Huybrighs, H.L.F.; Roussos, E.; Blöcker, A.; Krupp, N.; Futaana, Y.; Barabash, S.; Hadid, L.Z.; Holmberg, M.K.G.; Witasse, O.: Reply to Comment on “An Active Plume Eruption on Europa During Galileo Flyby E26 as Indicated by Energetic Proton Depletions”. Geophysical Research Letters 48 (18), e2021GL095240 (2021)
Palmerio, E.; Nieves-Chinchilla, T.; Kilpua, E. K. J.; Barnes, D.; Zhukov, A. N.; Jian, L. K.; Witasse, O.; Provan, G.; Tao, C.; Lamy, L.et al.; Bradley, T. J.; Mays, M. L.; Moestl, C.; Roussos, E.; Futaana, Y.; Masters, A.; Sanchez-Cano, B.: Magnetic Structure and Propagation of Two Interacting CMEs From the Sun to Saturn. Journal of Geophysical Research: Space Physics 126 (11), e2021JA029770 (2021)
Sun, Y. X.; Roussos, E.; Hao, Y. X.; Zong, Q.-G.; Liu, Y.; Lejosne, S.; Pan, D. X.; Zhou, X.-Z.; Yue, C.; Krupp, N.: Saturn's Inner Magnetospheric Convection in the View of Zebra Stripe Patterns in Energetic Electron Spectra. Journal of Geophysical Research: Space Physics 126 (10), e2021JA029600 (2021)
Bradley, T. J.; Cowley, S. W. H.; Bunce, E. J.; Melin, H.; Provan, G.; Nichols, J. D.; Dougherty, M. K.; Roussos, E.; Krupp, N.; Tao, C.et al.; Lamy, L.; Pryor, W. R.; Hunt, G. J.: Saturn's Nightside Dynamics During Cassini's F Ring and Proximal Orbits: Response to Solar Wind and Planetary Period Oscillation Modulations. Journal of Geophysical Research: Space Physics 125 (9), e2020JA027907 (2020)
Clark, G.; Mauk, B. H.; Kollmann, P.; Paranicas, C.; Bagenal, F.; Allen, R. C.; Bingham, S.; Bolton, S.; Cohen, I.; Ebert, R. W.et al.; Dunn, W.; Haggerty, D.; Houston, S. J.; Jackman, C. M.; Roussos, E.; Rymer, A.; Westlake, J. H.: Heavy Ion Charge States in Jupiter's Polar Magnetosphere Inferred From Auroral Megavolt Electric Potentials. Journal of Geophysical Research: Space Physics 125 (9), e2020JA028052 (2020)
Hedman, M. M.; Helfenstein, P.; Chancia, R. O.; Thomas, P.; Roussos, E.; Paranicas, C.; Verbiscer, A. J.: Photometric Analyses of Saturn's Small Moons: Aegaeon, Methone, and Pallene Are Dark; Helene and Calypso Are Bright. Astronomical Journal 159 (4), 129 (2020)
Huybrighs, H. L. F.; Roussos, E.; Blöcker, A.; Krupp, N.; Futaana, Y.; Barabash, S.; Hadid, L. Z.; Holmberg, M. K. G.; Lomax, O.; Witasse, O.: An Active Plume Eruption on Europa During Galileo Flyby E26 as Indicated by Energetic Proton Depletions. Geophysical Research Letters 47 (10), e2020GL087806 (2020)
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.
Inversion codes are used to aid the detailed interpretation of solar spectro-polarimetric data. This computer code attempts to find the atmospheric structure that produced an observed spectrum by minimizing the difference between the observed spectrum and a Stokes spectrum.
The MPS is one of the leading institutes worldwide in building instruments for solar research, both for ground based observatories as well as for balloon and space-borne missions. Scientists and engineers of MPS conceive new observing methods and develop novel instruments of highest technological complexity. These instruments are built in house, tested, calibrated, and used at the best solar observatories in the world, or delivered to NASA and ESA to be launched to space.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
Recently new, very sensitive observations of the ExoMars Trace Gas Orbiter (TGO) and its instruments NOMAD (Nadir and Occultation for MArs Discovery) an ACS (Atmospheric Chemistry Suite) became available and initiated a number of interesting scientific questions. Some of them are open PhD projects using the MPS General Circulation Model (MPS-GCM).