Cheung, M. C. M.; Schuessler, M.; Moreno-Insertis, F.: 3D magneto-convection and flux emergence in the photosphere. In: Proceedings of the International Scientific Conference on Chromospheric and Coronal Magnetic Fields (Eds. Innes, D.; Lagg, A.; Solanki, S. K.; Danesy, D.). ESA Publ. Div., Noordwijk (2006)
Cameron, R.; Vögler, A.; Schüssler, M.; Zakharov, V.: Simulations of solar pores. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Eds. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
Solanki, S. K.; Schüssler, M.: Small-scale solar magnetic elements: simulations and observations. In: The Solar-B Mission and the Forefront of Solar Physics, pp. 105 - 114 (Eds. Sakurai, T.; Sekii, T.). Astronomical Society of the Pacific, San Francisco (2005)
Usoskin, I. G.; Schüssler, M.; Solanki, S. K.; Mursula, K.: Solar activity over the last 1150 years: does it correlate with climate? In: Proc. The 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, pp. 19 - 22 (Eds. Favata, F.; Hussain, G. A. J.; Battrick, B.). ESA Publ. Div., Noordwijk (2005)
Cameron, R.; Vögler, A.; Shelyag, S.; Schüssler, M.: The Decay of a Simulated Pore. In: The Solar-B Mission and the Forefront of Solar Physics, pp. 57 - 62 (Eds. Sakurai, T.; Sekii, T.). (2004)
Gandorfer, A. M.; Solanki, S. K.; Schüssler, M.; Curdt, W.; Lites, B. W.; Martínez Pillet, V.; Schmidt, W.; Title, A. M.; the Sunrise Team: SUNRISE: High resolution UV/VIS observations of the Sun from the stratosphere. In: Astronomical Telescopes and Instrumentation - The Industrial Revolution in Astronomy, pp. 732 - 741 (Ed. Oschmann, J. M.). SPIE, Bellingham (2004)
Khomenko, E. V.; Shelyag, S.; Solanki, S. K.; Vögler, A.; Schüssler, M.: Stokes diagnostics of magneto-convection. Profile shapes and asymmetries. In: Multi-Wavelength Investigations of Solar Activity, Proc. IAU Symp. 223, pp. 635 - 636 (Eds. Stepanov, A. V.; Benevolenskaya, E. E.; Kosovichev, A. G.). University Press, Cambridge (2004)
Solanki, S. K.; Schüssler, M.: Small-Scale solar magnetic elements: simulations and observations. In: The Solar-B Mission and the Forefront of Solar Physics, pp. 105 - 113 (Eds. Sakurai, T.; Sekii, T.). (2004)
Schüssler, M.: MHD simulations: what's next? In: Solar Polarization 3, pp. 601 - 613 (Eds. Bueno, J. T.; Almeida, J. S.). Astron. Soc. of the Pacific, San Francisco (2003)
Schüssler, M.; The Sunrise Team: SUNRISE: Balloon-borne high-resolution observations of the Sun. In: Proc. of the 16th ESA Symposium on European Rocket and Balloon Programmes and Related Research, pp. 279 - 283 (Ed. Warmbein, B.). ESA Publ. Div., Noordwijk (2003)
Solanki, S. K.; Gandorfer, A. M.; Schüssler, M.; Curdt, W.; Lites, B. W.; Martinez Pillet, V.; Schmidt, W.; Title, A. M.; the SUNRISE Team: SUNRISE: A Balloon-borne Telescope for High Resolution Solar Observations in the Visible and UV. In: Innovative Telescopes and Instrumentation for Solar Astrophysics, pp. 129 - 139 (Eds. Keil, S. L.; Avakyan, S. V.). SPIE, Washington, US (2003)
Usoskin, I. G.; Mursula, K.; Solanki, S. K.; Schüssler, M.; Kovaltsov, G. A.: Long-term cosmic ray intensities: physical reconstruction. In: Proc. 28th Internat. Cosmic Ray Conf., pp. 4041 - 4044. Universal Academy Press Inc., Tokyo, Japan (2003)
Vögler, A.; Shelyag, S.; Schüssler, M.; Cattaneo, F.; Emonet, T.; Linde, T.: Simulation of solar magneto-convection. In: Modelling of Stellar Atmospheres, pp. 157 - 169 (Eds. Piskunov, N. E.; Weiss, W. W.; Gray, D. F.). Astron. Soc. of the Pacific, San Francisco (2003)
Schüssler, M.: Magnetic variability of the Sun. In: Proceedings of the Second Solar Cycle and Space Weather Conference, SOLSPA 2001,, pp. 3 - 8 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Schüssler, M.; Rempel, M.: Structure of the magnetic field in the lower convection zone. In: Proc. SOHO 11 Symposium ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 499 - 506 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Solanki, S. K.; Schüssler, M.; Curdt, W.; Lites, B. W.; Martinez-Pillet, V.; Schmidt, W.; Title, A. M.; the Sunrise Team: SUNRISE: A 1-m balloon borne solar telescope. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 27 - 32 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Granzer, T.; Caligari, P.; Schüssler, M.; Strassmeier, K. G.: Star Spot Patterns on Young Stars: Theoretical Approach. In: Cool Stars, Stellar Systems and the Sun, pp. CD - 1232 (Eds. López, G.; J., R.; Rebolo; R.; Osorio, Z. et al.). Astronomical Society of the Pacific, San Francisco (2001)
Holzwarth, V.; Schüssler, M.: Preferred longitudes of starspots on magnetically active close binaries. In: Magnetic Fields Across the Hertzsprung-Russell Diagram, pp. 247 - 250 (Eds. Mathys, G.; Solanki, S. K.; Wickramasinghe, D. T.). Astronomical Society of the Pacific, San Francisco, USA (2001)
Holzwarth, V.; Schüssler, M.; Solanki, S. K.: A model for the decline of coronal X-ray emission of cool giant stars. In: Magnetic Fields Across the Hertzsprung-Russell Diagram, pp. 259 - 262 (Eds. Mathys, G.; Solanki, S. K.; Wickramasinghe, D. T.). Astronomical Society of the Pacific, San Francisco/CA (2001)
Ploner, S. R. O.; Schüssler, M.; Solanki, S. K.; Gadun, A. S.: An example of reconnection and magnetic flux recycling near the solar surface. In: Advanced Solar Polarimetry - Theory, Observation and Instrumentation, pp. 363 - 370 (Ed. Sigwarth, M.). (2001)
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".