{"id":19,"date":"2015-04-17T11:10:07","date_gmt":"2015-04-17T11:10:07","guid":{"rendered":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/?page_id=19"},"modified":"2025-07-02T09:59:22","modified_gmt":"2025-07-02T09:59:22","slug":"publications","status":"publish","type":"page","link":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/publications\/","title":{"rendered":"Publications"},"content":{"rendered":"<h3>Refereed journal articles<\/h3>\n<ul>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025ApJ...984...83L\/abstract\">&#8220;Vortex avalanches and collective motion in neutron stars&#8221;<\/a>, Liu, Baggaley, Barenghi &amp; Wood, 2025, ApJ, 984, 83<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2025NatAs...9..541I\/abstract\">&#8220;A connection between proto-neutron-star Tayler\u2013Spruit dynamos and low-field magnetars&#8221;<\/a>, Igoshev, Barr\u00e8re, Raynaud, Guilet, Wood &amp; Hollerbach, 2025, Nat. Astron., 9, 541<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2024MNRAS.535...78D\/abstract\">&#8220;Shear-driven magnetic buoyancy in the solar tachocline: dependence of the mean electromotive force on diffusivity and latitude&#8221;<\/a>, Duguid, Bushby &amp; Wood, 2024, MNRAS, 535, 78<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2024JFM...994A...3H\/abstract\">&#8220;Stratified resistive tearing instability&#8221;<\/a>, Hopper, Wood &amp; Bushby, 2024, JFM, 994, A3<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2024JLTP..215..376L\/abstract\">&#8220;Vortex depinning in a two-dimensional superfluid&#8221;<\/a>, Liu, Prasad, Baggaley, Barenghi &amp; Wood, 2024, JLTP, 215, 376<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023MNRAS.525.3354I\/abstract\">&#8220;Three-dimensional magnetothermal evolution of off-centred dipole magnetic field configurations in neutron stars&#8221;<\/a>, Igoshev, Hollerbach &amp; Wood, 2023, MNRAS, 525, 3354<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023GApFD.117..263M\/abstract\">&#8220;Self-adjointness of sound-proof models for magnetic buoyancy&#8221;<\/a>, Moss, Wood &amp; Bushby, 2023, GAFD, 117, 263<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2023MNRAS.520..527D\/abstract\">&#8220;Shear-driven magnetic buoyancy in the solar tachocline: the mean electromotive force due to rotation&#8221;<\/a>, Duguid, Bushby &amp; Wood, 2023, MNRAS, 520, 527<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022PhRvF...7j3701M\/abstract\">&#8220;Validity of sound-proof approximations for magnetic buoyancy&#8221;<\/a>, Moss, Wood &amp; Bushby, 2022, PRFluids, 7, 103701<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022ApJ...936...99D\/abstract\">&#8220;Three-dimensional Magnetothermal Simulations of Magnetar Outbursts&#8221;<\/a>, De Grandis, Turolla, Taverna, Lucchetta, Wood &amp; Zane, 2022, ApJ, 936, 99<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/jov.arvojournals.org\/article.aspx?articleid=2783542\">&#8220;Seeing the future: Predictive control in neural models of ocular accommodation&#8221;<\/a>, Read, Kaspiris-Rousellis, Wood, Wu, Vlaskamp &amp; Schor, 2022, JoV, 22, 4<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022Univ....8..228W\/abstract\">&#8220;Superconducting phases in neutron star cores&#8221;<\/a>, Wood &amp; Graber, 2022, Universe, 8, 228<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022JFM...936A..14S\/abstract\">&#8220;A hybrid pseudo-incompressible\u2013hydrostatic model&#8221;<\/a>, Snodin &amp; Wood, 2022, JFM, 936, A14<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2022Chmsp.29132686D\/abstract\">&#8220;A scalable model of fluid flow, substrate removal and current production in microbial fuel cells&#8221;<\/a>, Day, Heidrich &amp; Wood, 2022, Chemosphere, 291, 132686<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021ApJ...914..118D\/abstract\">&#8220;X-Ray emission from isolated neutron stars revisited: 3D magnetothermal simulations&#8221;<\/a>, De Grandis, Taverna, Turolla, Gnarini, Popov, Zane &amp; Wood, 2021, ApJ, 914, 118<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2021NatAs...5..145I\/abstract\">&#8220;Strong toroidal magnetic fields required by quiescent X-ray emission of magnetars&#8221;<\/a>, Igoshev, Hollerbach, Wood &amp; Gourgouliatos, 2021, Nat. Astron., 5, 145<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020ApJ...903...40D\">&#8220;3D modelling of magneto-thermal evolution of neutron stars: method and test cases&#8221;<\/a>, De Grandis, Turolla, Wood, Zane, Taverna &amp; Gourgouliatos, 2020, ApJ, 903, 40<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2020PhRvF...5d3702S\">&#8220;On the saturation mechanism of the fluctuation dynamo at Pr_M \u2265 1&#8221;<\/a>, Seta, Bushby, Shukurov &amp; Wood, 2020, PRFluids, 5, 043702<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2019PhRvB.100b4505W\">&#8220;Quasiperiodic boundary conditions for three-dimensional superfluids&#8221;<\/a>, Wood, Mesgarnezhad, Stagg &amp; Barenghi, 2019, PRB, 100, 024505<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2018ApJ...853...97W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;A self-consistent model of the solar tachocline&#8221;<\/a>, Wood &amp; Brummell, 2018, ApJ, 853, 97<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2018MNRAS.473.4544S\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Relative distribution of cosmic rays and magnetic fields&#8221;<\/a>, Seta, Shukurov, Wood, Bushby, &amp; Snowdin, 2017, MNRAS, 473, 4544<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017ApJ...839L..16S\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Cosmic rays in intermittent magnetic fields&#8221;<\/a>, Shukurov, Snodin, Seta, Bushby, &amp; Wood, 2017, ApJL, 839, 16<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016JFM...803..502W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Oscillatory convection and limitations of the Boussinesq approximation&#8221;<\/a>, Wood &amp; Bushby, 2016, JFM, 803, 502<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2016PNAS..113.3944G\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Magnetic field evolution in magnetar crusts through three-dimensional simulations&#8221;<\/a>, Gourgouliatos, Wood &amp; Hollerbach, 2016, PNAS, 113, 3944<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015PhRvL.114s1101W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Three-dimensional simulation of the magnetic stress in a neutron star crust&#8221;<\/a>, Wood &amp; Hollerbach, 2015, PRL, 114, 191101<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2014PhPl...21e2110W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Density-shear instability in electron magneto-hydrodynamics&#8221;<\/a>, Wood, Hollerbach, &amp; Lyutikov, 2014, PoP, 21, 052110<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2013PhRvE..88e3010G\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Effect of metallic walls on dynamos generated by laminar boundary-driven flow in a spherical domain&#8221;<\/a>, Guervilly, Wood, &amp; Brummell, 2013, PRE, 88, 053010<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2013ApJ...773..169V\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Energy conservation and gravity waves in sound-proof treatments of stellar interiors: II. Lagrangian constrained analysis&#8221;<\/a>, Vasil, Leocanet, Brown, Wood, &amp; Zweibel, 2013, ApJ, 773, 169<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2013ApJ...768..157W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;A new model for mixing by double-diffusive convection (semi-convection): II. The transport of heat and composition through layers&#8221;<\/a>, Wood, Garaud, &amp; Stellmach, 2013, ApJ, 768, 157<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2013MNRAS.434..720A\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Dynamics of the solar tachocline: III. Numerical solutions of the Gough and McIntyre model&#8221;<\/a>, Acevedo-Arreguin, Garaud, &amp; Wood, 2013, MNRAS, 434, 720<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2012ApJ...755...99W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Transport by meridional circulations in solar-type stars&#8221;<\/a>, Wood &amp; Brummell, 2012, ApJ, 755, 99<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2012ApJ...750...61M\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;A new model for mixing by double-diffusive convection (semi-convection): I. The conditions for layer formation&#8221;<\/a>, Mirouh, Garaud, Stellmach, Traxler, &amp; Wood, 2012, ApJ, 750, 61<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2011ApJ...738...47W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;The Sun&#8217;s meridional circulation and interior magnetic field&#8221;<\/a>, Wood, McCaslin, &amp; Garaud, 2011, ApJ, 738, 47<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2011JFM...677..445W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Polar confinement of the Sun&#8217;s interior magnetic field by laminar magnetostrophic flow&#8221;<\/a>, Wood &amp; McIntyre, 2011, JFM, 677, 445<\/li>\n<\/ul>\n<h3>Conference proceedings<\/h3>\n<ul>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2011IAUS..271..409\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Magnetic confinement in the solar interior&#8221;<\/a>, Wood, 2011, Proceedings of IAU Symposium 271, 409<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/hdl.handle.net\/1912\/2803\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Crumpling of a thin ice sheet due to incident flow&#8221;<\/a>, Wood, 2008, Proceedings of the Woods Hole GFD program<\/li>\n<li style=\"margin-top: 0.5em\"><a href=\"http:\/\/adsabs.harvard.edu\/abs\/2007AIPC..948..303W\" target=\"_blank\" rel=\"noopener noreferrer\">&#8220;Confinement of the Sun&#8217;s interior magnetic field: some exact boundary-layer solutions&#8221;<\/a>, Wood &amp; McIntyre, 2007, IAU Conference Proceedings, 948, 303<\/li>\n<\/ul>\n<h3>PhD thesis<\/h3>\n<ul>\n<li style=\"margin-top: 0.5em\">&#8220;The solar tachocline: A self-consistent model of magnetic confinement&#8221;, Wood, 2010, University of Cambridge<\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>Refereed journal articles &#8220;Vortex avalanches and collective motion in neutron stars&#8221;, Liu, Baggaley, Barenghi &amp; Wood, 2025, ApJ, 984, 83 &#8220;A connection between proto-neutron-star Tayler\u2013Spruit dynamos and low-field magnetars&#8221;, Igoshev, Barr\u00e8re, Raynaud, Guilet, Wood &amp; Hollerbach, 2025, Nat. Astron., 9, 541 &#8220;Shear-driven magnetic buoyancy in the solar tachocline: dependence of the mean electromotive force on &hellip; <a href=\"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/publications\/\" class=\"more-link\">Continue reading <span class=\"screen-reader-text\">Publications<\/span> <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":874,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"open","ping_status":"open","template":"","meta":{"footnotes":""},"class_list":["post-19","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/pages\/19","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/users\/874"}],"replies":[{"embeddable":true,"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/comments?post=19"}],"version-history":[{"count":35,"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/pages\/19\/revisions"}],"predecessor-version":[{"id":141,"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/pages\/19\/revisions\/141"}],"wp:attachment":[{"href":"https:\/\/www.staff.ncl.ac.uk\/toby.wood\/wp-json\/wp\/v2\/media?parent=19"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}