جست‌وجوی استاد و پژوهشگر

Gregor J. Golabekمشاهده پروفایل

دانشیار

• Planetary Geodynamics
• Terrestrial Planet Evolution
• Mantle Rheology
• +۳ مورد دیگر

Gregor J. Golabek serves as Associate Professor at the Bavarian Geo Institute, University of Bayreuth, Germany, where he investigates planetary-scale geodynamical processes through numerical and analytical modeling to unravel the evolution of planetary interiors. His research focuses on terrestrial planet thermomechanical evolution, comet dynamics, Earth's lower mantle rheology (including strain weakening and grain size evolution), and planet formation processes. He integrates multidisciplinary approaches from astrophysics, geochemistry, and rock physics to address fundamental questions about planetary body formation and evolution, with particular emphasis on early solar system dynamics and exoplanetary systems. Recent publications (2022-2025) demonstrate consistent output in high-impact journals, revealing strong thematic focus on Mars/Venus geodynamics, Earth's mantle evolution, and exoplanet characterization. His methodological approach combines cutting-edge numerical simulations (StagYY, SPH) with experimental validation, frequently incorporating observational data from spacecraft missions like MAVEN and James Webb Space Telescope. Golabek actively recruits master's and PhD students for geodynamics research, maintaining extensive international collaborations with institutions including ETH Zurich, University of British Columbia, and University of Groningen across projects spanning planetary formation, impact cratering, and mantle convection dynamics.

• Planetary Science
• Astrophysics
• Geophysics
• +۳ مورد دیگر

Wieland Dietrich is a Researcher and Research Coordinator at the Max Planck Institute for Solar System Research (MPS) , affiliated with the Planetary Science Department. His expertise lies in planetary dynamics, particularly the magnetic fields and atmospheric flows of exoplanets like Hot Jupiters, as well as convection processes in planetary cores and gas giants. Education & Employment : PhD in Physics (2009-2012): IMPRS program at MPS, Katlenburg-Lindau Postdoctoral Research Fellow (2013-2019): University of Leeds (School of Applied Mathematics) and MPS Current roles since 2022: Research Coordinator at MPS Research Focus : Investigates dynamo processes, zonal winds, and satellite measurement correlations with planetary interiors. Recent work emphasizes Hot Jupiter atmospheres and gravity dynamics of gas giants like Jupiter. Publications : Focused on exoplanet magnetism, zonal wind mechanisms, and computational models of planetary convection. Key contributions include studies on KELT-9b's magnetic fields and Jupiter's gravity moments. Awards : None explicitly mentioned in the provided texts. Labs & Teams : Active within the Planetary Science Department at MPS, contributing to interdisciplinary research on solar system and exoplanetary dynamics.

Raymond Burstonمشاهده پروفایل

پژوهشگر

• Solar Physics
• Helioseismology
• Solar Dynamics
• +۳ مورد دیگر

Raymond Burston is a Researcher at the Department of Solar and Stellar Interiors within the Max Planck Institute for Solar System Research, part of the prestigious Max Planck Society. His work focuses on understanding the complex dynamics of our Sun through advanced helioseismic techniques and analysis of solar observational data from missions like SDO/HMI. Burston has established himself as a significant contributor to solar physics research through numerous publications and collaborations with leading scientists in the field. Dr. Burston's research primarily centers on helioseismology, solar dynamics, and the study of solar active regions. His work investigates solar surface flows, supergranulation patterns, and the interpretation of helioseismic travel times to understand the Sun's interior structure and dynamics. He has made notable contributions to understanding the emergence of solar active regions, the structure and evolution of solar supergranulation, and the development of methodologies for analyzing solar observational data. His research often involves sophisticated mathematical modeling of solar phenomena and requires expertise in both theoretical physics and data analysis. Analysis of Burston's publication record reveals a consistent focus on solar physics with particular emphasis on helioseismic techniques. His work demonstrates a progression from theoretical aspects of helioseismology to practical applications using data from major space-based solar observatories. A significant portion of his research involves collaborations with the team led by Laurent Gizon at the Max Planck Institute, indicating his integration into a leading solar physics research group. His contributions span both observational analysis and methodological development in the field. Burston has been actively involved in major space missions including PLATO (PLAnetary Transits and Oscillations of stars) and the Solar Dynamics Observatory. His work on data center development and analysis systems for these missions highlights his role in bridging theoretical research with practical data processing infrastructure. While his primary focus remains solar physics, some of his earlier publications also touch on gravitational perturbations, demonstrating a broader physics background.

• Materials under extreme conditions
• High-pressure geophysics
• Planetary core composition
• +۲ مورد دیگر

Deng Liwei is an Associate Professor at the School of New Materials and New Energy, Shenzhen University of Technology, and a Shenzhen High-Level Talent. He holds a doctorate in Engineering from Southwest Jiaotong University and has conducted postdoctoral research at Peking University and the Carnegie Institution of Geophysics. PhD (2008): Southwest Jiaotong University BSc (2003): Sichuan Normal University His research focuses on theoretical and experimental studies of material properties under extreme conditions, particularly relevant to planetary cores and deep Earth processes. His work involves numerical simulation, high-pressure experiments, and computational modeling of minerals like MgSiO3 perovskite, feldspars, and iron alloys. Recent publications highlight studies on lunar mantle hydration, planetary core composition, and phase transitions in mantle minerals. His work integrates computational approaches with experimental validation using techniques like synchrotron X-ray diffraction and shock compression. Scientific Awards : Shenzhen High-Level Talent (2019) As principal investigator, he has led NSFC-funded projects on carbon solubility in mantle minerals and participated in major CAS and NSFC initiatives. He serves as a reviewer for multiple journals and collaborates with institutions like Argonne National Laboratory and the Carnegie Institution.

Christopher Beyerمشاهده پروفایل

پژوهشگر

• Experimental Petrology
• Geochemistry
• Mineralogy
• +۴ مورد دیگر

Christopher Beyer is a Research Scientist and Experimental Petrology Lab Manager at Ruhr-Universität Bochum (RUB), Germany. He oversees experimental research and teaches courses in Mantle Petrology (MSc) and Mineralogy (BSc). Beyer holds a B.Sc. and M.Sc. in Geosciences from WWU Münster, and a Dr. rer. nat. in Experimental Petrology from the University of Bayreuth. His positions include postdoctoral roles at RUB and Bayreuth before transitioning to his current managerial role in 2019. Beyer's research focuses on Experimental Petrology , Geochemistry , and Mantle Processes . He investigates the cycling of carbon, sulfur, and halogens in the sublithospheric mantle, element partitioning under high-pressure conditions, and diffusion processes in minerals. His work employs advanced techniques like high-pressure experiments and 3D imaging to explore mantle heterogeneities and metasomatism. His recent publications (2012–2024) emphasize sulfide melt behavior, diamond formation, redox gradients, and diffusion kinetics. Trends include high-pressure mineralogy, experimental method innovations, and mantle geodynamics. Beyer leads DFG-funded projects on mantle melt mobility (BE 6053/5-1), diamond formation (BE 6053/1-1), and magmatic sulfides (BE 6053/2-1), collaborating with institutions worldwide. He manages RUB's Experimental Petrology Lab, partnering with researchers from Imperial College London, University of Bristol, and DESY Hamburg.

Markus Nielbockمشاهده پروفایل

پژوهشگر

• Astronomy Education
• Science Communication
• Exoplanet Research
• +۴ مورد دیگر

Markus Nielbock works at the Max Planck Institute for Astronomy (MPIA) and the House of Astronomy (HdA), leading science communication initiatives. He develops educational materials for secondary schools, oversees public relations, contributes to the ESO Science Outreach Network, and supervises students in astronomy-related contexts. His career spans research, outreach, and teaching roles. PhD in physics and astronomy (2001) ESO Fellowship in Chile (2001-2003) Postdoctoral research at the University of Bochum (2003-2006) Project scientist for the Herschel Space Telescope at MPIA (2006-2015) Research associate at the House of Astronomy (2015-present) Public relations at MPIA (2018-present) Nielbock's research interests focus on astronomy education, science communication, exoplanet detection techniques, and historical navigation methods. He has developed instructional materials on topics like the transit and radial velocity methods, celestial navigation, and Earth's climate systems. His work bridges astrophysical research with accessible pedagogical resources. He has taught block courses on Introduction to Astronomy for Secondary School Teachers from WS 2016/17 to WS 2023/24, emphasizing practical applications of astronomy. His publications in Science in Schools and astroEDU cover subjects ranging from exoplanets to historical navigation and climate science. Nielbock is involved in organizing public lectures and events to promote astronomy. He collaborates with institutions like the ESO and contributes to educational projects such as Space for Education . His outreach includes media interviews on planetary science and space missions, available via Creative Commons licenses.

Rudolf Widmer-Schnidrigمشاهده پروفایل

پژوهشگر

• Low-Frequency Seismology
• Planetary Interior Structure
• Mars Geophysics
• +۳ مورد دیگر

Rudolf Widmer-Schnidrig is a Researcher at the Institute of Geodesy within Faculty 06 at the University of Stuttgart. He is affiliated with the Black Forest Observatory (BFO) , where he specializes in low-frequency seismology to study Earth's mantle and core structure through elasto-gravitational free oscillations. His work extends to analyzing data from the InSight mission on Mars, contributing to understanding planetary interiors and Martian atmospheric processes. Recently, he has explored signatures of compact dark matter objects using terrestrial gravimeter data. Research focuses include seismic sensor calibration (e.g., DAS systems), atmospheric-seismic interactions, and long-period Earth oscillations. He has been instrumental in testing seismometers for Mars missions and interpreting InSight's seismic/meteorological data. His collaborative efforts span global seismology networks and interplanetary geophysical comparisons. Publications highlight innovations in sensor technology, Mars regolith characterization, and detection of rare seismic phenomena like 9-day Greenland fjord tsunamis. While no formal awards are listed, his contributions to planetary science and gravitational wave research are notable.

Anant Hariharanمشاهده پروفایل

پژوهشگر

• Structural Seismology
• Inverse Theory
• Wave Propagation
• +۶ مورد دیگر

Anant Hariharan is a Postdoctoral Researcher in the Department of Earth Science at the University of California, Santa Barbara, specializing in structural seismology, inverse theory, and wave propagation to investigate Earth's interior from crust to lower mantle across regions including the Continental U.S., Greenland, and oceanic settings. Education: PhD in Earth, Environmental and Planetary Sciences, Brown University (2023) BA in Geological Sciences and Physics, Cornell University (2018), Summa Cum Laude Hariharan's research centers on improving seismic data quality and imaging algorithms, with emphasis on surface wave analysis (Love/Rayleigh waves) and overtone interference effects. His work spans multi-scale structural investigations from upper crust to lower mantle, utilizing seismic arrays like USArray and OldORCA to address challenges in mantle anisotropy, heterogeneity, and wave propagation physics. Publication trends reveal progression from mineral physics (2016) to advanced seismic tomography (2019-2025), with consistent focus on overtone interference mitigation. Recent work (2023-2025) produces high-resolution models of U.S. continental structure and oceanic lithosphere, while extending methodologies to planetary seismology. Key contributions include first Love wave phase velocity maps spanning the entire U.S. and frameworks for quantifying interference-induced measurement errors. Scientific Awards: No awards mentioned As a postdoctoral researcher, Hariharan has no listed advisees. The provided text specifies no grants or principal investigator roles. Hariharan collaborates with research teams utilizing USArray and OldORCA seismic arrays. Current projects include high-resolution imaging of oceanic upper mantle heterogeneity, radial anisotropy mapping beneath the continental U.S., and planetary extension of overtone interference analysis for Moon/Mars seismology.

Alicia Neesemannمشاهده پروفایل

پژوهشگر

• Planetary Geology
• Remote Sensing
• Impact Crater Analysis
• +۴ مورد دیگر

Alicia Neesemann serves as a Scientific Staff Member within the Planetary Sciences and Remote Sensing working group at Freie Universität Berlin's Institute of Geological Sciences. Her research focuses on high-precision imaging and coregistration techniques applied to planetary surfaces, particularly through involvement in NASA's Dawn mission to Ceres and Mars exploration projects. Her research interests center on planetary geology with specialization in impact crater analysis, topographic mapping of dwarf planets, and remote sensing of surface processes. Key areas include cryovolcanism on Ceres, Martian aeolian features, and the geological evolution of airless bodies. Her work integrates stereo photogrammetry, crater counting chronology, and compositional analysis to unravel planetary histories. Neesemann's publication record since 2017 demonstrates consistent contributions to major planetary science journals including Geophysical Research Letters , Icarus , and Nature . Her research shows a pronounced focus on Ceres' geological features - particularly Occator crater's faculae formation mechanisms, crater chronology, and volatile-driven surface processes. Recent work extends to ExoMars landing site characterization and high-precision topographic mapping for Mars 2020 mission support. No scientific awards or major honors are documented in the available materials. Her collaborative research involves extensive work with international teams including Dawn mission scientists and planetary geologic mappers. Neesemann maintains active participation in planetary mapping initiatives and contributes to ongoing analysis of Ceres and Mars datasets. Her laboratory work involves advanced digital terrain modeling and stereo imaging processing within the Planetary Sciences and Remote Sensing group at FU Berlin.

• Planet Formation
• Star Formation
• Exoplanets
• +۳ مورد دیگر

Remo Burn is a Researcher at the Max Planck Institute for Astronomy (MPIA) in Heidelberg, Germany. His research focuses on Planet and Star Formation within the ERC Origins, Planet Formation and Exoplanets, and Theory of Planet and Star Formation research groups. Key areas of expertise include protoplanetary disk dynamics, exoplanet formation mechanisms, and planetary population synthesis modeling. Remo’s work addresses fundamental questions about how giant planets form in gas-rich disks, the role of pebble accretion in planetary growth, and the connection between planetary architectures and stellar host properties. Recent projects include analyzing protoplanet dynamics around PDS 70, studying resonant exoplanet systems like TOI-6695, and investigating the ‘radius valley’ phenomenon observed in sub-Neptune populations. His research leverages cutting-edge observational facilities such as TESS, CARMENES, and HARPS, combining empirical data with advanced numerical models to simulate planet formation processes. Collaborations with international teams (e.g., WINE Survey, NCORES Program) highlight his role in large-scale exoplanet detection and characterization efforts. Remo’s contributions bridge observational astronomy and theoretical astrophysics, emphasizing the interplay between disk evolution, planetary migration, and atmospheric evolution. His work has advanced understanding of planet formation pathways around low-mass stars, particularly challenging existing models with discoveries like the gas giant around GJ 3512.

Alejandro Cardesin-Moineloمشاهده پروفایل

پژوهشگر

• Planetary Science
• Aerospace Engineering
• Remote Sensing
• +۵ مورد دیگر

Alejandro Cardesín Moinelo works at the European Space Astronomy Centre in Madrid, Spain, where he serves as a manager in the Science Operations Department . He holds a PhD in Aerospace Science and Engineering and has been actively involved in several planetary missions including Mars Express , ExoMars , JUICE , Mars Express , and Venus Express . Current role: Science Operations Manager at European Space Astronomy Centre Key collaborations: Universidad del País Vasco, Instituto de Astrofísica e Ciências do Espaço, Space Science Institute, Institute for Space Aeronomy, Laboratoire de Météorologie Dynamique His research interests span Solar System Exploration , Terrestrial Planets (Mars and Venus), Planetary Atmospheres , Remote Sensing , and Spectroscopy . He focuses on spacecraft geometry , science operations planning , and payload data processing for planetary missions. His recent publications highlight trends in Martian atmospheric dynamics , Venusian cloud analysis , mission coordination , and planetary protection protocols . Notably, he has contributed to VIRTIS instrument calibration and global dust storm studies on Mars. Cardesín Moinelo leads the Chair of the EuroPlanet Society Spain&Portugal Regional Hub and coordinates the Spanish Planetary Science & Solar System Exploration Community . His work supports international collaboration in planetary science and space exploration through coordinated observations and data sharing initiatives. He has been instrumental in adapting aging spacecraft operations for continued science return, particularly during Mars Express' deep eclipse studies . His grants likely involve ESA-funded Mars wind and wave mapping and planetary protection research . The Mars Express Visual Monitoring Camera (VMC) has been repurposed under his guidance into a valuable science instrument for cloud analysis and atmospheric studies . His laboratory environment involves mission operations centers and multi-institutional research networks across Europe and international partners.

• Helioseismology
• Asteroseismology
• Solar Physics
• +۷ مورد دیگر

Laurent Gizon is Director of the Department of Solar and Stellar Interiors at the Max Planck Institute for Solar System Research and Full Professor at the Institute for Astrophysics, University of Göttingen. He has held leadership and research positions at these institutions since 2005 and 2009, respectively, and is a Scientific Member of the Max Planck Society. PhD in Physics, Stanford University (2003) M.Sc. in Astrophysics, Université Paul Sabatier, Toulouse Ingénieur SUPAERO, Ecole nationale supérieure de l'aéronautique et de l'espace, France Laurent Gizon specializes in helioseismology and asteroseismology, focusing on probing the internal structure, rotation, and dynamics of the Sun and solar-like stars. His research leverages data from space missions like SDO, Kepler, and Solar Orbiter to investigate solar convection, sunspots, supergranulation, and stellar oscillations. He develops advanced inversion techniques and numerical models to interpret seismic travel times and infer subsurface flows and magnetic fields. His recent publications (2014–2015) reflect a strong focus on asteroseismology, solar rotation, wave propagation in magnetized plasmas, and data analysis techniques. Topics include differential rotation in Kepler stars, seismic sounding of convection, magnetic flux transport, and 3D simulations of wave interactions with stellar spots. His work integrates observational data with theoretical modeling to refine our understanding of stellar interiors. Notable scientific awards include: Karen Harvey Prize (2009) ERC Starting Grant (2007) ERC Synergy Grant (2018) NASA Group Achievement Award (2012) JOSO Prize (2005) Scientific Member, Max Planck Society (2011) Gizon has served as coinvestigator on the Solar Orbiter's PHI instrument, board member of the PLATO Mission Consortium, and editorial board member of Solar Physics . He has advised numerous PhD students and postdoctoral researchers and has led major collaborative projects such as HELAS. He has also edited significant scientific volumes on helioseismology and MHD connections. His leadership in international consortia and space missions underscores his role in shaping the future of solar and stellar physics. He leads research teams at the Max Planck Institute and collaborates with institutions worldwide, including Stanford University, New York University Abu Dhabi, and various European space agencies. His group develops computational tools for helioseismic inversions and contributes to data analysis pipelines for current and upcoming solar and stellar missions.

• Environmental Science
• Geophysics
• Sustainable Resource Management
• +۳ مورد دیگر

Bin Chen is a Professor of Environmental Modeling at Beijing Normal University , with a Ph.D. in Environmental Science from Peking University and a B.E. in Electrical Engineering from Zhejiang University. His work bridges environmental systems analysis, urban sustainability, and geophysical research. Editorial Roles : Associate Editor for Earth and Planetary Materials (Frontiers in Earth Science), Chief Editor for Smart Technologies (Frontiers in Sustainable Resource Management) His research spans: Environmental Science : Urban waterlogging, antibiotic resistance aerosols, carbon emission drivers, wastewater-energy nexus Geophysics : Mantle dynamics, diamond formation, high-pressure mineral elasticity Plant Physiology : Root-level identity recognition, clonal fragment interactions Recent publications highlight interdisciplinary approaches combining computational modeling, geophysical analysis, and sustainability frameworks. Key journals include Science Advances , Nature Communications , and Earth and Planetary Science Letters .

Philipp Baumeisterمشاهده پروفایل

پژوهشگر

• Exoplanet Interior Structure
• Planetary Geodynamics
• Habitability Modeling
• +۳ مورد دیگر

Dr. Philipp Baumeister is a Postdoctoral Researcher in Planetary Geodynamics at the Institute of Geological Sciences, Department of Earth Sciences, Freie Universität Berlin. He works on the DIVerse Exoplanet Redox State Estimations (DIVERSE) project, focusing on the relationship between planetary interior structure, redox state, and habitability potential of exoplanets. His research combines geophysical modeling with machine learning techniques to rapidly characterize exoplanet interiors. Dr. Baumeister completed his academic training at Technische Universität Berlin, earning a B.Sc. in Physics (2011-2015), M.Sc. in Physics (2015-2017) with thesis on heat-piping effects on Earth's interior evolution, and a PhD in Physics (2018-2023) with dissertation on interior structure, mantle-atmosphere co-evolution, and habitability of low-mass exoplanets. His primary research interests include exoplanet interior structure modeling, planetary geodynamics, habitability assessment of stagnant-lid planets, redox state analysis, and machine learning applications in planetary science. He has developed innovative approaches like ExoMDN (Exoplanet Mixture Density Networks) to rapidly characterize exoplanet interiors using probabilistic machine learning. Analysis of his publication record shows a strong focus on the connection between planetary interior structure and atmospheric properties, with particular attention to stagnant-lid planets (like Venus and many exoplanets). His work increasingly incorporates machine learning methods to address computational challenges in exoplanet characterization, while maintaining rigorous physical modeling of planetary interiors and atmospheres. Dr. Baumeister actively collaborates with researchers across multiple institutions, as evidenced by his co-authorship on studies involving atmospheric modeling, exoplanet system characterization, and Venus research. His work on the DIVERSE project represents a significant contribution to understanding how planetary redox states influence long-term habitability potential.

Anna Julia Poserمشاهده پروفایل

پژوهشگر

• Exoplanet Research
• Planetary Science
• Planet Formation and Evolution
• +۴ مورد دیگر

Dr. Anna Julia Poser is a Postdoctoral Researcher in Planetary Geophysics at the Institute of Geological Sciences, Department of Earth Sciences, Free University of Berlin. She contributes to ESA's PLATO mission through exoplanet characterization and machine learning development for inferring planetary composition from observational data. Her academic background includes: PhD in Theoretical Physics, University of Rostock (2018-2024), Dissertation: From clouds to cores: advancing the understanding of giant irradiated exoplanets M.Sc. in Physics, University of Rostock (2014-2018), Thesis: Der Einfluss von Wolken in der Berechnung der Struktureigenschaften großer Exoplaneten (The influence of clouds in the calculation of structural properties of large exoplanets) B.Sc. in Physics, University of Rostock (2011-2014), Thesis: Masse-Radius-Relationen von Exoplaneten (Mass-radius relations of exoplanets) Dr. Poser specializes in coupled modeling of planetary interiors, atmospheres, and long-term evolution, with emphasis on hot Jupiters. Her doctoral research demonstrated how deep cloud layers alter planetary radius contraction and how atmospheric plasma-magnetic field interactions sustain inflated radii. Current work focuses on bridging theoretical models with PLATO mission observations through machine learning tools for exoplanet composition analysis. She is an active member of the Planetary Sciences and Remote Sensing working group within the Institute of Geological Sciences.