{"id":605679,"date":"2019-04-11T03:29:31","date_gmt":"2019-04-11T07:29:31","guid":{"rendered":"https:\/\/ntrs.nasa.gov\/search.jsp?R=20190002240"},"modified":"2019-04-11T03:29:31","modified_gmt":"2019-04-11T07:29:31","slug":"solar-flare-termination-shock-and-the-synthetic-fe-xxi-1354-08-a-line","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=605679","title":{"rendered":"Solar Flare Termination Shock and the Synthetic Fe XXI 1354.08 \u00c5 Line"},"content":{"rendered":"<p>Abstract: Solar flares are one of the most energetic phenomena occurred in the solar system. In the standard solar flare model, a fast mode shock, which is often referred to as the flare termination shock (TS), can exist above the loop-top source of hard X-ray emissions. The existence of the termination shock has been recently related to spectral hardening of flare hard X-ray spectrum at energies > 300 keV. Observations of the Fe XXI 1354.08 \u00c5 line during solar flares by the IRIS spacecraft have found &#8230;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Abstract: Solar flares are one of the most energetic phenomena occurred in the solar system. In the standard solar flare model, a fast mode shock, which is often referred to as the flare termination shock (TS), can exist above the loop-top source of hard X-ray emissions. The existence of the termination shock has been recently related to spectral hardening of flare hard X-ray spectrum at energies &gt; 300 keV. Observations of the Fe XXI 1354.08 &Aring; line during solar flares by the IRIS spacecraft have found &#8230;<\/p>\n","protected":false},"author":60,"featured_media":615444,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[],"tags":[],"class_list":["post-605679","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry"],"_links":{"self":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/605679","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/users\/60"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=605679"}],"version-history":[{"count":2,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/605679\/revisions"}],"predecessor-version":[{"id":609281,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/posts\/605679\/revisions\/609281"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=\/wp\/v2\/media\/615444"}],"wp:attachment":[{"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=605679"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=605679"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceweekly.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=605679"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}