Roth, M.: Future missions for helioseismology. In: Modern Solar Facilities - Advanced Solar Science, pp. 85 - 88 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen, Göttingen, Germany (2007)
Di Mauro, M. P.; Cardini, D.; D'Antona, F.; Weiss, A.; Döllinger, M. P.; Pasquini, L.; Girardi, L.; Hatzes, A.; von der Lühe, O.; de Medeiros, J. R.et al.; Roth, M.; Setiawan, J.; da Silva, L.: Asteroseismology of K Giants. In: Proceedings of SOHO 18 / GONG 2006 / HELAS I - Beyond the spherical Sun, 7-11 August 2006, Sheffield, UK (Ed. Fletcher, K.). ESA Publ. Div., Noordwijk, The Netherlands (2006)
Roth, M.; Gizon, L.; Birch, A. C.: Sensitivity kernels for helioseismic travel times in spherical geometry - preliminary results. In: Proceedings of SOHO 18 / GONG 2006 / HELAS I - Beyond the spherical Sun, 7-11 August 2006, Sheffield, UK (Ed. Fletcher, K.). ESA Publ. Div., Noordwijk, The Netherlands (2006)
Roth, M.; v. d. Lühe, O.; Pallé, P.; Thompson, M. J.; Christensen-Dalsgaard, J.; Monteiro, M. J. P. F. G.; Gizon, L.; Di Mauro, M. P.; Aerts, C.; Daszynska-Daszkiewicz, J.et al.; Corbard, T.: European helio- and asteroseismology network - HELAS. In: Proceedings of SOHO 18 / GONG 2006 / HELAS I - Beyond the spherical Sun, 7-11 August 2006, Sheffield, UK (Ed. Fletcher, K.). ESA Publ. Div., Noordwijk, The Netherlands (2006)
Roth, M.; v. d. Lühe, O.; Pallé, P.; Thompson, M. J.; Christensen-Dalsgaard, J.; Monteiro, M. J. P. F. G.; Gizon, L.; Di Mauro, M. P.; Aerts, C.; Daszynska-Daszkiewicz, J.et al.; Corbard, T.: HELAS - European Helio- and Asteroseismology Network. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Ed. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
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".
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.