da Silva Santos, J. M.; Danilovic, S.; Leenaarts, J.; de la Cruz Rodríguez, J.; Zhu, X.; White, S. M.; Vissers, G. J. M.; Rempel, M.: Heating of the solar chromosphere through current dissipation. Astronomy and Astrophysics 661, p. A59 (2022)
Vissers, G. J. M.; Danilovic, S.; Zhu, X.; Leenaarts, J.; Díaz Baso, C. J.; da Silva Santos, J. M.; de la Cruz Rodríguez, J.; Wiegelmann, T.: Active region chromospheric magnetic fields. Observational inference versus magnetohydrostatic modelling. Astronomy and Astrophysics 662, p. A88 (2022)
Jafarzadeh, S.; Solanki, S. K.; Stangalini, M.; Steiner, O.; Cameron, R. H.; Danilovic, S.: High-frequency Oscillations in Small Magnetic Elements Observed with SUNRISE/SuFI. Astrophysical Journal, Suppl. Ser. 229 (1), 10 (2017)
Lites, B. W.; Rempel, M.; Borrero, J. M.; Danilovic, S.: Are Internetwork Magnetic Fields in the Solar Photosphere Horizontal or Vertical? Astrophysical Journal 835 (1), 14 (2017)
Danilovic, S.; Rempel, M.; van Noort, M.; Cameron, R.: Observed and simulated power spectra of kinetic and magnetic energy retrieved with 2D inversions. Astronomy and Astrophysics 594, A103 (2016)
Danilovic, S.; Solanki, S. K.; Livingston, W.; Krivova, N.; Vince, I.: Variation of the Mn I 539.4 nm line with the solar cycle. Astronomy and Astrophysics 587, A33 (2016)
Danilovic, S.; van Noort, M.; Rempel, M.: Internetwork magnetic field as revealed by two-dimensional inversions. Astronomy and Astrophysics 593, A93 (2016)
Yeo, K. L.; Feller, A.; Solanki, S. K.; Couvidat, S.; Danilovic, S.; Krivova, N. A.: Point spread function of SDO/HMI and the effects of stray light correction on the apparent properties of solar surface phenomena. Astronomy and Astrophysics 561, A22 (2014)
Bello González, N.; Danilovic, S.; Kneer, F.: On the structure and dynamics of Ellerman bombs Detailed study of three events and modelling of Hα. Astronomy and Astrophysics 557, A102 (2013)
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".