{"version":"1.0","provider_name":"Multi-instrument analysis of solar events during 2002","provider_url":"https:\/\/sites.lesia.obspm.fr\/gmi-radio-cme","author_name":"pick","author_url":"https:\/\/sites.lesia.obspm.fr\/gmi-radio-cme\/author\/pick\/","title":"05Sept 2002 - Multi-instrument analysis of solar events during 2002","type":"rich","width":600,"height":338,"html":"<blockquote class=\"wp-embedded-content\" data-secret=\"mpvzfSUi5R\"><a href=\"https:\/\/sites.lesia.obspm.fr\/gmi-radio-cme\/2002-09-05\/05sept05-comp-2\/\">05Sept 2002<\/a><\/blockquote><iframe sandbox=\"allow-scripts\" security=\"restricted\" src=\"https:\/\/sites.lesia.obspm.fr\/gmi-radio-cme\/2002-09-05\/05sept05-comp-2\/embed\/#?secret=mpvzfSUi5R\" width=\"600\" height=\"338\" title=\"&#8220;05Sept 2002&#8221; &#8212; Multi-instrument analysis of solar events during 2002\" data-secret=\"mpvzfSUi5R\" frameborder=\"0\" marginwidth=\"0\" marginheight=\"0\" scrolling=\"no\" class=\"wp-embedded-content\"><\/iframe><script type=\"text\/javascript\">\n\/* <![CDATA[ *\/\n\/*! This file is auto-generated *\/\n!function(d,l){\"use strict\";l.querySelector&&d.addEventListener&&\"undefined\"!=typeof URL&&(d.wp=d.wp||{},d.wp.receiveEmbedMessage||(d.wp.receiveEmbedMessage=function(e){var t=e.data;if((t||t.secret||t.message||t.value)&&!\/[^a-zA-Z0-9]\/.test(t.secret)){for(var s,r,n,a=l.querySelectorAll('iframe[data-secret=\"'+t.secret+'\"]'),o=l.querySelectorAll('blockquote[data-secret=\"'+t.secret+'\"]'),c=new RegExp(\"^https?:$\",\"i\"),i=0;i<o.length;i++)o[i].style.display=\"none\";for(i=0;i<a.length;i++)s=a[i],e.source===s.contentWindow&&(s.removeAttribute(\"style\"),\"height\"===t.message?(1e3<(r=parseInt(t.value,10))?r=1e3:~~r<200&&(r=200),s.height=r):\"link\"===t.message&&(r=new URL(s.getAttribute(\"src\")),n=new URL(t.value),c.test(n.protocol))&&n.host===r.host&&l.activeElement===s&&(d.top.location.href=t.value))}},d.addEventListener(\"message\",d.wp.receiveEmbedMessage,!1),l.addEventListener(\"DOMContentLoaded\",function(){for(var e,t,s=l.querySelectorAll(\"iframe.wp-embedded-content\"),r=0;r<s.length;r++)(t=(e=s[r]).getAttribute(\"data-secret\"))||(t=Math.random().toString(36).substring(2,12),e.src+=\"#?secret=\"+t,e.setAttribute(\"data-secret\",t)),e.contentWindow.postMessage({message:\"ready\",secret:t},\"*\")},!1)))}(window,document);\n\/* ]]> *\/\n<\/script>\n","thumbnail_url":"https:\/\/sites.lesia.obspm.fr\/gmi-radio-cme\/files\/2017\/02\/05Sept05-comp-1.jpg","thumbnail_width":718,"thumbnail_height":945,"description":"05 September 2002: 16:10 UT: Microwave burst at 8.8-GHz (A) (SanVito), also observed in the 2-0.8 GHz frequency range by Ondrejov. Around 16:30: strong microwave flux increase which drifts in frequency and is successively detected by the Postdam spectrograph (600-200 MHz) and by WIND\/Waves (Type III bursts) (see right side panel). This is followed by the onset of a type II burst at 16:55 UT. The event is associated with a CME (CMEh36 16:54 UT, V 1748, 1855, 1903 km s\u22121). This CME displays, near the onset time of the type II burst, a rapid evolution of its western edge and the region located between this CME and its western neighbouring one becomes very bright; we suggest that the WIND\/Waves type II burst might originate from this region. The onset of a bursty continuum (a common property at low frequencies) is observed near 17 UT . This event shares the following characteristics: Microwave burst and continuum (type IV), Type II burst, (may-be originating from the encounter between two CMEs)."}