Roudier, T.; Rieutord, M.; Malherbe, J. M.; Renon, N.; Berger, T.; Frank, Z.; Prat, V.; Gizon, L.; Švanda, M.: Quasi full-disk maps of solar horizontal velocities using SDO/HMI data. Astronomy and Astrophysics 540, A88 (2012)
Žlebčík, R.; Švanda, M.; Klvana, M.: Space-time segmentation method for study of the vertical structure and evolution of solar supergranulation from data provided by local helioseismology. New Astron. 16 (1), pp. 1 - 5 (2011)
Švanda, M.; Klvana, M.; Sobotka, M.: Large-scale horizontal flows in the solar photosphere V: Possible evidence for the disconnection of bipolar sunspot groups from their magnetic roots. Astronomy and Astrophysics 506, pp. 875 - 884 (2009)
Doctoral candidates joining the Solar System School are offered attractive funding, clear prospects and optimal career conditions. IMPRS-funded students receive a three-year doctoral support contract at 65% pay level. Additional funds are available for travel to international conferences. Following their PhD period, graduates are offered postdoc wrap-up funding.