{"id":437,"date":"2017-03-15T11:41:09","date_gmt":"2017-03-15T10:41:09","guid":{"rendered":"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/?page_id=437"},"modified":"2017-05-05T10:54:10","modified_gmt":"2017-05-05T08:54:10","slug":"2002-03-22-2","status":"publish","type":"page","link":"https:\/\/sites-lira.obspm.fr\/gmi-radio-cme\/2002-03-22-2\/","title":{"rendered":"2002-03-18"},"content":{"rendered":"

18 March 2002 (SSC05, -13)ICME, CMEH06\"\"<\/h3>\n

18 March #02:00 UT:<\/strong> Drifting radio burst not detected above 500 MHz, followed by a continuum (onset observed by HIRAISO and by the Culgora radio spectrograph (~100-70 MHz not shown here) (B)<\/strong>. Presence of a type II <\/strong>burst detected by WIND\/Waves. This event is associated with a CME (CMEH06: March 18 (Halo, Width 360 (deg), V 980,971, 971 km\/s).<\/p>\n

This event shares the following characteristics: B, type II burst.<\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"

18 March 2002 (SSC05, -13)ICME, CMEH06 18 March #02:00 UT: Drifting radio burst not detected above 500 MHz, followed by a continuum (onset observed by HIRAISO and by the Culgora radio spectrograph (~100-70 MHz not shown here) (B). Presence of a type II burst detected by WIND\/Waves. This event is associated with a CME (CMEH06: Continue reading <\/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-437","page","type-page","status-publish","hentry"],"yoast_head":"\n2002-03-18 - 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\/2002-03-22-2\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"2002-03-18 - Multi-instrument analysis of solar events during 2002\" \/>\n<meta property=\"og:description\" content=\"18 March 2002 (SSC05, -13)ICME, CMEH06 18 March #02:00 UT: Drifting radio burst not detected above 500 MHz, followed by a continuum (onset observed by HIRAISO and by the Culgora radio spectrograph (~100-70 MHz not shown here) (B). Presence of a type II burst detected by WIND\/Waves. 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