James F. Drake is a Distinguished University Professor in the Department of Physics at the University of Maryland, College Park, with affiliations at the Institute for Physical Science and Technology (IPST) and the Institute for Research in Electronics and Applied Physics (IREAP). He holds a B.S., M.S., and Ph.D. in Physics from UCLA (1975). His research focuses on theoretical plasma physics, particularly magnetic reconnection and plasma turbulence, with applications to space physics, solar flares, and magnetic fusion. Key contributions include elucidating the role of whistler waves in reconnection dynamics and advancing understanding of energy release mechanisms in plasmas. Dr. Drake’s awards include the American Physical Society Fellowship and the Humboldt Senior Scientist Research Award. He teaches advanced physics courses (e.g., Physics 604, 611, 761-762) and has pioneered computational models to study reconnection, turbulence, and particle acceleration. Recent work leverages Parker Solar Probe data to explore solar wind dynamics and reconnection in near-Sun environments. Education: UCLA (B.S., M.S., Ph.D. in Physics, 1975) Research Themes: Magnetic Reconnection, Plasma Turbulence, Space Plasma Dynamics Notable Achievements: Leader in reconnection theory; developer of kinetic simulation frameworks; contributor to NASA missions
Dr David Pratt is a Fellow in History at Downing College, University of Cambridge , where he also serves as Archivist and Keeper of Art and Artefacts. His academic career focuses on early medieval political thought and court culture, particularly in Anglo-Saxon England and the Carolingian world. Academic Rank: Research Fellow Honors: FRHistS (Fellow of the Royal Historical Society) Research Interests center on the political ideology of King Alfred the Great, the origins of English coronation rituals, and broader themes of kingship, law, and social order in the later Anglo-Saxon period. His comparative approach highlights interactions between Anglo-Saxon and European medieval traditions. Recent Publications include English Coronation Ordines in the Ninth and Early Tenth Centuries (2023) and studies on Alfredian texts, taxation systems, and monastic reform. These works emphasize textual analysis, royal authority, and cross-cultural influences. Scientific Awards: FRHistS
Matthew W. Kunz is an Associate Professor of Astrophysical Sciences at Princeton University, serving as Associate Chair of the Department of Astrophysical Sciences and Director of Graduate Studies for the Program in Plasma Physics. He holds a B.S. in Astronomy-Physics and B.A. in Music from the University of Virginia (2003), and a Ph.D. in Physics from the University of Illinois at Urbana-Champaign (2009). His research focuses on astrophysical plasma dynamics, including instability, turbulence, and transport in weakly collisional and poorly ionized plasmas, with applications to galaxy clusters, accretion disks, and the solar wind. Dr. Kunz's work employs analytical and numerical methods to study multi-scale plasma dynamics, aiming to understand angular momentum transport in accretion disks, kinetic turbulence cascades, and magnetic field evolution. His research has been recognized with several awards, including an NSF CAREER Award (2020-25), Alfred P. Sloan Research Fellowship (2017-20), and NASA Einstein Postdoctoral Fellowship (2011-14). He teaches courses on plasma astrophysics (AST 521), irreversible processes in plasmas (AST 554), and astrophysical research methods (AST 303). His publications demonstrate a consistent focus on plasma turbulence, magnetic reconnection, and cosmic ray propagation, with recent work emphasizing collisionless plasma dynamics and high-energy astrophysical phenomena.
Prof Ineke De Moortel is a Professor in Applied Mathematics at the University of St Andrews, affiliated with the School of Mathematics and Statistics. Her research focuses on magnetohydrodynamic (MHD) waves in the solar corona, coronal seismology, and numerical modeling of solar phenomena. She has led projects funded by organizations like the Leverhulme Trust and STFC, contributing to understanding coronal heating mechanisms and wave dynamics. Prof De Moortel has supervised PhD students including Elisabeth Enerhaug and Anmol Kumar. She holds editorial roles, including at the Monthly Notices of the Royal Astronomical Society, and has received prestigious awards such as the Phillip Leverhulme Prize (2009) and the RAS Fowler Award (2010). Research Highlights: MHD wave propagation, coronal seismology, numerical simulations of solar plasma dynamics. Projects: Includes 'Joining up an Unprecedented View of our Sun' (Leverhulme Trust) and collaborations on the Multi-slit Solar Explorer (MUSE) mission. Awards: Royal Society of Edinburgh Young Academy Co-Chair (2012), Deputy Chair of UK Solar Physics Council (2013).
Moira Jardine is Professor of Astronomy at the University of St Andrews School of Physics and Astronomy, where she became the first female physics professor in 2010. Education: Ph.D. Applied Mathematics, University of St Andrews B.Sc. Astronomy and Astrophysics, University of St Andrews Research investigates stellar magnetic activity to understand planetary habitability and solar system evolution. Uses magnetic field measurements to model stellar winds, coronal X-ray emissions, and their impact on planetary atmospheres. Work supports exoplanet detection initiatives including JWST, GAIA, and WFIRST. Publications focus on stellar coronae, magnetic confinement processes, star-planet interactions, and coronal rain dynamics. Current projects model magnetic interactions in systems like AB Dor and HD 189733. Collaborates with international consortia including MagIcS and Bcool for stellar magnetic field surveys. Awards: Fellow of the Royal Society of Edinburgh and Suffrage Science Award (2019).
Scott England is a Professor in the Department of Aerospace and Ocean Engineering at the College of Engineering, Virginia Polytechnic Institute and State University. He serves as the Project Scientist for NASA’s Ionospheric Connection Explorer (ICON), Co-Investigator for Global-scale Observations of the Limb and Disk (GOLD), and Participating Scientist for Mars Atmosphere and Volatile Evolution (MAVEN). Education PhD, University of Leicester (UK), 2005 MPhys First Class Honors, University of Leicester (UK), 2001 England’s research focuses on planetary atmosphere-space environment interactions, particularly gravity waves, atmospheric tides, and ionosphere-thermosphere coupling on Earth and Mars. His work integrates NASA mission data (ICON, GOLD, MAVEN) with numerical modeling to study thermal dynamics, wind systems, and solar flare impacts. Recent publications highlight his expertise in thermospheric gravity wave science, planetary wave-induced ionospheric variability, and Mars atmosphere studies using EMUS and IUVS instruments. Articles span topics like Seasonal variability of DE3/DE2 tides , Transient Martian hot oxygen corona , and Shock-induced plasma dynamics . Scientific Honors 2020 Dean's Award for Teaching Excellence 2016 RHG Exceptional Achievement for Mars Science As a professional leader, England served as Thermospheric Lead for the 2019 Planetary Mission Concept Studies Program and on the National Academy of Sciences Decadal Survey panel. He manages Virginia Tech’s participation in the Virginia Space Grant Consortium and has contributed to high-performance computing committees.
Dr. Nicholas Nelson is an Associate Professor in the Department of Physics at California State University, Chico. His research spans interdisciplinary areas including astrophysics, dynamical chaos, and medical education curriculum development. He specializes in stellar evolution models, solar convection dynamics, and magnetic field generation in stars. His work bridges physics and healthcare, addressing structural competency in medical training and social determinants of health through innovative curricula. Research interests include: solar magnetic loop formation, chaotic dynamics in celestial bodies, and integrating social determinants of health into residency programs. His publications reflect a dual focus on computational astrophysics and healthcare equity. Notable contributions include studies on knuckleball aerodynamics, early career challenges in astrophysics, and curriculum design for addressing health disparities. Though no awards are explicitly listed, his work demonstrates impactful cross-disciplinary engagement. No advising relationships or grant information was provided in the source material. His office is located in PHSC 121B on campus.
Colby Haggerty is an Assistant Professor at the Institute for Astronomy (IfA Mānoa) at the University of Hawaiʻi at Mānoa. He specializes in computational plasma physics, focusing on magnetospheric, heliospheric, and astrophysical systems. His research emphasizes collisionless plasma shocks, magnetic reconnection, and kinetic plasma turbulence. He holds a Ph.D. in Plasma Physics from the University of Delaware (2017) and conducted postdoctoral work at the University of Chicago (2017–2021). His work bridges theory, numerical simulations, and observational data analysis using advanced computational tools like Python, C++, Fortran, and MPI/OpenMP frameworks. Research Interests: He investigates collisionless plasma shocks and energetic particle acceleration (e.g., Earth’s bow shock, coronal mass ejections), plasma instabilities, magnetic reconnection dynamics, and the role of turbulence in energy dissipation. His studies often involve hybrid and particle-in-cell (PIC) simulations to model cosmic phenomena like supernova remnants and solar wind interactions. Articles & Trends: His recent publications highlight advancements in understanding shock-drift acceleration mechanisms, the saturation of plasma instabilities (e.g., Bell instability), and scaling laws for magnetic reconnection in asymmetric and relativistic regimes. Collaborations with institutions like NASA Goddard, Columbia University, and the University of Chicago underscore his interdisciplinary approach. He has also contributed to developing Python-based plasma physics tools (e.g., PlasmaPy) for the scientific community. Grants & Impact: His CAREER award (2024) supports studies on collisionless magnetic reconnection as a heliospheric process. He emphasizes computational methods and educational outreach, reflecting his dual focus on advancing science and training future researchers. Labs & Teams: While no specific lab is named, his work relies on collaborative networks with leading institutions, leveraging state-of-the-art simulation infrastructure to tackle complex plasma problems.
Wayne Springer is a Professor in the Department of Physics & Astronomy at the University of Utah, with a career spanning over 25 years. He has been actively involved in experimental particle astrophysics, ultra-high-energy cosmic ray (UHECR) physics, and gamma-ray astronomy. Ph.D. in Physics from University of Maryland (1991) B.S. in Physics from University of Maryland (1985) Postdoctoral training at University of Maryland and University of Alberta His research focuses on particle astrophysics, cosmic ray detection, and gamma-ray astronomy. He has made significant contributions to the development of the HiRes and Telescope Array cosmic ray observatories, as well as the HAWC and SWGO gamma-ray observatories. His recent work includes deployment of the Trinity neutrino detector prototype and serving as SWGO project manager for Chile site infrastructure. Article trends show strong emphasis on TeV gamma-ray observations (HAWC, SWGO), cosmic ray diffusion mechanisms, dark matter searches, and high-energy astrophysical source characterization (pulsars, microquasars, supernova remnants). He has secured multiple NSF grants for particle astrophysics research and leads detector working groups in international collaborations. Professor Springer actively participates in astronomy outreach, co-developing observatories and implementing computational physics teaching tools with Gradescope auto-graders for enhanced pedagogy. His work bridges experimental high-energy physics, detector development, and multiwavelength astrophysical studies.
Justin C. Kasper is an Affiliated Professor in the Department of Climate and Space Sciences and Engineering at the University of Michigan. He serves as Graduate Advisor for the Ph.D. program in Space & Planetary Physics and leads multiple high-profile space exploration initiatives. Education 2003: PhD in Physics from Massachusetts Institute of Technology 1999: AB in Physics from University of Chicago Research Focus Dr. Kasper's work centers on solar physics and space weather , investigating heating mechanisms, plasma instabilities, and helium dynamics in the solar corona and solar wind. His research examines space weather impacts on society and develops early warning systems using deep space monitors. He also studies Jupiter's moon Europa and its interaction with Jupiter's magnetosphere. As an instrument designer, Kasper creates sensors for spacecraft operating in extreme environments from the Sun's surface to the solar system's edge. His research provides critical insights into solar flares and the million-degree solar wind. Scientific Contributions Analysis of Dr. Kasper's publications reveals consistent focus on solar wind composition, heating mechanisms, and plasma diagnostics. His work tracks helium abundance variations through solar cycles, examines ion-cyclotron resonant heating, and investigates temperature anisotropy constraints in solar wind protons. Awards and Honors 2011: Popular Science Brilliant 10 2010: Presidential Early Career Award for Scientists and Engineers 2010: Smithsonian Innovative Spirit Award Multiple NASA Group Achievement Awards for LRO and Triana projects 2004: MIT Dean's Educational and Student Advising Award Research Leadership Dr. Kasper serves as Principal Investigator for the SWEAP Investigation on NASA's Solar Probe Plus mission, Instrument Lead for the Faraday Cup on the Deep Space Climate Observatory, and Co-Investigator for FIELDS. He leads international teams developing sensors that will make the first direct measurements of the solar corona.
Chuanfei Dong is an Assistant Professor of Astronomy at Boston University's College of Arts & Sciences and of Electrical and Computer Engineering at the College of Engineering. His research focuses on understanding plasma physics and its applications to space science, planetary atmospheres, and fusion energy. Dong joined BU in January 2023 after working as a staff scientist at the Princeton Plasma Physics Laboratory. Education: B.S. in Space Science from University of Science and Technology of China M.S. in Earth and Atmospheric Sciences from Georgia Institute of Technology M.S.E. in Nuclear Engineering and Radiological Sciences from University of Michigan M.S. in Planetary and Space Sciences from University of Michigan Ph.D. in Scientific Computing from University of Michigan Research Interests: Dr. Dong's research spans multiple disciplines within space physics and plasma science. His primary interests include Star-Terrestrial Planet Interactions in our Solar System and beyond, magnetic reconnection and turbulence phenomena, wave-particle interactions in space plasmas, and applications of physics-informed machine learning to plasma problems. He also investigates high-intensity laser-plasma interactions with applications to fusion energy research. His work bridges the gap between theoretical plasma physics and observational space science, with particular focus on planetary atmospheres, solar wind interactions, and exoplanet habitability. Dong's interdisciplinary approach combines computational modeling, observational data analysis, and theoretical frameworks to address fundamental questions in space physics. Research Trends: Dong's recent publications demonstrate a strong focus on applying advanced computational techniques to space plasma physics problems. His work spans solar system bodies including Earth, Mars, Mercury, and the Moon, with increasing attention to exoplanet systems. A notable trend is the integration of machine learning approaches with traditional plasma physics modeling, particularly for complex phenomena like Landau damping and magnetic reconnection. His research has significant implications for understanding atmospheric evolution, space weather, and potential habitability of planetary bodies. Scientific Awards: DOE Early Career Research Award (2023) - $875,000 grant for plasma turbulence research Alfred P. Sloan Research Fellow (2024) Metcalf Travel Award Advising and Grants: Dr. Dong mentors undergraduate research assistants and plans to expand his research group with the support of his DOE Early Career Award, which will fund a graduate student and postdoctoral researcher. His research is supported by the Department of Energy and has connections to NASA missions including MAVEN (Mars) and BepiColombo (Mercury). Dong is also involved with the Mauve telescope project as BU institutional PI. His work has been featured in numerous media outlets including Phys.org, Science Daily, and German TV program zdf/3sat. Labs and Teams: Dr. Dong leads a research group focused on computational plasma physics at Boston University. He collaborates with researchers at Princeton Plasma Physics Laboratory and is involved with multiple NASA missions. His team develops advanced computational models to simulate space plasma phenomena, with particular expertise in magnetohydrodynamics (MHD), particle-in-cell methods, and physics-informed machine learning approaches. Dong is also affiliated with BU's Hariri Institute for Computing.
Susan T. Lepri is a Professor in the Department of Climate and Space Sciences and Engineering at the University of Michigan's College of Engineering, where she serves as Director of the Space Physics Research Laboratory. Her work focuses on heliospheric physics, utilizing spacecraft data from missions like ACE, WIND, and Solar Orbiter to investigate solar wind origins and coronal mass ejections. Her educational background includes: Ph.D. in Atmospheric and Space Sciences, University of Michigan M.S. in Atmospheric and Space Sciences, University of Michigan B.S. in Physics, Astronomy and Astrophysics, University of Michigan Lepri's research centers on tracing charged particles in the heliosphere using heavy ion measurements to study solar wind sources, coronal mass ejection physics, and particle acceleration mechanisms. She develops space-based ion mass spectrometers for missions including the European Space Agency's Solar Orbiter (Heavy Ion Sensor) and the Interstellar Mapping and Acceleration Probe. Her work integrates statistical analysis of solar wind composition with magnetohydrodynamic model validation to unravel plasma behavior in space environments. Analysis of her 15 most recent publications (2015-2017) reveals consistent focus on solar wind composition dynamics, particularly charge state evolution and elemental fractionation. Key themes include magnetic reconnection signatures in slow solar wind formation, anomalous composition in depleted interplanetary coronal mass ejections, and solar wind charge exchange contributions to X-ray backgrounds. Her instrumentation work bridges observational gaps in inner heliospheric measurements. Major recognitions include: 2018 Claudia Joan Alexander Trailblazer Award (University of Michigan) 2012-2013 Kenneth M. Reese Outstanding Research Scientist Award 2008 JGR-Space Physics Excellence in Refereeing Citation NASA Graduate Fellowship (2001-2003) Lepri actively mentors through outreach programs including K-12 initiatives with the Michigan Space Grant Consortium and Detroit Area Pre-College Engineering Program. She has coordinated Rochester Adams High School STEAM fairs and elementary science outreach while developing educational content like MConnex videos. Her research is supported by NASA grants enabling instrument development for Solar Orbiter and IMAP missions, with collaborations spanning international space agencies and academic institutions. As Director of the Space Physics Research Laboratory, she leads teams developing next-generation space instrumentation, particularly ion mass spectrometers for heliospheric exploration. Current projects include the Heavy Ion Sensor for Solar Orbiter (measuring inner heliospheric composition) and innovative sensors for IMAP, advancing capabilities to trace solar wind sources and particle acceleration mechanisms.
Professor Jack D. Scudder is a distinguished Professor of Physics and Astronomy at the University of Iowa, where he has been faculty since 1993. His research focuses on space magneto-plasmas and their kinetic properties, particularly in the solar corona, solar wind, collisionless shocks, magnetosheath, magnetopause, and collisionless reconnection phenomena. Scudder received his B.A. in Physics and Mathematics from Williams College in 1969, followed by an M.S. in Plasma Physics from the University of Maryland in 1971, and a Ph.D. in Plasma Physics from the same institution in 1975. His doctoral thesis was titled "Fission Driven Acoustic Waves in a Uranium Gas Core Reactor" under advisor D.A. Tidman. His research interests span Space Physics, Plasma Physics, Solar Wind dynamics, Magnetic Reconnection mechanisms, Collisionless Shocks, and Magnetospheric Physics. Scudder has made significant contributions to understanding non-thermal electron distributions in the solar wind, the role of ambipolar electric fields, and the fundamental processes of magnetic reconnection in space plasmas. His work often bridges theoretical models with spacecraft observations from missions like Voyager, ISEE-1, and NASA's Magnetospheric Multiscale Mission. Analysis of his recent publications (2012-2023) reveals a strong focus on non-Maxwellian distributions in space plasmas, with particular emphasis on solar wind electron behavior, the thermal force in astrophysical plasmas, and detailed measurements of magnetic reconnection sites. His research demonstrates a consistent theme of challenging conventional assumptions about plasma behavior in space environments, particularly the ubiquitous presence of non-thermal particle distributions. NASA Exceptional Scientific Achievement Medal, 1991 NASA Group Achievement Award for GGS-Polar Hydra Experiment, June, 1998 NASA Special Achievement Awards (1976, 1979, 1981, 1986) NASA Voyager Group Achievement Awards (Saturn 1983, Uranus 1986) NASA Voyager (Cruise, Jupiter) Certificate of Appreciation, 1981 Professor Scudder has advised several graduate students, including Arthur J. Hull (PhD 1998) and John C. Dorelli (PhD 1999), as well as Master's students Chonghui Shen, Robert Holdaway, and Xuejun Cao. He has served as Principal Investigator for the Polar Hydra Hot Plasma Experiment and was Deputy Project Scientist for the ISTP/GGS Wind and Polar Spacecraft missions. His professional service includes editorial work for the Journal of Geophysical Research and extensive proposal reviewing for NASA and NSF. As Principal Investigator for the Polar Hydra Hot Plasma Experiment and through his long-standing involvement with NASA missions including Voyager, ISEE-1, and MMS, Scudder has led significant laboratory and spacecraft-based investigations of space plasma phenomena. His research group has contributed to the fundamental understanding of collisionless plasma processes that govern space weather and astrophysical environments.
Brian Walsh is an Associate Professor of Mechanical Engineering at Boston University, with affiliations in the Departments of Astronomy and Electrical and Computer Engineering. He holds a Ph.D. in Mechanical Engineering from Boston University (2011) and a B.A. from Colgate University (2006). His research focuses on experimental space physics and spacecraft instrumentation, particularly studying solar wind-magnetosphere interactions, magnetopause reconnection, and X-ray imaging techniques. His work investigates energy transfer from the Sun to Earth's space environment, with a primary focus on the magnetopause. Walsh develops instruments for NASA and ESA missions, including the LEXI lunar X-ray imager and the CuPID CubeSat. He has contributed to missions like SMILE and pioneered compact solar energetic particle telescopes. His research spans CubeSat-based observations and large-scale space missions, emphasizing cross-scale coupling and global magnetospheric dynamics. Key research interests include plasma turbulence, magnetosheath dynamics, and exosphere variability. Walsh collaborates on projects like the Trans-Heliospheric Survey and the Magnetospheric Constellation (MagCon), aiming to advance understanding of heliospheric plasma behavior. His work also addresses space weather prediction and instrument calibration, such as the Carruthers Observatory Student Solar Monitor (COSSMo). Walsh's recent studies explore solar wind acceleration, ionospheric outflow asymmetry, and the role of recirculated plasmasphere material in ring current dynamics. His contributions to instrumentation and mission design highlight his dual role as a researcher and engineer in aerospace and space physics.
Patrick Antolin is an Associate Professor at Northumbria University's Department of Mathematics, Physics and Electrical Engineering. His research focuses on solar atmospheric phenomena, including coronal heating via MHD waves, coronal cooling processes (e.g., coronal rain and prominences), and thermal instabilities. He holds dual PhDs from Kyoto University (2009, numerical simulations) and the University of Oslo (2012, solar observations). Education: BSc Mathematics (2003), Universidad de los Andes, Colombia BSc Physics (2004), Universidad de los Andes, Colombia MSc (2006), Kyoto University, Japan PhD (2009), Kyoto University PhD (2012), University of Oslo Research Interests: Magnetohydrodynamics (MHD) and wave dynamics Numerical modelling (parallel computing) Forward modelling of observational diagnostics Solar observations using space- and ground-based instruments His work emphasizes understanding coronal heating mechanisms, thermal non-equilibrium processes, and the role of magnetic topology in solar phenomena. Key Contributions: Developed models for coronal rain formation via thermal instabilities near magnetic null points Investigated MHD wave-driven heating in coronal loops Advanced techniques for decomposing solar EUV emissions to study plasma components Awards: 2018: The Cool Alter-Ego of the Hot Solar Corona (recognizing contributions to thermal non-equilibrium research) Grants & Activities: Recipient of STFC Ernest Rutherford Fellowship (2016–2019) Collaborator on Solar Orbiter/EUI Consortium since 2020 Organized COSPAR 2021 sessions on solar physics Lab/Team: Leads a research group focusing on solar coronal dynamics, numerical simulations, and multi-wavelength observational analysis.
