{"id":5067,"date":"2022-04-28T15:45:12","date_gmt":"2022-04-28T13:45:12","guid":{"rendered":"https:\/\/site.uit.no\/spaceweather\/?page_id=5067"},"modified":"2022-05-05T12:50:20","modified_gmt":"2022-05-05T10:50:20","slug":"xray-flux","status":"publish","type":"page","link":"https:\/\/site.uit.no\/spaceweather\/xray-flux\/","title":{"rendered":"Xray Flux"},"content":{"rendered":"<div class=\"responsive-tabs\">\n<h2 class=\"tabtitle\">Xray Flux<\/h2>\n<div class=\"tabcontent\">\n\n<div style=\"text-align: left\" class=\"iframe-container\">\n<!-- iframe plugin v.6.0 wordpress.org\/plugins\/iframe\/ -->\n<iframe src=\"https:\/\/spaceweather2.uit.no\/noswe\/pics\/xrays_24h_log.html\" width=\"100%\" height=\"580px\" 0=\"border:0\" 1=\"meta\" http-equiv=\"refresh\" content=\"600\" scrolling=\"yes\" class=\"iframe-class\" frameborder=\"0\"><\/iframe>\n<\/div>\n<div style=\"text-align: center\" class=\"iframe-container\">\n<!-- iframe plugin v.6.0 wordpress.org\/plugins\/iframe\/ -->\n<iframe src=\"https:\/\/spaceweather2.uit.no\/noswe\/pics\/xrays_48h_log.html\" width=\"100%\" height=\"580px\" 0=\"border:0\" 1=\"meta\" http-equiv=\"refresh\" content=\"600\" scrolling=\"yes\" class=\"iframe-class\" frameborder=\"0\"><\/iframe>\n<\/div>\n<p align=\"center\">Xrays<\/p>\n\n<\/div><h2 class=\"tabtitle\">Information<\/h2>\n<div class=\"tabcontent\">\n\n<p align=\"left\">The observed solar X-rays are a result of solar activity and solar flares. Solar flares are intense emissions of electromagnetic radiation from active regions on the Sun. Solar flares, especially larger flares, can be accompanied by coronal mass ejections (CMEs) and Solar Proton Events (SPEs). The increased X-ray flux from solar flares can cause absorption of HF radio signals on the sunlit side of the Earth with the largest solar flares causing complete HF blackout. Some large flares are also accompanied by broadband radio bursts that may cause problems for radar systems, satellite communication, and satellite navigation.<\/p>\n<p>The shown data are from NOAA GOES, and the NOAA Space Weather Prediction Center R-scale thresholds are indicated in the plots.<\/p>\n<\/div><\/div>\n","protected":false},"excerpt":{"rendered":"<p>Xrays The observed solar X-rays are a result of solar activity and solar flares. Solar flares are intense emissions of electromagnetic radiation from active regions on the Sun. Solar flares, especially larger flares, can be accompanied by coronal mass ejections (CMEs) and Solar Proton Events (SPEs). The increased X-ray flux &#8230;<\/p>\n","protected":false},"author":1082,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-5067","page","type-page","status-publish","hentry","column","threecol"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v28.8 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Xray Flux - Norwegian Centre for Space Weather (NOSWE)<\/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:\/\/site.uit.no\/spaceweather\/xray-flux\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Xray Flux - Norwegian Centre for Space Weather (NOSWE)\" \/>\n<meta property=\"og:description\" content=\"Xrays The observed solar X-rays are a result of solar activity and solar flares. 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