{"id":5,"date":"2024-09-30T16:27:13","date_gmt":"2024-09-30T15:27:13","guid":{"rendered":"https:\/\/blogs.ncl.ac.uk\/gafd\/?page_id=5"},"modified":"2026-01-19T13:02:18","modified_gmt":"2026-01-19T13:02:18","slug":"gafd-group","status":"publish","type":"page","link":"https:\/\/blogs.ncl.ac.uk\/gafd\/gafd-group\/","title":{"rendered":"Group members"},"content":{"rendered":"\n<div class=\"wp-block-media-text is-stacked-on-mobile is-vertically-aligned-top\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"367\" height=\"461\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/CFB-2015.jpg\" alt=\"\" class=\"wp-image-70 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/CFB-2015.jpg 367w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/CFB-2015-239x300.jpg 239w\" sizes=\"auto, (max-width: 367px) 100vw, 367px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\"><strong><a href=\"http:\/\/www.mas.ncl.ac.uk\/~ncfb\/\">Prof Carlo Barenghi<\/a><\/strong> (Emeritus)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">My research interests are Taylor-Couette flow, vortices and turbulence, superfluid hydrodynamics, superfluidity and Bose-Einstein condensation, quantum vortices and quantum turbulence<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile is-vertically-aligned-center\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\"><strong><a href=\"https:\/\/www.ncl.ac.uk\/maths-physics\/people\/profile\/paulbushby.html\">Prof Paul Bushby<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I have worked on a broad range of problems relating to astrophysical fluid dynamics and dynamo theory. My main area of astrophysics research centres around the origin and evolution of magnetic fields in the solar interior, but I have also worked on planetary atmospheres and the dynamics of the interstellar medium. More generally, I am also interested in assessing the capabilities and limitations of sound-proof approximations in fluid dynamics.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"753\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul-753x1024.jpeg\" alt=\"\" class=\"wp-image-7 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul-753x1024.jpeg 753w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul-221x300.jpeg 221w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul-768x1044.jpeg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul-1130x1536.jpeg 1130w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul-1506x2048.jpeg 1506w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Paul.jpeg 1813w\" sizes=\"auto, (max-width: 753px) 100vw, 753px\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile is-vertically-aligned-center\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"993\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Magda-Carr-2-993x1024.jpg\" alt=\"\" class=\"wp-image-8 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Magda-Carr-2-993x1024.jpg 993w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Magda-Carr-2-291x300.jpg 291w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Magda-Carr-2-768x792.jpg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Magda-Carr-2-1489x1536.jpg 1489w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Magda-Carr-2-1986x2048.jpg 1986w\" sizes=\"auto, (max-width: 993px) 100vw, 993px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\"><strong><a href=\"https:\/\/www.ncl.ac.uk\/maths-physics\/people\/profile\/magdacarr.html\">Dr Magda Carr<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I work on experimental and numerical modelling of internal solitary waves (ISWs) in the stratified ocean specifically in the context of Offshore Wind, Sea-Ice, and interaction with topography. My expertise includes laboratory generation and visualisation of ISWs (via PIV and micro-conductivity sensors) and numerical modelling via a spectral parallel incompressible Navier-Stokes solver.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile is-vertically-aligned-center\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\"><strong><a href=\"https:\/\/mncrowe.github.io\" data-type=\"link\" data-id=\"https:\/\/mncrowe.github.io\">Dr Matthew Crowe<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I work on the fluid dynamics of the ocean and atmosphere, using a combination of asymptotic methods and numerical simulations. In particular, I study submesoscale processes (scales of 100m-10km) such as ocean fronts, internal waves, baroclinic and symmetric instabilities, coastal-trapped waves, and dipolar vortices.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1816\" height=\"2296\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/12\/IMG_20241205_151524009.jpeg\" alt=\"\" class=\"wp-image-77 size-full\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"847\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2025\/11\/tiago_photo-847x1024.jpg\" alt=\"\" class=\"wp-image-115 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2025\/11\/tiago_photo-847x1024.jpg 847w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2025\/11\/tiago_photo-248x300.jpg 248w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2025\/11\/tiago_photo-768x929.jpg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2025\/11\/tiago_photo.jpg 1036w\" sizes=\"auto, (max-width: 847px) 100vw, 847px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"https:\/\/www.mas.ncl.ac.uk\/tiago.costa\/\">Dr Tiago Costa<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I research the physical processes governing galaxy evolution and, in particular, the growth of supermassive black holes, the \u200b impact of Active Galactic Nuclei (AGN), the hydrodynamics of galactic outflows and the origin of multi-phase structure. My research combines analytic modelling, radiation-hydrodynamic simulations and the analysis of multi-wavelength data.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"https:\/\/www.ncl.ac.uk\/maths-physics\/people\/profile\/celineguervilly.html\">Dr C\u00e9line Guervilly<\/a> <\/strong>(group leader)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I work on the fluid dynamics of planetary interiors and the generation of planetary magnetic fields using computational modelling. My current research involves rotating convection with applications to terrestrial liquid cores and gas giants: formation of large-scale vortices, magneto-convection, dynamo action, and double-diffusive effects. <\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"769\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-769x1024.jpeg\" alt=\"\" class=\"wp-image-34 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-769x1024.jpeg 769w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-225x300.jpeg 225w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-768x1023.jpeg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-1153x1536.jpeg 1153w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-1538x2048.jpeg 1538w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/IMG_20241007_153639-scaled.jpeg 1922w\" sizes=\"auto, (max-width: 769px) 100vw, 769px\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"333\" height=\"333\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/12\/Chris-Jones.png\" alt=\"\" class=\"wp-image-84 size-full\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Prof Chris Jones<\/strong> (visiting researcher)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">My research interests are: Magnetic field generation in the Earth and other planets; structure and dynamics of the Earth\u2019s outer core; thermal convection in rotating and magnetic systems; structure and dynamics of the giant planets and their magnetic fields; deep zonal flows in the giant planets; instability mechanisms and angular momentum transport in stars; &nbsp;the solar dynamo.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile\" style=\"grid-template-columns:auto 30%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"http:\/\/www.mas.ncl.ac.uk\/~ngrs\/home.html\">Dr Graeme Sarson<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am interested in a wide range of problems in geophysical and&nbsp;astrophysical fluids and magnetohydrodynamics.&nbsp; Much of my research has&nbsp;been on planetary dynamos, with some focus on field reversals;&nbsp; but I&nbsp;have also worked extensively on magnetic field generation and cosmic ray&nbsp;dynamics in the supernova-driven interstellar medium.&nbsp; I am currently&nbsp;involved in a project studying double-diffusive convection in planetary interiors.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"135\" height=\"180\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/grs_uni.jpg\" alt=\"\" class=\"wp-image-69 size-full\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile is-vertically-aligned-center\" style=\"grid-template-columns:35% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1298\" height=\"1617\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/12\/IAU_GA_Vienna_2018_cropped.jpeg\" alt=\"\" class=\"wp-image-81 size-full\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"https:\/\/www.ncl.ac.uk\/maths-physics\/people\/profile\/anvarshukurov.html\" data-type=\"link\" data-id=\"https:\/\/www.ncl.ac.uk\/maths-physics\/people\/profile\/anvarshukurov.html\">Prof Anvar Shukurov<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">My main research fields are:&nbsp;Interstellar medium, Astrophysical magnetohydrodynamics, Dynamo theory.&nbsp;<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">Other fields:&nbsp;Fluid dynamics, Turbulence, Mathematical modelling for stem cells research and prehistoric population dynamics, Medical image analysis, Air quality control in urban environments. <\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">Current research interests:&nbsp;Magnetic fields of galaxies, Dynamo theory, Interstellar matter, Interstellar turbulence; Cosmic rays; Neolithic dispersal in Eurasia, Stochastic dynamics of prehistoric settlement systems; Dynamics of human stem cells.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile is-vertically-aligned-center\" style=\"grid-template-columns:auto 35%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"https:\/\/www.ncl.ac.uk\/maths-physics\/people\/profile\/tobywood.html\">Dr Toby Wood<\/a><\/strong><\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am interested in the fluid dynamics of stellar interiors, including the Sun and neutron stars, where magnetic fields play a crucial role.&nbsp; My current research involves&nbsp;magneto-hydrodynamics and superfluidity.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"681\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-681x1024.jpg\" alt=\"\" class=\"wp-image-20 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-681x1024.jpg 681w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-200x300.jpg 200w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-768x1154.jpg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-1022x1536.jpg 1022w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-1363x2048.jpg 1363w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/Toby-Wood-2-scaled.jpg 1703w\" sizes=\"auto, (max-width: 681px) 100vw, 681px\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1873\" height=\"1941\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/12\/Niraj_Kr_Prasad.jpg\" alt=\"\" class=\"wp-image-87 size-full\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Dr Niraj Prasad <\/strong>(postdoc)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">My work primarily involves experimental and computational investigation of mode-2 internal solitary waves.&nbsp; I am currently working on the laboratory generation of mode-2 waves with multi-humped profiles.&nbsp; I have also performed experimental research in microfluidics and microfabrication and have expertise in photolithography and multiphase modelling of viscoelastic fluids.&nbsp;&nbsp;<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Dr Devika Tharakkal<\/strong> (postdoc)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am interested in astrophysical magnetic fields and related magnetohydrodynamical (MHD) problems. My current research focuses on MHD instabilities and dynamo processes in the solar tachocline. I also work on interstellar medium (ISM) dynamics, including the effects of magnetic fields and cosmic rays, as well as dust polarisation in star-forming clouds through radiative transfer simulations.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"640\" height=\"640\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/photo_6298345763657944915_x.jpg\" alt=\"\" class=\"wp-image-119 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/photo_6298345763657944915_x.jpg 640w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/photo_6298345763657944915_x-300x300.jpg 300w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/photo_6298345763657944915_x-150x150.jpg 150w\" sizes=\"auto, (max-width: 640px) 100vw, 640px\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"727\" height=\"769\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/photo.jpg\" alt=\"\" class=\"wp-image-59 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/photo.jpg 727w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/photo-284x300.jpg 284w\" sizes=\"auto, (max-width: 727px) 100vw, 727px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"https:\/\/www.mas.ncl.ac.uk\/Yue-Kin.Tsang\/\">Dr Yue-Kin Tsang<\/a> <\/strong>(postdoc)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am interested in the many complex phenomena arise in various geophysical and astrophysical fluid systems. This ranges from vortices and waves in Earth&#8217;s atmosphere and oceans to the dynamos inside the Earth and the giant planets of our solar system. A recent project is the investigation of double-diffusive convection under Saturn-like condition.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Martin Gray <\/strong>(PhD student)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am a PhD student and my current research is on double-diffusive convection in planetary interiors of Mercury-like planets working under C\u00e9line&nbsp;Guervilly and Graeme Sarson. Some of my other areas of interest are Astophysical Magnetohydronamics, Dynamo Theory and Turbulence.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"1080\" height=\"1748\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/12\/Screenshot_20240721_154311_Gallery.jpeg\" alt=\"\" class=\"wp-image-88 size-full\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"576\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057-576x1024.png\" alt=\"\" class=\"wp-image-22 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057-576x1024.png 576w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057-169x300.png 169w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057-768x1366.png 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057-863x1536.png 863w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057-1151x2048.png 1151w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/10\/20230916_133057.png 1452w\" sizes=\"auto, (max-width: 576px) 100vw, 576px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Rose Hinz <\/strong>(PhD student)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">My research focuses on computational fluid dynamics (CFD) using Dedalus,&nbsp;a spectral partial differential equation (PDE) solver widely used by&nbsp;researchers. Specifically, I model incompressible, rotating convection&nbsp;under low Prandtl number conditions. The primary goal of my research is&nbsp;to explain the formation, evolution, and structure of the large-scale&nbsp;vortices observed in Jupiter&#8217;s polar region. Additionally, I am working&nbsp;on integrating machine learning to support the computationally intensive&nbsp;CFD programs. My areas of interest include surrogate modeling,&nbsp;super-resolution, and autoencoding methods.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Scott Hopper <\/strong>(PhD student)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am a PhD student supervised by Toby Wood and Paul Bushby. My work revolves around the solar interior, specifically looking at magnetohydrodynamic instabilities which may arise in the solar tachocline. These include tearing instability, magnetorotational instability and magnetic buoyancy instability.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"481\" height=\"640\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Scott.jpg\" alt=\"\" class=\"wp-image-11 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Scott.jpg 481w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2024\/09\/Scott-225x300.jpg 225w\" sizes=\"auto, (max-width: 481px) 100vw, 481px\" \/><\/figure><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text is-stacked-on-mobile\" style=\"grid-template-columns:40% auto\"><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"937\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/IMG_6585-937x1024.jpg\" alt=\"\" class=\"wp-image-121 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/IMG_6585-937x1024.jpg 937w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/IMG_6585-274x300.jpg 274w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/IMG_6585-768x840.jpg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/IMG_6585-1405x1536.jpg 1405w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/IMG_6585-1873x2048.jpg 1873w\" sizes=\"auto, (max-width: 937px) 100vw, 937px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong>Jamie Jones <\/strong>(PhD student)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I\u2019m a PhD student supervised by Anvar Shukurov. My work revolves around simulating the turbulent interstellar medium (ISM) using the PENCIL code, a specialised partial differential equation (PDE) solver. My main areas of interest are galactic magnetohydrodynamics (MHD) and turbulent dynamo theory.<\/p>\n<\/div><\/div>\n\n\n\n<div style=\"height:20px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-media-text has-media-on-the-right is-stacked-on-mobile\" style=\"grid-template-columns:auto 40%\"><div class=\"wp-block-media-text__content\">\n<p class=\"has-medium-font-size\" style=\"font-style:normal;font-weight:400\"><strong><a href=\"https:\/\/rionnazareth.github.io\">Rion Nazareth<\/a> <\/strong>(PhD student)<\/p>\n\n\n\n<p style=\"font-style:normal;font-weight:400\">I am a PhD student working with Dr Tiago Costa. My research uses magnetohydrodynamical simulations with cosmic-ray transport physics to explore how powerful winds launched by supermassive black holes interact with the surrounding gas, affecting how galaxies grow, form stars, and produce signals that astronomers can observe.<\/p>\n<\/div><figure class=\"wp-block-media-text__media\"><img loading=\"lazy\" decoding=\"async\" width=\"682\" height=\"1024\" src=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot-682x1024.jpg\" alt=\"\" class=\"wp-image-122 size-full\" srcset=\"https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot-682x1024.jpg 682w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot-200x300.jpg 200w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot-768x1152.jpg 768w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot-1024x1536.jpg 1024w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot-1365x2048.jpg 1365w, https:\/\/blogs.ncl.ac.uk\/gafd\/files\/2026\/01\/rion_photoshoot.jpg 1706w\" sizes=\"auto, (max-width: 682px) 100vw, 682px\" \/><\/figure><\/div>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Prof Carlo Barenghi (Emeritus) My research interests are Taylor-Couette flow, vortices and turbulence, superfluid hydrodynamics, superfluidity and Bose-Einstein condensation, quantum vortices and quantum turbulence Prof Paul Bushby I have worked on a broad range of problems relating to astrophysical fluid &hellip; <a href=\"https:\/\/blogs.ncl.ac.uk\/gafd\/gafd-group\/\">Continue reading <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":6219,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-5","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/pages\/5","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/users\/6219"}],"replies":[{"embeddable":true,"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/comments?post=5"}],"version-history":[{"count":20,"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/pages\/5\/revisions"}],"predecessor-version":[{"id":125,"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/pages\/5\/revisions\/125"}],"wp:attachment":[{"href":"https:\/\/blogs.ncl.ac.uk\/gafd\/wp-json\/wp\/v2\/media?parent=5"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}