{"id":146,"date":"2018-12-08T01:32:49","date_gmt":"2018-12-08T01:32:49","guid":{"rendered":"http:\/\/burnhamradioclub.co.uk\/?page_id=146"},"modified":"2019-10-24T21:27:44","modified_gmt":"2019-10-24T20:27:44","slug":"hf-propagation","status":"publish","type":"page","link":"https:\/\/burnhamradioclub.co.uk\/index.php\/transmission-modes\/hf-propagation\/","title":{"rendered":"Propagation"},"content":{"rendered":"<h2><a href=\"http:\/\/Eugene Parker proposed the idea of the solar wind, with the term 'magnetosphere' being proposed by Thomas Gold in 1959 to explain how the solar wind interacted with the Earth's magnetic field. The later mission of Explorer 12 in 1961 led by the Cahill and Amazeen observation in 1963 of a sudden decrease in magnetic field strength near the noon-time meridian, later was named the magnetopause. By 1983, the International Cometary Explorer observed the magnetotail, or the distant magnetic field.\" target=\"_blank\" rel=\"noopener noreferrer\">Ionosphere-and-Magnetosphere<\/a><\/h2>\n<p>&#8220;The<a href=\"https:\/\/en.wikipedia.org\/wiki\/Ionosphere\" target=\"_blank\" rel=\"noopener noreferrer\">\u00a0<b>ionosphere<\/b><\/a>\u00a0(<span class=\"nowrap\"><span class=\"IPA nopopups noexcerpt\"><a title=\"Help:IPA\/English\" href=\"https:\/\/en.wikipedia.org\/wiki\/Help:IPA\/English\">\/<span title=\"\/a\u026a\/: 'i' in 'tide'\">a\u026a<\/span><span title=\"\/\u02c8\/: primary stress follows\">\u02c8<\/span><span title=\"\/\u0252\/: 'o' in 'body'\">\u0252<\/span><span title=\"'n' in 'nigh'\">n<\/span><span title=\"\/\u0259\/: 'a' in 'about'\">\u0259<\/span><span title=\"\/\u02cc\/: secondary stress follows\">\u02cc<\/span><span title=\"'s' in 'sigh'\">s<\/span><span title=\"'f' in 'find'\">f<\/span><span title=\"\/\u026a\u0259r\/: 'ear' in 'near'\">\u026a\u0259r<\/span>\/<\/a><\/span><\/span><sup id=\"cite_ref-1\" class=\"reference\"><a href=\"https:\/\/en.wikipedia.org\/wiki\/Ionosphere#cite_note-1\">[1]<\/a><\/sup><sup id=\"cite_ref-2\" class=\"reference\"><a href=\"https:\/\/en.wikipedia.org\/wiki\/Ionosphere#cite_note-2\">[2]<\/a><\/sup>) is the ionized part of Earth&#8217;s upper\u00a0<a class=\"mw-redirect\" title=\"Earth's atmosphere\" href=\"https:\/\/en.wikipedia.org\/wiki\/Earth%27s_atmosphere\">atmosphere<\/a>, from about 60\u00a0km (37\u00a0mi) to 1,000\u00a0km (620\u00a0mi) altitude, a region that includes the\u00a0<a title=\"Thermosphere\" href=\"https:\/\/en.wikipedia.org\/wiki\/Thermosphere\">thermosphere<\/a>\u00a0and parts of the\u00a0<a title=\"Mesosphere\" href=\"https:\/\/en.wikipedia.org\/wiki\/Mesosphere\">mesosphere<\/a>\u00a0and\u00a0<a title=\"Exosphere\" href=\"https:\/\/en.wikipedia.org\/wiki\/Exosphere\">exosphere<\/a>. The ionosphere is\u00a0<a class=\"mw-redirect\" title=\"Ionized\" href=\"https:\/\/en.wikipedia.org\/wiki\/Ionized\">ionized<\/a>\u00a0by solar radiation. It plays an important role in\u00a0<a title=\"Atmospheric electricity\" href=\"https:\/\/en.wikipedia.org\/wiki\/Atmospheric_electricity\">atmospheric electricity<\/a>\u00a0and forms the inner edge of the\u00a0<a title=\"Magnetosphere\" href=\"https:\/\/en.wikipedia.org\/wiki\/Magnetosphere\">magnetosphere<\/a>. It has practical importance because, among other functions, it influences\u00a0<a title=\"Radio propagation\" href=\"https:\/\/en.wikipedia.org\/wiki\/Radio_propagation\">radio propagation<\/a>\u00a0to distant places on the\u00a0<a title=\"Earth\" href=\"https:\/\/en.wikipedia.org\/wiki\/Earth\">Earth<\/a><\/p>\n<p><a title=\"Eugene Parker\" href=\"https:\/\/en.wikipedia.org\/wiki\/Eugene_Parker\">Eugene Parker<\/a>\u00a0proposed the idea of the\u00a0<a title=\"Solar wind\" href=\"https:\/\/en.wikipedia.org\/wiki\/Solar_wind\">solar wind<\/a>, with the term &#8216;<a href=\"https:\/\/en.wikipedia.org\/wiki\/Magnetosphere\" target=\"_blank\" rel=\"noopener noreferrer\">magnetosphere<\/a>&#8216; being proposed by\u00a0<a title=\"Thomas Gold\" href=\"https:\/\/en.wikipedia.org\/wiki\/Thomas_Gold\">Thomas Gold<\/a>\u00a0in 1959 to explain how the solar wind interacted with the Earth&#8217;s magnetic field. The later mission of Explorer 12 in 1961 led by the Cahill and Amazeen observation in 1963 of a sudden decrease in magnetic field strength near the noon-time meridian, later was named the\u00a0<a title=\"Magnetopause\" href=\"https:\/\/en.wikipedia.org\/wiki\/Magnetopause\">magnetopause<\/a>. By 1983, the\u00a0<a title=\"International Cometary Explorer\" href=\"https:\/\/en.wikipedia.org\/wiki\/International_Cometary_Explorer\">International Cometary Explorer<\/a>observed the magnetotail, or the distant magnetic field.&#8221;<\/p>\n<h1><a title=\"Click to add Solar-Terrestrial Data to your website!\" href=\"http:\/\/www.hamqsl.com\/solar.html\"><img loading=\"lazy\" decoding=\"async\" class=\"alignleft\" src=\"http:\/\/www.hamqsl.com\/solarmap.php\" width=\"864\" height=\"432\" \/><\/a><\/h1>\n<h1><\/h1>\n<h1><a title=\"Click to add Solar-Terrestrial Data to your website!\" href=\"http:\/\/www.hamqsl.com\/solar.html\"><img decoding=\"async\" src=\"http:\/\/www.hamqsl.com\/solarsystem.php\" \/><\/a><\/h1>\n<h1 class=\"page-title\">Live solar data<\/h1>\n<p><a title=\"Solar information from N0NBH\" href=\"http:\/\/www.hamqsl.com\/solar.html\" target=\"_blank\" rel=\"noopener noreferrer\">Information from N0NBH<\/a><\/p>\n<p><center><br \/>\n<a title=\"Click to add Solar-Terrestrial Data to your website!\" href=\"http:\/\/www.hamqsl.com\/solar.html\"><img decoding=\"async\" src=\"http:\/\/www.hamqsl.com\/solar101vhf.php\" \/><\/a><\/center><center><br \/>\n<a title=\"Click to add Solar-Terrestrial Data to your website!\" href=\"http:\/\/www.hamqsl.com\/solar.html\"><img decoding=\"async\" src=\"http:\/\/www.hamqsl.com\/marston.php\" \/><\/a><\/center>You can also see solar images at the\u00a0<a title=\"SOHO satellite images by NASA\" href=\"http:\/\/soho.nascom.nasa.gov\/data\/realtime-images.html\" target=\"_blank\" rel=\"noopener noreferrer\">NASA website<\/a>.<\/p>\n<h1><img loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-15447\" src=\"https:\/\/rsgb.org\/main\/files\/2016\/07\/ITURHFProp.png\" sizes=\"auto, (max-width: 193px) 100vw, 193px\" srcset=\"https:\/\/rsgb.org\/main\/files\/2016\/07\/ITURHFProp.png 193w, https:\/\/rsgb.org\/main\/files\/2016\/07\/ITURHFProp-150x118.png 150w\" alt=\"ITURHFProp\" width=\"193\" height=\"152\" \/>\u00a0 \u00a0G4FKH\u2019s new propagation predictions tool Click the button below to start the application.<\/h1>\n<h1><a href=\"http:\/\/www.predtest.uk\/\" target=\"_blank\" rel=\"noopener noreferrer\"><button>Start Application<\/button><\/a><\/h1>\n<h1><\/h1>\n<p>&nbsp;<\/p>\n<div id=\"attachment_15447\" class=\"wp-caption alignleft\">\n<h3><a href=\"http:\/\/www.spacew.com\/www\/160pred.html\" target=\"_blank\" rel=\"noopener noreferrer\"><b><span style=\"font-family: 'Times New Roman', Times;\">160 Meter Radio Propagation Prediction Table<\/span><span style=\"font-family: Times New Roman,Times;\">\u00a0for\u00a0<\/span><\/b><b><span style=\"font-family: Times New Roman,Times;\">Middle and High Latitude Northern Hemisphere Circuits<\/span><\/b><\/a><\/h3>\n<p><a href=\"http:\/\/k9la.us\/NM7M_The_Little_Pistol_s_Guide_to_HF_Propagation.pdf\" target=\"_blank\" rel=\"noopener noreferrer\">The Little Pistol&#8217;s Guide\u00a0to HF Propagation<\/a><\/p>\n<p><a href=\"http:\/\/myplace.frontier.com\/~k9la\/NM7M_The_Big_Gun_s_Guide_to_Low-Band_Propagation.pdf\" target=\"_blank\" rel=\"noopener noreferrer\">The Big Gun&#8217;s Guide to Low-Band Propagation<\/a><\/p>\n<p><a href=\"http:\/\/www.infotechcomms.net\/Understanding_LF_and_HF_propagation.pdf\" target=\"_blank\" rel=\"noopener noreferrer\">Understanding LF and HF propagation<\/a><\/p>\n<p><a href=\"https:\/\/www.earth-prints.org\/bitstream\/2122\/820\/1\/15Warrington.pdf\" target=\"_blank\" rel=\"noopener noreferrer\">Propagation of HF radio waves over\u00a0northerly paths: measurements,\u00a0simulation and systems aspects<\/a><\/p>\n<p><a href=\"https:\/\/spaceweather.com\/\" target=\"_blank\" rel=\"noopener noreferrer\">Space weather<\/a><\/p>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<div class=\"mh-excerpt\"><p>Ionosphere-and-Magnetosphere &#8220;The\u00a0ionosphere\u00a0(\/a\u026a\u02c8\u0252n\u0259\u02ccsf\u026a\u0259r\/[1][2]) is the ionized part of Earth&#8217;s upper\u00a0atmosphere, from about 60\u00a0km (37\u00a0mi) to 1,000\u00a0km (620\u00a0mi) altitude, a region that includes the\u00a0thermosphere\u00a0and parts of the\u00a0mesosphere\u00a0and\u00a0exosphere. <a class=\"mh-excerpt-more\" href=\"https:\/\/burnhamradioclub.co.uk\/index.php\/transmission-modes\/hf-propagation\/\" title=\"Propagation\">[&#8230;]<\/a><\/p>\n<\/div>","protected":false},"author":1,"featured_media":0,"parent":85,"menu_order":4,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-146","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/pages\/146","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/comments?post=146"}],"version-history":[{"count":17,"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/pages\/146\/revisions"}],"predecessor-version":[{"id":149,"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/pages\/146\/revisions\/149"}],"up":[{"embeddable":true,"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/pages\/85"}],"wp:attachment":[{"href":"https:\/\/burnhamradioclub.co.uk\/index.php\/wp-json\/wp\/v2\/media?parent=146"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}