David Burgess is a Professor of Mathematics and Astronomy at Queen Mary University of London, affiliated with the School of Physical and Chemical Sciences and the Centre for Fundamental Physics. His research focuses on space and astrophysical plasma physics, particularly shocks in collisionless plasmas, turbulence, particle acceleration, and large-scale simulations. He collaborates internationally with ESA and NASA mission groups. Key Research Areas: Solar wind turbulence, bow shock dynamics, interplanetary shocks, and plasma simulations. Grants: £868k from STFC for heliospheric research (2023–2027), £626k for planetary studies (2020–2024). Collaborations: Involves groups in Europe and the USA, leveraging data from space missions like Solar Orbiter and MMS. His work uses particle-in-cell simulations and hybrid models to study plasma behavior, with recent emphasis on magnetic reconnection, electron heating, and shock-turbulence interactions.
Dr. Luke Barnard is an Associate Professor in the Department of Meteorology at the University of Reading, specializing in solar physics and space weather. His research focuses on solar wind dynamics, coronal mass ejections (CMEs), and their interactions with planetary environments. He contributes to models like HUXt for solar wind prediction and collaborates on space missions such as STEREO, Parker Solar Probe, and Tianwen-1. His work involves data assimilation techniques, ensemble modeling, and reconstruction of historical solar activity. Dr. Barnard's studies bridge observational data with theoretical models to advance understanding of heliospheric phenomena and their geophysical impacts. Key Affiliations: Department of Meteorology, University of Reading. Research Themes: Solar wind modeling, CME propagation, space weather forecasting, geomagnetic effects, and long-term solar variability. Collaborations: Extensive international collaborations, including with NASA, ESA, and institutions such as BepiColombo and MAVEN missions. His recent work emphasizes probabilistic solar wind forecasting, CME interaction with comets and planets, and historical reconstructions of solar activity. He has published over 79 peer-reviewed articles, with a focus on solar-heliospheric dynamics and space weather mitigation strategies.
Professor Christopher Scott is a Professor in Space & Atmospheric Physics at the University of Reading's Department of Meteorology, serving as Laboratory Manager. His research focuses on space weather, solar-terrestrial interactions, auroral physics, ionospheric dynamics, and long-term atmospheric changes. He leads projects like the Dr Carbon Atmospheric Observatory and the citizen science initiative Solar Stormwatch (www.solarstormwatch.com). His work integrates observations from spacecraft (e.g., STEREO, BepiColombo) and ground-based systems to study solar wind impacts, CME propagation, and ionospheric responses. Key contributions include advancing CME forecasting models, analyzing comet-solar wind interactions, and quantifying long-term ionospheric changes. He supervises postdoctoral researchers Luke Barnard and Kim Tucker-Hood, and collaborates on global initiatives like the Solar Stormwatch project. His research spans disciplines including geophysics, astrophysics, and planetary science, with over 100 peer-reviewed publications since 1994.
Dr. Christopher Chen is a Reader in Space Plasma Physics at Queen Mary University of London, holding a UKRI Future Leaders Fellowship. He is affiliated with the School of Physical and Chemical Sciences within the Department of Physics and Astronomy. Chen earned his PhD in Space Physics from Imperial College London in 2011 and has held research positions at the University of California, Berkeley and Imperial College before joining QMUL in 2017, where he progressed from Lecturer to Senior Lecturer in 2021 and then to Reader in 2022. Chen's research focuses on space plasma physics, particularly solar wind turbulence and its fundamental properties. His work bridges theoretical models, spacecraft data analysis, and laboratory experiments to understand complex plasma behavior. He is actively involved in several major space missions including Parker Solar Probe (as a member of FIELDS and SWEAP teams), Interstellar Probe mission study, and Magnetospheric Multiscale mission (as a member of the Science Working Team). His publication record shows a strong focus on solar wind turbulence, Alfvén wave interactions, and plasma dynamics in the inner heliosphere. The most recent work emphasizes forecasting techniques for solar wind parameters, laboratory experiments of wave interactions, and detailed analysis of turbulence properties using data from Parker Solar Probe. His research demonstrates a clear progression toward understanding the kinetic-scale processes that govern energy transfer in space plasmas. Royal Astronomical Society Fowler Award (2017) American Geophysical Union Macelwane Medal (2021) Conferred Fellow of the American Geophysical Union (2021) American Physical Society Landau-Spitzer Award (2022) Chen actively supervises a large research group including multiple postdoctoral researchers and PhD students, and has secured significant research funding through an STFC Ernest Rutherford Fellowship (2016-21), UKRI Future Leaders Fellowship (2022-26), and multiple STFC Consolidated Grants. His teaching responsibilities include organizing and lecturing the Astrophysical Plasmas module and supervising Masters and undergraduate research projects. He is also engaged in extensive public outreach through media interviews, public talks, and participation in science festivals.
Dr. Heli Hietala is a Lecturer in Space Plasma Physics and Royal Society University Research Fellow at Queen Mary University of London, affiliated with the School of Physical and Chemical Sciences. She is an active researcher in the Centre for Fundamental Physics and Centre for Experimental and Applied Physics, focusing on space plasma phenomena and contributing significantly to our understanding of space weather dynamics. Dr. Hietala's research primarily centers on space plasma physics with specific expertise in: Magnetosheath jets and their formation mechanisms Collisionless shock physics throughout the solar system Interplanetary shocks and solar wind-magnetosphere interactions Space plasma turbulence and particle acceleration Observational space physics using multi-spacecraft missions Analysis of Dr. Hietala's recent publications (2022-2025) reveals a strong focus on magnetosheath jets, collisionless shocks, and interplanetary phenomena. Her work combines observational data from missions like Solar Orbiter, Parker Solar Probe, and MMS with theoretical modeling to understand fundamental plasma processes. A notable trend is the increasing emphasis on multi-spacecraft observations to study three-dimensional structures in space plasmas, and the development of empirical models connecting solar wind parameters to magnetospheric phenomena. Dr. Hietala has received significant recognition through: Royal Society University Research Fellowship Enhanced Research Expenses grant (2023) Enhancement award (2018) Dr. Hietala currently supervises PhD student Rose Atkinson, who is researching "Quasi-Parallel Shocks Across The Solar System." Her research is supported by multiple grants from the Royal Society totaling over £700,000, demonstrating strong institutional support for her innovative work in space plasma physics. As a member of the Centre for Fundamental Physics, Dr. Hietala collaborates with an interdisciplinary team of researchers studying fundamental physical processes. Her work connects observational space physics with theoretical plasma physics, contributing to both basic scientific understanding and practical space weather applications.
Dr. Charles Wang is a Reader in the Department of Physics at the University of Aberdeen, within the School of Natural and Computing Sciences. He has held this position since 2005 and is also an Honorary Cruickshank Lecturer in Astronomy at the same institution. His academic journey began with a BSc in Physics from National Taiwan University, followed by a Certificate of Advanced Study in Mathematics from Cambridge, and culminated in a PhD in Mathematical Physics from Lancaster University. Education: BSc (National Taiwan University), CASM (Cambridge), PhD (Lancaster) Current Position: Reader, Department of Physics, University of Aberdeen Additional Role: Honorary Cruickshank Lecturer in Astronomy Dr. Wang's research lies at the intersection of theoretical physics and experimental gravity, focusing on general relativity, quantum gravity, modified gravity, astrophysics, and cosmology. He is a pioneer in quantum gravity phenomenology, particularly through atom interferometry techniques. His work extends into applied mathematics, including differential geometry, Clifford algebra, and the Cosserat theory of rods. He actively collaborates with industry and research institutions on quantum sensing, gravity gradiometry, and precision measurement applications. His recent publications reveal a strong trajectory in quantum aspects of gravity, including Unruh radiation, gravitational decoherence, quantum sensing of spacetime fluctuations, and loop quantum gravity formulations. These works are published in high-impact journals such as Physical Review D, Classical and Quantum Gravity, and the European Physical Journal C. Scientific honors include being a Fellow of the STFC Centre for Fundamental Physics. He has secured significant research funding from sources like MoD/Dstl, EPSRC, UKSA, and BP for projects related to quantum gravity experiments and gravity sensing technologies. STFC Centre for Fundamental Physics Fellow Dr. Wang has supervised PhD students and contributed to major international collaborations such as STE-QUEST (ESA mission candidate), GG-TOP (with Birmingham), and CERN-related supernova research. He has also served in professional roles including Grampian Regional Organiser for the Institute of Physics in Scotland and as a Series Editor for Springer Briefs in Physics. He is affiliated with research groups including the Plasma Science Research Group (PSRG) and contributes to interdisciplinary initiatives such as the Advanced Centre for Energy and Sustainability (ACES).
Dr. Clare E. J. Watt is a prominent researcher in space physics at the University of Reading, with a distinguished publication record spanning over 15 years. Her work primarily focuses on magnetospheric physics, radiation belt dynamics, and space weather phenomena, contributing significantly to our understanding of Earth's space environment. Dr. Watt's research interests center on wave-particle interactions in Earth's magnetosphere, particularly examining ultra-low frequency (ULF) waves, plasmaspheric hiss, and their effects on radiation belt electrons. Her work bridges theoretical modeling with observational data, investigating how these waves influence electron acceleration and loss processes during geomagnetic storms. She has made significant contributions to understanding the temporal and spatial variability of wave-particle interactions, developing probabilistic mapping tools, and creating advanced models for radiation belt dynamics. Analysis of her recent publications reveals a strong emphasis on data-driven approaches to space physics, including machine learning applications for solar wind classification and ULF wave modeling. Her research demonstrates a consistent focus on quantifying uncertainties in space weather models and understanding the complex interplay between different wave modes in the magnetosphere. Dr. Watt frequently collaborates with leading space physics researchers across multiple institutions, contributing to major studies on space climate and radiation belt dynamics. Dr. Watt has co-authored numerous high-impact publications in leading journals including Journal of Geophysical Research: Space Physics, Geophysical Research Letters, and Space Weather. Her work has been instrumental in advancing our understanding of radiation belt dynamics and space weather prediction capabilities. She has also contributed to book chapters on ULF waves and Alfvén wave acceleration of auroral electrons, demonstrating her expertise in both observational and theoretical aspects of space physics.
Professor Michael Lockwood is a distinguished Professor of Space Environment Physics at the Department of Meteorology, University of Reading. With an extensive publication record spanning decades, he is a leading figure in space physics research, particularly in solar-terrestrial interactions and space weather phenomena. Lockwood's research focuses on understanding the complex interactions between solar activity and Earth's space environment. His work spans solar physics, magnetospheric dynamics, ionospheric phenomena, and space climate studies. He investigates how solar wind variations impact Earth's magnetosphere, causing geomagnetic storms and auroral activity. His research has significant implications for space weather forecasting and understanding long-term solar variability. His recent publications demonstrate a continued focus on solar-terrestrial physics, with particular attention to solar wind-magnetosphere coupling, polar cap dynamics, and historical space weather reconstruction. Lockwood's work often involves multi-instrument and multi-mission analysis, leveraging data from missions like Solar Orbiter, MAVEN, and various ground-based observatories. Lockwood has made significant contributions to understanding space weather events, including the recent May 2024 event, space hurricanes, and polar cap phenomena. His research bridges fundamental space physics with practical space weather applications, contributing to improved forecasting models and a deeper understanding of solar-terrestrial relationships. His extensive collaborative network is evident in his numerous co-authored publications with researchers across the globe, reflecting the international nature of space physics research. He has contributed to major projects involving solar wind modeling, historical space climate reconstruction, and the analysis of extreme space weather events.
Professor Eduard Kontar is a Professor of Astrophysics at the University of Glasgow's School of Physics & Astronomy. His research focuses on solar flare physics, plasma kinetic theory, and radio/X-ray emission mechanisms. He leads projects using data from missions like RHESSI, Solar Orbiter, and the Square Kilometer Array (SKA). He has organized international workshops, including the STFC Summer School on Solar System Plasmas and the Franco-British Alliance collaboration. His software contributions include tools for X-ray spectroscopy analysis and inversion methods. Key affiliations: SUPA School of Physics & Astronomy, European Solar Physics Division, RHESSI mission collaborations Research projects: SKA solar physics, EU-funded HESPE project, ISSI teams on flare diagnostics Teaching: Courses on stellar physics, observational astrophysics, plasma theory, and high-energy astrophysics Research interests span particle acceleration in flares, coronal plasma dynamics, and radio/X-ray observational techniques. His work bridges theory, simulation, and multi-wavelength data analysis to understand energy release processes in solar flares. Advising and grants: Principal Investigator on Franco-British Alliance projects, STFC grants, and EU Horizon 2020 initiatives. Collaborations include LOFAR, Solar Orbiter/RPW instrument teams, and Parker Solar Probe analyses. Labs/teams: Involved with Glasgow's solar physics group, CESRA (European Solar Radio community), and international ISSI teams in Bern.
Claire Foullon is a Senior Lecturer in Heliophysics at the University of Exeter's Centre for Geophysical and Astrophysical Fluid Dynamics. An STFC Advanced Fellow, she researches wave phenomena in solar-terrestrial plasmas using multi-spacecraft data. Her work addresses solar wind dynamics, magnetic reconnection, and space weather prediction. She mentors PhD candidates in solar/heliospheric physics and developed curriculum for STFC Summer Schools. Awards: STFC Advanced Fellowship (2011) Foullon contributes to ESA's Solar Orbiter mission development and leads international collaborations in space plasma diagnostics.
Shaun Bloomfield is an Associate Professor at Northumbria University's Mathematics, Physics and Electrical Engineering Department. His research focuses on solar physics, particularly solar flare forecasting, space weather prediction, and the application of machine learning in heliophysics. He holds a PhD and MSc in Astrophysics from Queen's University Belfast (2005 and 2001, respectively). Education: PhD in Astrophysics, Queen's University Belfast (2001-2005) MSc in Astrophysics, Queen's University Belfast (1998-2001) Research Interests: Space weather and solar flare forecasting Machine learning applications in solar physics Coronal mass ejections and solar eruptions EUV imaging and instrumentation Magnetic field dynamics in active regions Recent Articles: Bloomfield's work emphasizes forecasting solar energetic events, validating EUV wave simulations, and developing ensemble forecasting techniques. His contributions include advancements in flare prediction algorithms and EUV filter design for the SWAP telescope. Professional Activities: Member of the International Astronomical Union (IAU) since 2021 Editor of the Journal of Space Weather and Space Climate since 2017 Past member of the European Solar Physics Division (2014-2021) Labs/Teams: Collaborates on projects like the FLARECAST initiative, focusing on big data and machine learning for flare forecasting.
Sargam Mulay is a Researcher at the University of Glasgow's School of Physics and Astronomy since July 2021, previously serving as a Research Assistant (2019-2021). She holds a Ph.D. in Solar Physics from the University of Cambridge (2018), focusing on solar active region jets. Her work has included postdoctoral research at IUCAA, Pune (2018-2019), studying sigmoid observations with Prof. Durgesh Tripathi. Her research emphasizes observational spectroscopy, solar flares, coronal heating, and molecular hydrogen emission analysis using IRIS satellite data. Key collaborations include studies with Prof. Lyndsay Fletcher at Glasgow and Prof. Helen Mason at Cambridge. Education: Ph.D. in Solar Physics (University of Cambridge, 2018), prior research at IUCAA and collaborative work across institutions like NASA Goddard Space Flight Center and Inter-University Centre for Astronomy and Astrophysics. Research Interests: X-ray/UV spectroscopy of solar phenomena, reconnection processes in flares, molecular hydrogen emission diagnostics, and multiwavelength analysis of active region jets. Her work bridges observational data from SDO, Hinode, IRIS, and RHESSI with theoretical models. Publications highlight contributions to solar energetic particle studies, flare dynamics, and coronal flow mechanisms. Her recent focus on molecular hydrogen emission in flares has advanced understanding of chromospheric processes. Collaborative projects include studies of nonthermal radio bursts and spatial correlations with solar jets.
Julia Stawarz is an Associate Professor at Northumbria University's Department of Mathematics, Physics, and Electrical Engineering, specializing in space plasma physics. She holds a Royal Society University Research Fellowship and serves as an Associate Editor for Physics of Plasmas . Her research focuses on plasma turbulence, magnetic reconnection, and collisionless phenomena using spacecraft data from missions like MMS, Parker Solar Probe, and Solar Orbiter. Education: BSc in Physics (University of New Hampshire, 2011), MSc and PhD in Astrophysics (University of Colorado Boulder, 2013 and 2016). Postdoctoral work at Imperial College London before joining Northumbria in 2022. Research Interests: Solar wind dynamics, magnetospheric interactions, turbulence-driven reconnection, and developing the ESA Plasma Observatory mission. Key areas include electron kinetic physics, machine learning applications in plasma analysis, and cross-scale plasma modeling. Notable Awards: Winton Award (2021), Ronald C. Davidson Award (2024), and numerous fellowships including the NSF Graduate Research Fellowship. Current Projects: Leading the Electron Kinetic Physics book project, advising on ESA's Plasma Observatory mission, and mentoring PhD students in reconnection and turbulence studies.
Dr. Xing Li is a Senior Lecturer in the Department of Physics at Aberystwyth University. He holds a BSc and MSc from the University of Science and Technology of China, and a PhD from Hefei. His research focuses on coronal heating, solar wind acceleration, and space plasma physics. He has contributed significantly to understanding ion dynamics in the solar wind and developed models like the 16-moment solar wind model. His work explores plasma instabilities, ion cyclotron resonance, and multi-fluid MHD modeling. Affiliation: Aberystwyth University, Department of Physics Appointed as Lecturer in March 2001 Postdoctoral research at Harvard-Smithsonian Center for Astrophysics Research Interests: Coronal heating mechanisms, solar wind dynamics, plasma waves and instabilities, and solar wind turbulence at small scales. Current projects include studying space plasma turbulence and ion kinetic processes. Recent articles highlight studies on solar wind turbulence, magnetic reconnection, and Alfvén waves. His work bridges observational data with theoretical models, advancing understanding of solar phenomena. Grants and Projects: Co-Investigator in the 'Solar System Physics at Aberystwyth University' project (2019–2022), PI of 'Arc-polarised Alfvén Wave in Solar Wind' (2010).
Professor Michael Balikhin is a distinguished academic in the Space Systems Laboratory at the University of Sheffield's School of Electrical and Electronic Engineering . With over 30 years of research experience, his work focuses on space plasma physics , collisionless shocks , plasma turbulence , and radiation belt dynamics . He serves as Principal Investigator for the Digital Wave Processor instruments on ESA's Cluster satellites and as editor of Journal of Geophysical Research: Space Physics . PhD in Physics (1989) Joined Sheffield in 1995 Key contributor to Cluster mission Leading expert in nonlinear space plasma systems Research Areas His research spans space weather , solar-terrestrial relations , and spacecraft instrumentation , with particular emphasis on electron heating mechanisms , shock structures , and nonlinear system identification . The 15 most recent articles demonstrate his expertise in gamma-ray burst analysis , magnetospheric wave dynamics , and multi-point space plasma observations . Scientific Recognition Leverhulme Grant (2024-2027) STFC/NERC grants exceeding £1.5M EPSRC Platform Grant (2010-2015) Over 20 years of ESA Cluster mission involvement Key Collaborations Extensive collaborations with ESA , STFC , AGU , and international space agencies. Currently working with University of Michigan , Space Research Institute (Austria) , and Skobeltsyn Institute (Russia) .
