Doerr, H.-P.; Iglesias, F.; Lagg, A.; van Noort, M.; The GRIS+ Tteam: GRIS+ - Instrument Setup and First Data. GREGOR technical development meeting, Potsdam, Germany (2017)
Doerr, H.-P.; van Noort, M.: Progress of workpackage 4.2: spectro-polarimetry using a microlens-fed spectrograph. GREST Board Meeting, Rome, Italy (2017)
Milic, I.; van Noort, M.: Response functions for NLTE lines. Solarnet IV Meeting : 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)
van Noort, M.; Doerr, H.-P.: Status of work-package 4.2: spectropolarimetry using a microlens-fed spectrograph. GREST board meeting, Brussels, Belgium (2017)
van Noort, M.; Feller, A.; de la Cruz-Rodriguez, J.; Doerr, H.-P.; Kiselman, D.: Image restoration of polarimetric spectrograph data. SOLARNET IV: The Physics of the Sun from the Interior to the Outer Atmosphere , Lanzarote, Spain (2017)
Zeuner, F.; Feller, A.; van Noort, M.; Iglesias, F.; Reardon, K.: Fast dual-beam spectropolarimetry - first results on scattering polarization measurements with FSP II at the DST. AG 2017 HiRes Splinter, Göttingen, Germany (2017)
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)
van Noort, M.; Feller, A.; Iglesias, F. A.; Doerr, H.-P.: Image restoration with a grating spectro-polarimeter at the SST and plans for GREGOR/GRIS. 2nd GREGOR/SOLARNET science meeting, Göttingen, Germany (2016)
Chanumolu, A.; van Noort, M.: Model based Calibrations for Microlens fed hyperspectral imager (MiHI). Astronomische Gesellschaft 2017 , Göttingen, Germany (2017)
Tapia, A. L. S.; Solanki, S. K.; Lagg, A.; van Noort, M.: ANOMALOUS REVERSED EVERSHED FLOW IN A SUNSPOT PENUMBRA. Sunspot formation: theory, simulations and observations, Stockholm, Sweden (2015)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".