{"id":106,"date":"2018-05-25T16:35:27","date_gmt":"2018-05-25T14:35:27","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/solheliomagnet\/?page_id=106"},"modified":"2018-05-25T16:35:27","modified_gmt":"2018-05-25T14:35:27","slug":"list-of-publications-by-the-team","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/list-of-publications-by-the-team\/","title":{"rendered":"List of publications by the team"},"content":{"rendered":"<ol reversed=\"\">\n<li>T\u00e4htinen, I., Virtanen, I.I., Pevtsov, A.A., and Mursula, K.: 2022, <strong>Reconstructing solar magnetic fields from historical observations VIII. AIA 1600 \u00c5 contrast as a proxy of solar magnetic fields<\/strong>\u201c, Astron. Astrophys., <strong>664<\/strong>, A2, 26 pp., DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/202141164\">10.1051\/0004-6361\/202141164<\/a><\/li>\n<li>Penza, V., Berrilli, F., Bertello, L., Cantoresi, M., Criscuoli, S., 2021, &#8220;<strong>Prediction of Sunspot and Plage Coverage for Solar Cycle 25<\/strong>&#8220;, Astrophys. J., <strong>922<\/strong>. DOI: <a href=\"https:\/\/doi.org\/10.3847\/2041-8213\/ac3663\">10.3847\/2041-8213\/ac3663<\/a><\/li>\n<li>Bertello. L., Pevtsov, A.A., Ulrich, R.: 2020, \u201c<strong>70 Years of Chromospheric Solar Activity and Dynamics<\/strong>\u201c, Astrophys. J., <b>897<\/b> 181, DOI: <a href=\"https:\/\/doi.org\/10.3847\/1538-4357\/ab9746\">10.3847\/1538-4357\/ab9746<\/a><\/li>\n<li>Virtanen, I.O.I. , I.I. Virtanen, A.A.\u00a0Pevtsov, and K. Mursula: 2019, \u201c<strong>Reconstructing solar magnetic fields from historical observations. VI. Axial dipole moments of solar active regions of cycles 21-24 <\/strong>\u201c, Astron. Astrophys., <strong>632<\/strong>, A39, 7pp, DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201936134\">10.1051\/0004-6361\/201936134<\/a><\/li>\n<li>Virtanen, I.I., Pevtsov, A.A., and K. Mursula: 2019, &#8220;<strong>Photospheric and coronal magnetic fields in six magnetographs. III. Photospheric and coronal magnetic fields in 1974-2017<\/strong>&#8220;, Astron. Astrophys., <strong>626<\/strong>, A67, DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201935713\">10.1051\/0004-6361\/201935713<\/a><\/li>\n<li>Chatzistergos, T., Ermolli, I., Krivova, N. A., and Solanki, S.K.: 2019, &#8220;<strong>Analysis of full disc Ca II K spectroheliograms. II. Towards an accurate assessment of long-term variations in plage areas<\/strong>&#8220;, Astron. Astrophys., <strong>625<\/strong>, A69, DOI:\u00a0 <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201834402\">10.1051\/0004-6361\/201834402<\/a><\/li>\n<li>Pevtsov, A.A., Tlatova, K.A., Pevtsov, A.A., Heikkinen, E., Virtanen, I.,\u00a0 Karachik, N.V., Bertello, L., Tlatov, A.G., Ulrich, R., Mursula, K.: 2019, &#8220;<strong>Reconstructing solar magnetic fields from historical observations. V. Sunspot magnetic field measurements at Mount Wilson Observatory<\/strong>&#8220;, Astron. Astrophys., <strong>628<\/strong>, A103, 14pp, DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201834985\">10.1051\/0004-6361\/201834985<\/a>, Arxiv: <a href=\"https:\/\/arxiv.org\/abs\/1907.06492\">1907.06492<\/a><\/li>\n<li>Virtanen, I. I., Pevtsov, A.A.,\u00a0 and Mursula, K.: 2019, &#8220;<strong>Structure and evolution of the photospheric magnetic field in 2010 &#8211; 2017: Comparison of SOLIS\/VSM vector field and B<sub>LOS<\/sub> potential field<\/strong>&#8220;,\u00a0 Aston. Astrophys., <strong>624<\/strong>, A73, DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201834895\">10.1051\/0004-6361\/201834895<\/a><\/li>\n<li>Virtanen, I.O.I. , Virtanen, I.I., Pevtsov, A.A., Bertello, L., Yeates, A.,\u00a0 and Mursula, K.: 2019, <strong>&#8220;Reconstructing solar magnetic fields from historical observations. IV. Testing the reconstruction method<\/strong>&#8220;, Astron. Astrophysics, DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201935606\">10.1051\/0004-6361\/201935606<\/a><\/li>\n<li>Chatterjee, S.; Banerjee, D., McIntosh, S. W., Leamon, R. J.; Dikpati, M., Srivastava, A. K., Bertello, L.: 2019. <strong>&#8220;Signature of Extended Solar Cycles as Detected from Ca II K Synoptic Maps of Kodaikanal and Mount Wilson Observatory&#8221;<\/strong>, Astrophys. J. Letters, <strong>874<\/strong>, Issue 1, article id. L4, DOI: <a href=\"https:\/\/doi.org\/10.3847\/2041-8213\/ab0e0e\">10.3847\/2041-8213\/ab0e0e<\/a><\/li>\n<li>Tlatova, K., Tlatov, A., Pevtsov, A., Mursula, K., Vasil&#8217;eva, V., Heikkinen, E., Bertello, L.,\u00a0 Pevtsov, A., Virtanen, I., and Karachik, N.: 2018, &#8220;<strong>Tilt of sunspot bipoles in solar cycles 15 to 24<\/strong>&#8220;, Solar Phys., , <strong>293<\/strong>:118, DOI: <a href=\"http:\/\/doi.org\/10.1007\/s11207-018-1337-y\">10.1007\/s11207-018-1337-y<\/a><\/li>\n<li>Virtanen, I.O.I., Virtanen, I.I., Pevtsov, A.A., and Mursula, K.: 2018, &#8220;<strong>Reconstructing solar magnetic fields from historical observations. III. Activity in one hemisphere is sufficient to maintain the magnetic cycle in both hemispheres<\/strong>&#8220;, Astron. Astrophys., <strong>616<\/strong>, A134, DOI: <a href=\"https:\/\/doi.org\/10.1051\/0004-6361\/201732323\">10.1051\/0004-6361\/201732323<\/a><\/li>\n<\/ol>\n","protected":false},"excerpt":{"rendered":"<p>T\u00e4htinen, I., Virtanen, I.I., Pevtsov, A.A., and Mursula, K.: 2022, Reconstructing solar magnetic fields from historical observations VIII. AIA 1600 \u00c5 contrast as a proxy of solar magnetic fields\u201c, Astron. Astrophys., 664, A2, 26 pp., DOI: 10.1051\/0004-6361\/202141164 Penza, V., Berrilli, &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/list-of-publications-by-the-team\/\">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-106","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/pages\/106","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/comments?post=106"}],"version-history":[{"count":0,"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/pages\/106\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/solheliomagnet\/wp-json\/wp\/v2\/media?parent=106"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}