Ball, W. H.; Gizon, L.: A new correction of stellar oscillation frequencies for near-surface effects (Corrigendum). Astronomy and Astrophysics 569, C2 (2014)
Cameron, R. H.; Jiang, J.; Schuessler, M.; Gizon, L.: Physical causes of solar cycle amplitude variability. Journal of Geophysical Research: Space Physics 119, pp. 680 - 688 (2014)
Deheuvels, S.; Doğan, G.; Goupil, M. J.; Appourchaux, T.; Benomar, O.; Bruntt, H.; Campante, T. L.; Casagrande, L.; Ceillier, T.; Davies, G. R.et al.; De Cat, P.; Fu, J. N.; García, R. A.; Lobel, A.; Mosser, B.; Reese, D. R.; Regulo, C.; Schou, J.; Stahn, T.; Thygesen, A. O.; Yang, X. H.; Chaplin, W. J.; Christensen-Dalsgaard, J.; Eggenberger, P.; Gizon, L.; Mathis, S.; Molenda-Żakowicz, J.; Pinsonneault, M.: Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants. Astronomy and Astrophysics 564, A27 (2014)
Fournier, D.; Gizon, L.; Hohage, T.; Birch, A.: Generalization of the noise model for time‐distance helioseismology. Astronomy and Astrophysics 567, A137 (2014)
Jiang, J.; Hathaway, D. H.; Cameron, R. H.; Solanki, S. K.; Gizon, L.; Upton, L.: Magnetic Flux Transport at the Solar Surface. Space Science Reviews 186, pp. 491 - 523 (2014)
Langfellner, J.; Gizon, L.; Birch, A. C.: Time-distance helioseismology: A new averaging scheme for measuring flow vorticity. Astronomy and Astrophysics 570, A90 (2014)
Papini, E.; Gizon, L.; Birch, A. C.: Propagating Linear Waves in Convectively Unstable Stellar Models: a Perturbative Approach. Solar Physics 289, pp. 1919 - 1929 (2014)
Roudier, T.; Švanda, M.; Rieutord, M.; Malherbe, J. M.; Burston, R.; Gizon, L.: Structure and evolution of solar supergranulation using SDO/HMI data. Astronomy and Astrophysics 567, A138 (2014)
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".