Chitta, L. P.; Peter, H.; Solanki, S.: Coronal loop footpoints threaded with small-scale mixed polarity surface magnetic fields. SOLARNET IV: The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
Iglesias, F. A.; Feller, A.; Solanki, S. K.; Zeuner, F.: Prototype characterization and future development of the Fast Solar Polarimeter. SOLARNET IV: The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
Siu-Tapia, A. L.; Lagg, A.; Solanki, S. K.; van Noort, M.; Rempel, M.: Photospheric counter-Evershed flows in the penumbra of sunspots. Solarnet IV Meeting "The physics of the Sun from the interior to the outer atmosphere", Lanzarote, Spain (2017)
Wu, C.-J.; Usoskin, I.; Krivova, N.; Kavoltsov, G.; Solanki, S.: Solar Spectral Irradiance Reconstruction over 9 Millennia from a Composite 14C and 10Be series. AGU Fall Meeting, New Orleans, USA (2017)
Zeuner, F.; Feller, A.; Iglesias, F.; Milic, I.; Solanki, S. K.: Spatially resolved Stokes measurements in the Sr I (4607.3 Å) line with FSP at VTT/TESOS. SOLARNET IV: The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
Chatzistergos, T.; Ermolli, I.; Solanki, S. K.; Krivova, N. A.: The potential of historical spectroheliograms for Sun-climate studies. 9th IAGA - ICMA/IAMAS - ROSMIC/VarSITI/SCOSTEP workshop on long-term changes and trends in the atmosphere, Kühlungsborn, Germany (2016)
Siu-Tapia, A. L.; Lagg, A.; Solanki, S. K.; van Noort, M.; Rempel, M.: Anomalous counter Evershed flows: HINODE observations and MHD simulations. IAU Symposium 327: Fine structure and dynamics of the solar atmosphere, Cartagena de Indias, Colombia (2016)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Why do measurements and models of UV SSI variability not agree? 9th IAGA - ICMA/IAMAS - ROSMIC/VarSITI/SCOSTEP workshop on Long-Term Changes and Trends in the Atmosphere, Kühlungsborn, Germany (2016)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
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.
Karen Harvey solar physics prize 2020 for Prof. Dr. Tian who studies dynamic phenomena in the Sun’s atmosphere; his research group is a partner group of the Max Planck Institute for Solar System Research.
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.