{"id":71,"date":"2019-02-14T19:24:40","date_gmt":"2019-02-14T17:24:40","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/solwindconnect\/?page_id=71"},"modified":"2019-02-14T19:24:40","modified_gmt":"2019-02-14T17:24:40","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<p>List of publications acknowledging our ISSI Team<\/p>\n<p><strong>T. S. Metcalfe &amp; R.\u00a0Egeland, 2019, ApJ, 871<\/strong><br \/>\nUnderstanding the Limitations of Gyrochronology for Old Field Stars, <a href=\"https:\/\/arxiv.org\/abs\/1811.11905\">ArXiv<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/#abs\/arXiv:1811.11905\">ADS<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2019ApJ...871...39M\/doi:10.3847\/1538-4357\/aaf575\">DOI<\/a><\/p>\n<p><strong>V. See, S. M. Matt et al., 2019, ApJ, 876<\/strong><br \/>\nEstimating Magnetic Filling Factors from Zeeman-Doppler Magnetograms, <a href=\"https:\/\/arxiv.org\/abs\/1903.05595\">ArXiv<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019ApJ...876..118S\/abstract\">ADS<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2019ApJ...876..118S\/doi:10.3847\/1538-4357\/ab1096\">DOI<\/a><\/p>\n<p><strong>S. Carolan, A.A. Vidotto, C. Loesch, P. Coogan, 2019, MNRAS, 489<br \/>\n<\/strong>The evolution of Earth\u2019s magnetosphere during the solar main sequence, <a href=\"https:\/\/arxiv.org\/abs\/1908.03537\">ArXiV<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019MNRAS.489.5784C\/abstract\">ADS<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2019MNRAS.489.5784C\/doi:10.1093\/mnras\/stz2422\">DOI<\/a><\/p>\n<p><strong>T. S. Metcalfe, O.\u00a0Kochukhov, I. V.\u00a0Ilyin, K. G.\u00a0Strassmeier, D.\u00a0Godoy-Rivera, M. H. Pinsonneault, 2019, ApJL, 887\u00a0<\/strong><br \/>\nLBT\/PEPSI Spectropolarimetry of a Magnetic Morphology Shift in Old Solar-type Stars, <a href=\"https:\/\/arxiv.org\/abs\/1912.01186\">ArXiV<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019ApJ...887L..38M\/abstract\">ADS<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2019ApJ...887L..38M\/doi:10.3847\/2041-8213\/ab5e48\">DOI<\/a><\/p>\n<p><strong>M. Shoda,\u00a0<\/strong><strong>T. K. Suzuki , S. P. Matt, S. R. Cranmer, A. A. Vidotto, A. Strugarek, V. See, V. R\u00e9ville, A. J. Finley, A. S. Brun, 2020, ApJ, 896<br \/>\n<\/strong>Alfv\u00e9n-wave-driven Magnetic Rotator Winds from Low-mass Stars. I. Rotation Dependences of Magnetic Braking and Mass-loss Rate, <a href=\"https:\/\/arxiv.org\/abs\/2005.09817\">ArXiV<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020arXiv200509817S\/abstract\">ADS<\/a>, <a href=\"https:\/\/doi.org\/10.3847\/1538-4357\/ab94bf\">DOI<\/a><\/p>\n<p class=\"s-abstract-title\"><strong>J. Ahuir, A.S. Brun, A. Strugarek, 2020, A&amp;A, 635, A170<\/strong><br \/>\nFrom stellar coronae to gyrochronology: A theoretical and observational exploration, <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2020A%26A...635A.170A\/EPRINT_HTML\">ArXiV<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020A%26A...635A.170A\/abstract\">ADS<\/a>, <a href=\"https:\/\/ui.adsabs.harvard.edu\/link_gateway\/2020A&amp;A...635A.170A\/doi:10.1051\/0004-6361\/201936974\">DOI<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"<p>List of publications acknowledging our ISSI Team T. S. Metcalfe &amp; R.\u00a0Egeland, 2019, ApJ, 871 Understanding the Limitations of Gyrochronology for Old Field Stars, ArXiv, ADS, DOI V. See, S. M. Matt et al., 2019, ApJ, 876 Estimating Magnetic Filling &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/solwindconnect\/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-71","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/pages\/71","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/comments?post=71"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/pages\/71\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/solwindconnect\/wp-json\/wp\/v2\/media?parent=71"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}