{"id":46,"date":"2015-07-20T14:51:47","date_gmt":"2015-07-20T13:51:47","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/solarchromosphere\/?page_id=46"},"modified":"2015-07-20T14:51:47","modified_gmt":"2015-07-20T13:51:47","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<p>A giant quiescent solar filament observed with high-resolution spectroscopy<br \/>\n<a href=\"http:\/\/dx.doi.org\/10.1051\/0004-6361\/201526636\">http:\/\/dx.doi.org\/10.1051\/0004-6361\/201526636<\/a><\/p>\n<p>Continuum Enhancements in the Ultraviolet, the Visible and the Infrared during the X1 Flare on 2014 March 29<br \/>\n<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016ApJ...816...88K\">http:\/\/adsabs.harvard.edu\/abs\/2016ApJ&#8230;816&#8230;88K<\/a><\/p>\n<p>Multiwavelength Observations of a Slow-rise, Multistep X1.6 Flare and the Associated Eruption<br \/>\n<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015ApJ...812..172Y\">http:\/\/adsabs.harvard.edu\/abs\/2015ApJ&#8230;812..172Y<\/a><\/p>\n<p>Formation and Eruption of a Small Flux Rope in the Chromosphere Observed by NST, IRIS, and SDO<br \/>\n<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015ApJ...809...83K\">http:\/\/adsabs.harvard.edu\/abs\/2015ApJ&#8230;809&#8230;83K<\/a><\/p>\n<p>The Fast Filament Eruption Leading to the X-flare on 2014 March 29<br \/>\n<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015ApJ...806....9K\" target=\"_blank\" rel=\"noopener\"> http:\/\/adsabs.harvard.edu\/abs\/2015ApJ&#8230;806&#8230;.9K<\/a><\/p>\n<p>The Role of Partial Ionization Effects in the Chromosphere<br \/>\n<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015RSPTA.37340268M\">http:\/\/adsabs.harvard.edu\/abs\/2015RSPTA.37340268M<\/a><\/p>\n<p>Comparison of inversion codes for polarized line formation in MHD simulations. I. Milne-Eddington codes<br \/>\n<a href=\"http:\/\/adsabs.harvard.edu\/abs\/2014A%26A...572A..54B\" target=\"_blank\" rel=\"noopener\"> http:\/\/adsabs.harvard.edu\/abs\/2014A%26A&#8230;572A..54B<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>A giant quiescent solar filament observed with high-resolution spectroscopy http:\/\/dx.doi.org\/10.1051\/0004-6361\/201526636 Continuum Enhancements in the Ultraviolet, the Visible and the Infrared during the X1 Flare on 2014 March 29 http:\/\/adsabs.harvard.edu\/abs\/2016ApJ&#8230;816&#8230;88K Multiwavelength Observations of a Slow-rise, Multistep X1.6 Flare and the Associated &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/publications\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-46","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/pages\/46","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/comments?post=46"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/pages\/46\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/solarchromosphere\/wp-json\/wp\/v2\/media?parent=46"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}