Schlegel, K.; Diendorfer, G.; Thern, S.; Schmidt, M.: Thunderstorms, lightning and solar activity - Middle Europe. Journal of Atmospheric and Solar-Terrestrial Physics 63, pp. 1705 - 1713 (2001)
Schmidt, J. M.: Spatial transport and spectral transfer of solar wind turbulence composed of Alfvén waves and convective structures II: Numerical results. Annales Geophysicae 13 (5), pp. 475 - 493 (1995)
Schmidt, J. M.; Marsch, E.: Spatial transport and spectral transfer of solar wind turbulence composed of Alfvén waves and convective structures I: The theoretical model. Annales Geophysicae 13 (5), pp. 459 - 474 (1995)
Schmidt, M.; Borchers, R.; Fabian, P.; Flentje, G.; Matthews, W. A.; Szabo, A.; Lal, S.: Trace gas measurements during aircraft flights in the tropopause region over Europe and North Africa. J. Atmos. Chem. 2, pp. 133 - 143 (1984)
Schmidt, M.: Results of ozone measurements in Northern Germany-A case study. In: Ozone in the Troposphere and Stratosphere, Part 1, pp. 170 - 173 (Ed. Hudson, R. D.). GSFC, Greenbelt (1994)
Schmidt, J.: Zur magneto-hydro-dynamischen Turbulenz im Sonnenwind und in der Sonnenkorona: numerische Simulation und Datenanalyse. Dissertation, Georg-August-Universität Göttingen (1993)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.