{"id":86,"date":"2018-01-31T17:25:04","date_gmt":"2018-01-31T15:25:04","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/observecoronloop\/?page_id=86"},"modified":"2018-01-31T17:25:04","modified_gmt":"2018-01-31T15:25:04","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<p>This page is regularly updated with the publications that acknowledge the ISSI team<br \/>\n<a href=\"https:\/\/ui.adsabs.harvard.edu\/public-libraries\/xOGW87IXR_q024SAU_Q-8A\" target=\"_blank\" rel=\"noopener noreferrer\">ADS library of the team publications<\/a><\/p>\n<p>&nbsp;<\/p>\n<p><span style=\"font-size: 14pt\"><strong>2020<\/strong><\/span><\/p>\n<h2 class=\"s-abstract-title\"><a href=\"http:\/\/aanda.org\/articles\/aa\/abs\/2020\/10\/aa38546-20\/aa38546-20.html\" target=\"_blank\" rel=\"noopener noreferrer\">Ubiquitous hundred-Gauss magnetic fields in solar spicules, A&amp;A, Volume 642, A61, 2020<\/a><\/h2>\n<p class=\"bold\"><span id=\"aa38546-20-author-1\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038546&amp;n=1\" data-hasqtip=\"5\" aria-describedby=\"qtip-5\">M. Kriginsky<\/span>, <span id=\"aa38546-20-author-2\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038546&amp;n=2\" data-hasqtip=\"1\">R. Oliver<\/span>, <span id=\"aa38546-20-author-3\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038546&amp;n=3\" data-hasqtip=\"0\">N. Freij<\/span>, <span id=\"aa38546-20-author-4\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038546&amp;n=4\" data-hasqtip=\"9\">D. Kuridze<\/span>, <span id=\"aa38546-20-author-5\" class=\"author\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038546&amp;n=5\" data-hasqtip=\"4\" aria-describedby=\"qtip-4\">A. Asensio Ramos<\/span>\u00a0and <span id=\"aa38546-20-author-6\" class=\"author author-orcid\" data-url=\"\/component\/author\/?dkey=10.1051\/0004-6361\/202038546&amp;n=6\" data-hasqtip=\"2\" aria-describedby=\"qtip-2\">P. Antolin<\/span><\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-354\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12.jpg\" alt=\"\" width=\"1200\" height=\"406\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12.jpg 1200w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12-300x102.jpg 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12-1024x346.jpg 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12-768x260.jpg 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/aa38546-20-fig12-500x169.jpg 500w\" sizes=\"auto, (max-width: 1200px) 100vw, 1200px\" \/><\/a><\/p>\n<h2 class=\"s-abstract-title\"><a href=\"https:\/\/www.nature.com\/articles\/s41550-020-1199-8\" target=\"_blank\" rel=\"noopener noreferrer\">Reconnection nanojets in the solar corona, Nature Astronomy, 2020<\/a><\/h2>\n<p>P. Antolin, P. Pagano, P. Testa, A. Petralia and F. Reale<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets-.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-355\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets-.png\" alt=\"\" width=\"1326\" height=\"741\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets-.png 1326w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets--300x168.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets--1024x572.png 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets--768x429.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2021\/01\/antolin_2020_nanojets--500x279.png 500w\" sizes=\"auto, (max-width: 1326px) 100vw, 1326px\" \/><\/a><\/p>\n<h2 class=\"s-abstract-title\"><a href=\"http:\/\/aanda.org\/articles\/aa\/abs\/2020\/07\/aa37899-20\/aa37899-20.html\" target=\"_blank\" rel=\"noopener noreferrer\">Self-consistent 3D radiative MHD simulations of coronal rain formation and evolution, A&amp;A, Volume 639, A20, 2020<\/a><\/h2>\n<p>P. Kohutova, P. Antolin, A. Popovas, M. Szydlarski, and V. H. Hansteen<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-344\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020.png\" alt=\"\" width=\"1651\" height=\"698\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020.png 1651w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020-300x127.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020-1024x433.png 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020-768x325.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020-1536x649.png 1536w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/05\/Fig1_Kohutova_2020-500x211.png 500w\" sizes=\"auto, (max-width: 1651px) 100vw, 1651px\" \/><\/a><\/p>\n<h1><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2020\/03\/aa36979-19\/aa36979-19.html\" target=\"_blank\" rel=\"noopener noreferrer\">Modelling the solar transition region using an adaptive conduction method, A&amp;A, Volume 635, A168, 2020<\/a><\/h1>\n<p>C. D. Johnston, P. J. Cargill, A. W. Hood, I. De Moortel, S. J. Bradshaw, and A. C. Vaseekar<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Screenshot-2020-02-10-at-16.40.35.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-321\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Screenshot-2020-02-10-at-16.40.35.png\" alt=\"\" width=\"786\" height=\"578\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Screenshot-2020-02-10-at-16.40.35.png 786w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Screenshot-2020-02-10-at-16.40.35-300x221.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Screenshot-2020-02-10-at-16.40.35-768x565.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Screenshot-2020-02-10-at-16.40.35-408x300.png 408w\" sizes=\"auto, (max-width: 786px) 100vw, 786px\" \/><\/a><\/p>\n<p><a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ab6bdc\" target=\"_blank\" rel=\"noopener noreferrer\"><strong>Electron Beams Cannot Directly Produce Coronal Rain, ApJ, Volume 890(2), 2020<\/strong><\/a><\/p>\n<p>J. W. Reep, P. Antolin, and S. J. Bradshaw<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-328\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4.png\" alt=\"\" width=\"938\" height=\"931\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4.png 938w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4-300x298.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4-150x150.png 150w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4-768x762.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2020\/02\/Fig4-302x300.png 302w\" sizes=\"auto, (max-width: 938px) 100vw, 938px\" \/><\/a><\/p>\n<h1><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2020\/02\/aa37078-19\/aa37078-19.html\" target=\"_blank\" rel=\"noopener noreferrer\">Two-dimensional simulations of coronal rain dynamics I. Model consisting of a vertical magnetic field and an unbounded atmosphere, A&amp;A, Volume 633, A36, 2020<\/a><\/h1>\n<p>D. Mart\u00ednez-G\u00f3mez, R. Oliver, E. Khomenko, M. Collados<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-303\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain.png\" alt=\"\" width=\"1493\" height=\"967\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain.png 1493w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain-300x194.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain-1024x663.png 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain-768x497.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/2D_rain-463x300.png 463w\" sizes=\"auto, (max-width: 1493px) 100vw, 1493px\" \/><\/a><\/p>\n<h2 class=\"s-abstract-title\"><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2020\/02\/aa35872-19\/aa35872-19.html\" target=\"_blank\" rel=\"noopener noreferrer\">Spectroscopic detection of coronal plasma flows in loops undergoing thermal non-equilibrium cycles, A&amp;A, Volume 633, A54, 2020<\/a><\/h2>\n<p>G. Pelouze, F. Auch\u00e8re, K. Bocchialini, C. Froment, S. Parenti, and E. Soubri\u00e9<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-309\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3.png\" alt=\"\" width=\"1454\" height=\"554\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3.png 1454w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3-300x114.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3-1024x390.png 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3-768x293.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/12\/fig3-500x191.png 500w\" sizes=\"auto, (max-width: 1454px) 100vw, 1454px\" \/><\/a><\/p>\n<h1><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2020\/01\/aa36717-19\/aa36717-19.html\" target=\"_blank\" rel=\"noopener noreferrer\">Multi-scale observations of thermal non-equilibrium cycles in coronal loops, A&amp;A, 633, A11, 2020<\/a><\/h1>\n<p>C. Froment, P. Antolin, V. M. J. Henriques, P. Kohutova, L. H. M. Rouppe van der Voort<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/figure_froment2019.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-305\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/figure_froment2019.png\" alt=\"\" width=\"503\" height=\"503\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/figure_froment2019.png 503w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/figure_froment2019-300x300.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/figure_froment2019-150x150.png 150w\" sizes=\"auto, (max-width: 503px) 100vw, 503px\" \/><\/a><\/p>\n<h1><a href=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6587\/ab5406\" target=\"_blank\" rel=\"noopener noreferrer\">Thermal instability and non-equilibrium in solar coronal loops: from coronal rain to long-period intensity pulsations, Plasma Phys. Control. Fusion, 62, 2020<\/a><\/h1>\n<p>P. Antolin<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/ppcfab5406f1_lr.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone size-full wp-image-298\" src=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/ppcfab5406f1_lr.jpg\" alt=\"\" width=\"725\" height=\"298\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/ppcfab5406f1_lr.jpg 725w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/ppcfab5406f1_lr-300x123.jpg 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/ppcfab5406f1_lr-500x206.jpg 500w\" sizes=\"auto, (max-width: 725px) 100vw, 725px\" \/><\/a><\/p>\n<p><span style=\"font-size: 14pt\"><strong>2019<\/strong><\/span><\/p>\n<h1><a href=\"https:\/\/link.springer.com\/article\/10.1007%2Fs11207-019-1562-z\" target=\"_blank\" rel=\"noopener noreferrer\">The Distinction Between Thermal Nonequilibrium and Thermal Instability, Solar Physics, 294, 173, 2019<\/a><\/h1>\n<p>J. A. Klimchuk<\/p>\n<h1><a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/ab41f4\" target=\"_blank\" rel=\"noopener noreferrer\">The Role of Asymmetries in Thermal Non-Equilibrium, The Astrophysical Journal, 884(1), 2019<\/a><\/h1>\n<p>J. A. Klimchuk and M. Luna<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/apjab41f4f3_hr.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-242 size-medium\" src=\"http:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/2019\/11\/apjab41f4f3_hr-300x242.jpg\" alt=\"\" width=\"300\" height=\"242\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/apjab41f4f3_hr-300x242.jpg 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/apjab41f4f3_hr-372x300.jpg 372w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/11\/apjab41f4f3_hr.jpg 600w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/a><\/p>\n<h1><a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2019\/05\/aa34742-18\/aa34742-18.html\" target=\"_blank\" rel=\"noopener noreferrer\">The effects of numerical resolution, heating timescales and background heating on thermal non-equilibrium in coronal loops, A&amp;A, Volume 625, 2019<\/a><\/h1>\n<p>C. D. Johnston, P. J. Cargill, P. Antolin, A. W. Hood, I. De Moortel, and S. J. Bradshaw<\/p>\n<p><a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/aa34742-18-fig3-e1565010079867.png\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-193 size-full\" src=\"http:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/2019\/06\/aa34742-18-fig3-e1565010079867.png\" alt=\"\" width=\"1118\" height=\"445\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/aa34742-18-fig3-e1565010079867.png 1118w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/aa34742-18-fig3-e1565010079867-300x119.png 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/aa34742-18-fig3-e1565010079867-1024x408.png 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/aa34742-18-fig3-e1565010079867-768x306.png 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/aa34742-18-fig3-e1565010079867-500x199.png 500w\" sizes=\"auto, (max-width: 1118px) 100vw, 1118px\" \/><\/a><\/p>\n<h1><a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ab0c1f\" target=\"_blank\" rel=\"noopener noreferrer\">A Fast and Accurate Method to Capture the Solar Corona\/Transition Region Enthalpy Exchange, The Astrophysical Journal Letters, 873(2), 2019<\/a><\/h1>\n<p>C. D. Johnston &amp; S. J. Bradshaw<\/p>\n<p><a href=\"https:\/\/iopscience.iop.org\/2041-8205\/873\/2\/L22\/suppdata\/apjlab0c1ff3_video.mp4\"><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-191 size-full\" src=\"http:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/2019\/06\/apjlab0c1ff3_hr-e1565010117532.jpg\" alt=\"\" width=\"1799\" height=\"1199\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/apjlab0c1ff3_hr-e1565010117532.jpg 1799w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/apjlab0c1ff3_hr-e1565010117532-300x200.jpg 300w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/apjlab0c1ff3_hr-e1565010117532-1024x682.jpg 1024w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/apjlab0c1ff3_hr-e1565010117532-768x512.jpg 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/apjlab0c1ff3_hr-e1565010117532-1536x1024.jpg 1536w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2019\/06\/apjlab0c1ff3_hr-e1565010117532-450x300.jpg 450w\" sizes=\"auto, (max-width: 1799px) 100vw, 1799px\" \/><\/a><\/p>\n<p><span style=\"font-size: 14pt\"><strong>2018<\/strong><\/span><\/p>\n<h1 class=\"single-entry-title\" style=\"text-align: left\"><a href=\"http:\/\/iopscience.iop.org\/article\/10.3847\/1538-4357\/aaa5a3\"><strong>The Coronal Monsoon: Thermal Nonequilibrium<br \/>\nRevealed by Periodic Coronal Rain, The Astrophysical Journal, 853(2), 2018<\/strong><\/a><\/h1>\n<p><span class=\"nowrap\">F. Auch\u00e8re<\/span>,\u00a0<span class=\"nowrap\">C. Froment<\/span>,\u00a0<span class=\"nowrap\">E. Soubri\u00e9<\/span>,\u00a0<span class=\"nowrap\">P. Antolin<\/span>,\u00a0<span class=\"nowrap\">R. Oliver\u00a0<\/span>and\u00a0<span class=\"nowrap\">G. Pelouze<\/span><a href=\"http:\/\/iopscience.iop.org\/0004-637X\/853\/2\/176\/suppdata\/apjaaa5a3f6_video.mp4\"><img loading=\"lazy\" decoding=\"async\" class=\"aligncenter wp-image-137 size-large\" src=\"http:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/2018\/09\/apjaaa5a3f6_hr-1018x1024.jpg\" alt=\"\" width=\"584\" height=\"587\" srcset=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2018\/09\/apjaaa5a3f6_hr-1018x1024.jpg 1018w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2018\/09\/apjaaa5a3f6_hr-298x300.jpg 298w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2018\/09\/apjaaa5a3f6_hr-150x150.jpg 150w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2018\/09\/apjaaa5a3f6_hr-768x772.jpg 768w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2018\/09\/apjaaa5a3f6_hr-1527x1536.jpg 1527w, https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-content\/uploads\/sites\/105\/2018\/09\/apjaaa5a3f6_hr-2036x2048.jpg 2036w\" sizes=\"auto, (max-width: 584px) 100vw, 584px\" \/><\/a><\/p>\n<h1 class=\"single-entry-title\" style=\"text-align: left\"><\/h1>\n","protected":false},"excerpt":{"rendered":"<p>This page is regularly updated with the publications that acknowledge the ISSI team ADS library of the team publications &nbsp; 2020 Ubiquitous hundred-Gauss magnetic fields in solar spicules, A&amp;A, Volume 642, A61, 2020 M. Kriginsky, R. Oliver, N. Freij, D. &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/observecoronloop\/publications\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":3,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-86","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/pages\/86","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/comments?post=86"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/pages\/86\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/observecoronloop\/wp-json\/wp\/v2\/media?parent=86"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}