{"id":211,"date":"2017-02-20T17:48:55","date_gmt":"2017-02-20T16:48:55","guid":{"rendered":"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/?page_id=211"},"modified":"2017-09-11T17:12:36","modified_gmt":"2017-09-11T15:12:36","slug":"2002-08-17","status":"publish","type":"page","link":"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/2002-08-17\/","title":{"rendered":"2002-05-17"},"content":{"rendered":"<h3>May 17 2002 (SSC15, -36) ICME, CMEN22 <img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-212\" src=\"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/files\/2017\/02\/17MAY2002dern-228x300.jpg\" width=\"500\" height=\"658\" srcset=\"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/files\/2017\/02\/17MAY2002dern-228x300.jpg 228w, https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/files\/2017\/02\/17MAY2002dern.jpg 718w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/h3>\n<p><strong>17 May 2002:<\/strong>\u00a0 07:38 UT: Onset\u00a0 of a\u00a0 microwave burst <strong>(A)<\/strong> which drifts\u00a0 towards\u00a0 lower frequencies\u00a0 and\u00a0 stops abrutly its development at 08:00 UT. This disappearance could be attributed to the encounter between the coronal structure, site of the microwave burst, and\u00a0 a CME\u00a0 (<strong>CMEN22<\/strong>: 08:06 UT PA 61 (deg),\u00a0 Width 92 (deg),\u00a0 V 665 616 575 km\/s).\u00a0 The signature of this encounter is\u00a0 the onset of a short duration radio burst observed at discrete frequencies (between roughly 800 MHz and hectometer wave-lengths) .<\/p>\n<p><em>This event shares the following characteristics<\/em>: Microwave burst <strong>(A)<\/strong> drifting in frequency; sudden stop as inferred from radio observations, presumably after its <strong>encounter<\/strong> with a coronal obstacle.<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>May 17 2002 (SSC15, -36) ICME, CMEN22 17 May 2002:\u00a0 07:38 UT: Onset\u00a0 of a\u00a0 microwave burst (A) which drifts\u00a0 towards\u00a0 lower frequencies\u00a0 and\u00a0 stops abrutly its development at 08:00 UT. This disappearance could be attributed to the encounter between the coronal structure, site of the microwave burst, and\u00a0 a CME\u00a0 (CMEN22: 08:06 UT PA <a class=\"more-link\" href=\"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/2002-08-17\/\">Continue reading <i class=\"fa fa-chevron-right\"><\/i><\/a><\/p>\n","protected":false},"author":43,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-211","page","type-page","status-publish","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v28.3 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>2002-05-17 - Multi-instrument analysis of solar events during 2002<\/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:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/2002-08-17\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"2002-05-17 - Multi-instrument analysis of solar events during 2002\" \/>\n<meta property=\"og:description\" content=\"May 17 2002 (SSC15, -36) ICME, CMEN22 17 May 2002:\u00a0 07:38 UT: Onset\u00a0 of a\u00a0 microwave burst (A) which drifts\u00a0 towards\u00a0 lower frequencies\u00a0 and\u00a0 stops abrutly its development at 08:00 UT. 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