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)
Švanda, M.; Gizon, L.; Hanasoge, S. M.; Ustyugov, S. D.: Validated helioseismic inversions for 3D vector flows. Astronomy and Astrophysics 530, A148 (2011)
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)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.