sup>[3]<\/sup>; Barbosa, Domingos<sup>[4]<\/sup><\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-20bec53 elementor-widget elementor-widget-text-editor\" data-id=\"20bec53\" data-element_type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<p><strong>Type\u00a0<\/strong>Presentation<\/p><p><strong>Event <\/strong>44th COSPAR Scientific Assembly<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-326074b elementor-widget elementor-widget-text-editor\" data-id=\"326074b\" data-element_type=\"widget\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<p>[1] Esta\u00e7\u00e3o RAEGE de Santa Maria, Associa\u00e7\u00e3o RAEGE A\u00e7ores, Santa Maria &#8211; Azores, Portugal<\/p><p>[2] Universidade Eduardo Mondlane, Maputo &#8211; Mo\u00e7ambique<\/p><p>[3] Centro de Investiga\u00e7\u00e3o em Ci\u00eancias Geoespaciais da Universidade do Porto, Vila Nova de Gaia &#8211; Portugal<\/p><p>[4] Instituto de Telecomunica\u00e7\u00f5es, Aveiro-Portugal<\/p>\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<div class=\"elementor-element elementor-element-cd1e58d elementor-widget elementor-widget-button\" data-id=\"cd1e58d\" data-element_type=\"widget\" data-widget_type=\"button.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\t\t\t\t\t\t<div class=\"elementor-button-wrapper\">\n\t\t\t\t\t<a class=\"elementor-button elementor-button-link elementor-size-sm\" href=\"\/en\/publicacoes\/\">\n\t\t\t\t\t\t<span class=\"elementor-button-content-wrapper\">\n\t\t\t\t\t\t\t\t\t<span class=\"elementor-button-text\">Voltar \u00e0 p\u00e1gina publica\u00e7\u00f5es<\/span>\n\t\t\t\t\t<\/span>\n\t\t\t\t\t<\/a>\n\t\t\t\t<\/div>\n\t\t\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<\/div>","protected":false},"excerpt":{"rendered":"<p>A Solar Energetic Particle (SEP) was detected by the Electron Proton and Alpha Monitor (EPAM) onboard of the Advanced Composition Explorer (ACE) spacecraft on 2013 May 22 both in the electrons and ion channels. In the electrons channels, it is a prompt fast rising highly isotropic event. There is an evidence in the ion channels [&hellip;]<\/p>","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"elementor_theme","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"default","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":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"default","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 center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","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-opacity":"","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-opacity":"","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-opacity":"","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-opacity":"","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-opacity":"","overlay-gradient":""}},"footnotes":""},"categories":[41,36,33],"tags":[],"class_list":["post-6853","post","type-post","status-publish","format-standard","hentry","category-41","category-apresentacao","category-publicacoes"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v25.5 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>High energy ions associated with the SEP event on May 22, 2013 - RAEGE-Az<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/raege-az.pt\/en\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/\" \/>\n<meta property=\"og:locale\" content=\"en_GB\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"High energy ions associated with the SEP event on May 22, 2013 - RAEGE-Az\" \/>\n<meta property=\"og:description\" content=\"A Solar Energetic Particle (SEP) was detected by the Electron Proton and Alpha Monitor (EPAM) onboard of the Advanced Composition Explorer (ACE) spacecraft on 2013 May 22 both in the electrons and ion channels. In the electrons channels, it is a prompt fast rising highly isotropic event. There is an evidence in the ion channels [&hellip;]\" \/>\n<meta property=\"og:url\" content=\"https:\/\/raege-az.pt\/en\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/\" \/>\n<meta property=\"og:site_name\" content=\"RAEGE-Az\" \/>\n<meta property=\"article:publisher\" content=\"https:\/\/www.facebook.com\/raege.az\" \/>\n<meta property=\"article:published_time\" content=\"2022-07-11T15:47:12+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2023-12-14T16:33:26+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/raege-az.pt\/wp-content\/uploads\/2021\/04\/2.png\" \/>\n\t<meta property=\"og:image:width\" content=\"1500\" \/>\n\t<meta property=\"og:image:height\" content=\"1500\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/png\" \/>\n<meta name=\"author\" content=\"admin\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<meta name=\"twitter:label1\" content=\"Written by\" \/>\n\t<meta name=\"twitter:data1\" content=\"admin\" \/>\n\t<meta name=\"twitter:label2\" content=\"Est. reading time\" \/>\n\t<meta name=\"twitter:data2\" content=\"2 minutes\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\/\/schema.org\",\"@graph\":[{\"@type\":\"Article\",\"@id\":\"https:\/\/raege-az.pt\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/#article\",\"isPartOf\":{\"@id\":\"https:\/\/raege-az.pt\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/\"},\"author\":{\"name\":\"admin\",\"@id\":\"https:\/\/raege-az.pt\/en\/#\/schema\/person\/18312cab60131e2890511f343fbbd7a7\"},\"headline\":\"High energy ions associated with the SEP event on May 22, 2013\",\"datePublished\":\"2022-07-11T15:47:12+00:00\",\"dateModified\":\"2023-12-14T16:33:26+00:00\",\"mainEntityOfPage\":{\"@id\":\"https:\/\/raege-az.pt\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/\"},\"wordCount\":310,\"publisher\":{\"@id\":\"https:\/\/raege-az.pt\/en\/#organization\"},\"articleSection\":[\"2022\",\"Apresenta\u00e7\u00e3o\",\"Publica\u00e7\u00f5es\"],\"inLanguage\":\"en-GB\"},{\"@type\":\"WebPage\",\"@id\":\"https:\/\/raege-az.pt\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/\",\"url\":\"https:\/\/raege-az.pt\/high-energy-ions-associated-with-the-sep-event-on-may-22-2013\/\",\"name\":\"High energy ions associated with the SEP event on May 22, 2013 - 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