Ploner, S. R. O.; Schüssler, M.; Solanki, S. K.; Sheminova, V. A.; Gadun, A. S.; Frutiger, C.: The formation of one-lobed Stokes V profiles in an inhomogeneous atmosphere. In: Advanced Solar Polarimetry - Theory, Observation and Instrumentation, pp. 371 - 378 (Ed. Sigwarth, M.). (2001)
Rempel, M.; Schüssler, M.: Intensification of a magnetic field in a stellar convection zone by conversion of potential energy. In: Magnetic Fields Across the Hertzsprung-Russell Diagram, pp. 165 - 168 (Eds. Mathys, G.; Solanki, S. K.; Wickramasinghe, D. T.). Astronomical Society of the Pacific, San Francisco, USA (2001)
Rempel, M.; Schüssler, M.; Moreno-Insertis, F.: Storage of a strong magnetic field below the solar convection zone. In: Cool Stars, Stellar Systems, and the Sun, pp. CD - 738 (Eds. López, G.; J., R.; Rebolo; R.; Osorio, Z. et al.). Astronomical Society of the Pacific, San Francisco (2001)
Schüssler, M.: Numerical simulation of solar magneto-convection (review). In: Advanced Solar Polarimetry - Theory, Observation and Instrumentation, pp. 343 - 354 (Ed. Sigwarth, M.). Astronomical Society of the Pacific, San Francisco, USA (2001)
Schüssler, M.; Holzwarth, V.; Solanki, S. K.; Charbonnel, C.: Buried flux tubes in the coronal graveyard. In: Cool Stars, Stellar Systems and the Sun, pp. CD - 1114 (Eds. López, G.; J., R.; Rebolo; R.; Osorio, Z. et al.). Astronomical Society of the Pacific, San Francisco (2001)
Schüssler, M.; Knölker, M.: Magneto-Convection (review). In: Magnetic Fields Across the Hertzsprung-Russell Diagram, pp. 115 - 123 (Eds. Mathys, G.; Solanki, S. K.; Wickramasinghe, D. T.). Astronomical Society of the Pacific, San Francisco, USA (2001)
Schüssler, M.: Photospheric research: where are we and what's next? (invited). NSO Workshop #30: High resolution solar physics: past, present, future, Sacramento Peak Obs., New Mexico, USA (2017)
Schüssler, M.: Solar magnetic fields: from complexity to simplicity (invited). 48th Meeting of the AAS Solar Physics Dvision, Portland, Oregon, USA (2017)
Cameron, R. H.; Schüssler, M.: The Babcock-Leighton solar dynamo. SOLARNET III / HELAS VII / SpaceInn Conference "The Sun, the stars, and solar-stellar relations", Freiburg, Germany (2015)
Jiang, J.; Cameron, R. H.; Schüssler, M.: The cause of the weak solar cycle 24. SOLARNET III / HELAS VII / SpaceInn Conference "The Sun, the stars, and solar-stellar relations", Freiburg, Germany (2015)
Schüssler, M.: Small-scale dynamo action in the Sun. ISSI Workshop on "Solar Magnetic Fields: From Measurements Towards Understanding", Bern, Switzerland (2015)
Schüssler, M.: Simulation of magnetic structure in the photosphere. Annual meeting of the Astronomische Gesellschaft, Splinter session on "High Resolution Physics'', Bamberg, Germany (2014)
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".