{"id":25,"date":"2019-08-29T11:57:35","date_gmt":"2019-08-29T09:57:35","guid":{"rendered":"http:\/\/www.issibern.ch\/teams\/solactregars\/?page_id=25"},"modified":"2023-12-06T08:26:11","modified_gmt":"2023-12-06T08:26:11","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.issibern.ch\/teams\/solactregars\/main-page\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"\r\n<p>Publications resulting from ISSI Team project 474 with ISSI acknowledgement:<\/p>\r\n<p>[1] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020JSWSC..10...50P\/abstract\">Petrovay, Nagy &amp; Yeates: Towards an algebraic method of solar cycle prediction I: Calculating the ultimate dipole contributions of individual active regions<\/a>. J. Space Weather Space Clim. 10, 50 (2020)<\/p>\r\n<p>[2] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020JSWSC..10...46N\/abstract\">Nagy, Petrovay, Lemerle &amp; Charbonneau: Towards an algebraic method of solar cycle prediction II: Reducing the need for detailed input data with ARDoR<\/a>. J. Space Weather Space Clim. 10, 46 (2020)<\/p>\r\n<p>[3] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020JSWSC..10...62N\/abstract\">Nagy, Lemerle &amp; Charbonneau:\u00a0 Impact of nonlinear surface inflows into activity belts on the solar dynamo.<\/a>\u00a0 J. Space Weather Space Clim. 10, 62 (2020)<\/p>\r\n<p>[4] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020SoPh..295..119Y\/abstract\">Yeates: How good is the bipolar approximation of active regions for surface flux transport?<\/a>\u00a0 Solar Phys., 295, 119 (2020)<\/p>\r\n<p>[5] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...900...19J\/abstract\">Jiang: Non-linear mechanisms that regulate the solar cycle amplitude.<\/a> Astrophys. J. 900, 19 (2020)<\/p>\r\n<p>[6] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...901L..35K\/abstract\">Karak: Dynamo saturation through the latitudinal variation of bipolar magnetic regions in the Sun.<\/a> Astrophys. J. 901, L35 (2020)<\/p>\r\n<p>[7] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...904...62W\/abstract\">Wang, Jiang, Zhang &amp; Wang: Activity complexes and a prominent poleward surge during Solar Cycle 24.<\/a> Astrophys. J. 904, 62 (2020)<\/p>\r\n<p>[8] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021A%26A...650A..87W\/abstract\">Wang, Jiang &amp; Wang: Algebraic quantification of an active region contribution to the solar cycle.<\/a> Astron. Astrophys. 650, A87 (2021)<\/p>\r\n<p>[9] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021ApJ...909...87K\/abstract\">Kumar, Karak, Nagy, Lemerle, Petrovay: The polar precursor method for solar cycle prediction: Comparison of predictors and their temporal range.<\/a> Astrophys. J. 909, 87 (2021)<\/p>\r\n<p>[10] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021A%26A...653A..27J\/abstract\">Jiao, Jiang &amp; Wang: Sunspot tilt angles revisited: Dependence on the solar cycle strength.<\/a> Astron. Astrophys.\u00a0 653, 27 (2021)<\/p>\r\n<p>[11] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021arXiv211214465T\/abstract\">Talafha, Nagy, Lemerle, Petrovay: The role of observable nonlinearities in solar cycle modulation. <\/a>Astron. Astrophys. 660, A92 (2022)<\/p>\r\n<p>[12] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023JASTP.24306018J\/abstract\">Jiang, Zhang &amp; Petrovay: Comparison of physics-based prediction models of solar cycle 25. <\/a>Journal of Atmospheric and Solar-Terrestrial Physics 243, 106018 (2023)<\/p>\r\n<p>[13] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023SSRv..219...19B\/abstract\">Biswas, Karak, Usoskin &amp; Weisshaar: Long-term modulation of solar cycles.<\/a> Space Sci. Res. 219, 19 (2023)<\/p>\r\n<p>[14] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023SSRv..219...31Y\/abstract\">Yeates, Cheung, Jiang, Petrovay &amp; Wang: Surface flux transport on the Sun.<\/a> Space Sci. Res. 219, 31 (2023)<\/p>\r\n<p>[15] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023MNRAS.526.3994B\/abstract\">Biswas, Karak &amp; Kumar: Exploring the reliability of polar field rise rate as a precursor for an early prediction of solar cycle.<\/a> Mon.Not. Roy. Ast. Soc.\u00a0 526, 3994 (2023)<\/p>\r\n<p>[16] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023ApJS..268...55W\/abstract\">Wang, Jiang &amp; Luo: Toward a live homogeneous database of solar active regions based on SOHO\/MDI and SDO\/HMI synoptic magnetograms. I. Automatic detection and calibration.<\/a> Astrophys. J.\u00a0 Suppl. 268, 55 (2023)<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>[17] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023ApJS..268...58S\/abstract\">Sreedevi, Jha, Karak &amp; Banerjee : AutoTAB: Automatic Tracking Algorithm for Bipolar Magnetic Regions.<\/a> Astrophys. J.\u00a0 Suppl. 268, 58 (2023)<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>[18] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023ApJ...953...51P\/abstract\">Pal, Bhowmik, Mahajan &amp; Nandy : Impact of anomalous active regions on the large-scale magnetic field of the Sun.<\/a> Astrophys. J.\u00a0 953, 51 (2023)<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>[19] <a href=\"https:\/\/www.aanda.org\/articles\/aa\/abs\/2023\/12\/aa47536-23\/aa47536-23.html\">Chatzistergos et al. : Analysis of full-disc H alpha observations: Carrington maps and filament properties in 1909-2022.<\/a> Astron. Astrophys.\u00a0 680, A15 (2023)<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>[20] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023arXiv231118800K\/abstract\">Kirti Mishra, Routh, Jha, Chatzistergos, Basu, Chatterjee, Banerjee &amp; Ermolli: Differential rotation of the solar chromosphere: A century-long perspective from Kodaikanal Solar Observatory Ca II K data.<\/a> Astrophys. J.\u00a0 accepted (2023)<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>[21] <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2024MNRAS.528L..27J\/abstract\">Jaswal, Saha &amp; Nandy: Discovery of a relation between the decay rate of the Sun&#8217;s magnetic dipole and the growth rate of the following sunspot cycle: a new precursor for solar cycle prediction.<\/a> Mon.Not. Roy. Ast. Soc.\u00a0 528, L27 (2024)<\/p>\r\n<p>&nbsp;<\/p>\r\n<p>&nbsp;<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<p>A BibTeX entry for these pages:<\/p>\r\n<p>\r\n\r\n<\/p>\r\n<pre>@webpage{Petrovayetal2019,<br \/>\r\n    Author = {{Petrovay}, K., {Cameron}, R.~H., {Charbonneau}, P., {Jiang}, J., {Karak}, B.~B., {Lemerle}, A., {Mursula}, K., {Nagy}, M., {Norton}, A.~A., {Upton}, L., {Virtanen}, Ilpo, {Virtanen}, Iiro, {Yeates}, A.},<br \/>\r\n    Title = {ISSI Team - What Determines The Dynamo Effectivity Of Solar Active Regions?},<br \/>\r\n    Url = {http:\/\/www.issibern.ch\/teams\/solactregars\/},<br \/>\r\n    Year = {2019}}<\/pre>\r\n<p>\r\n\r\n<\/p>\r\n<pre class=\"wp-block-preformatted\">\u00a0<\/pre>\r\n<p><\/p>\r\n<div class=\"notranslate\">\u00a0<\/div>","protected":false},"excerpt":{"rendered":"<p>Publications resulting from ISSI Team project 474 with ISSI acknowledgement: [1] Petrovay, Nagy &amp; Yeates: Towards an algebraic method of solar cycle prediction I: Calculating the ultimate dipole contributions of individual active regions. J. Space Weather Space Clim. 10, 50 &hellip; <a href=\"https:\/\/www.issibern.ch\/teams\/solactregars\/main-page\/publications\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":2,"featured_media":14,"parent":269,"menu_order":3,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-25","page","type-page","status-publish","has-post-thumbnail","hentry"],"_links":{"self":[{"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/pages\/25","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/comments?post=25"}],"version-history":[{"count":7,"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/pages\/25\/revisions"}],"predecessor-version":[{"id":452,"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/pages\/25\/revisions\/452"}],"up":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/pages\/269"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/media\/14"}],"wp:attachment":[{"href":"https:\/\/www.issibern.ch\/teams\/solactregars\/wp-json\/wp\/v2\/media?parent=25"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}