Solanki, S. K.; Régulo, C.; Fligge, M.; Kosovichev, A. G.: Noise reduction in helioseismic power spectra by non-orthogonal wavelets. Astronomy and Astrophysics 379, pp. 1039 - 1044 (2001)
Berdyugina, S. V.; Frutiger, C.; Solanki, S. K.; Livingston, W.: Successful spectral synthesis of Zeeman-split molecular bands in sunspot spectra. Astronomy and Astrophysics 364, pp. L101 - L104 (2000)
Brkovic, A.; Rüedi, I.; Solanki, S. K.; Fludra, A.; Harrison, R. A.; Huber, M. C. E.; Stenflo, J. O.; Stucki, K.: EUV brightness variations in the quiet Sun. Astronomy and Astrophysics 353, pp. 1083 - 1093 (2000)
Fligge, M.; Solanki, S. K.: Properties of flux tubes and the relation with solar irradiance variability. J. Astrophys. Astron. 21, pp. 275 - 282 (2000)
Fligge, M.; Solanki, S. K.; Unruh, Y.: Modelling irradiance variations from the surface distribution of the solar magnetic field. Astronomy and Astrophysics 353, pp. 380 - 388 (2000)
Frutiger, C.; Solanki, S. K.; Fligge, M.; Bruls, J. H. M. J.: Properties of the solar granulation obtained from the inversion of low spatial resolution spectra. Astronomy and Astrophysics 358, pp. 1109 - 1121 (2000)
Gadun, A. S.; Hanslmeier, A.; Pikalov, K. N.; Ploner, S. R. O.; Puschmann, K. G.; Solanki, S. K.: Size-dependent properties of simulated 2-D solar granulation. Astronomy and Astrophysics, Suppl. Ser. 146, pp. 267 - 291 (2000)
Keppens, R.; Solanki, S. K.; Charbonnel, C.: Spin and orbital angular momentum exchange in binary star systems. II. Ascending the giant branch: a new path to FK Comae stars. Astronomy and Astrophysics 359, pp. 552 - 562 (2000)
Keppens, R.; Solanki, S. K.; Charbonnel, C.: Spin and orbital angular momentum exchange in binary star systems. II. Ascending the giant branch: a new path to FK Comae stars. Astronomy and Astrophysics 359, pp. 552 - 562 (2000)
Moreno-Insertis, F.; Solanki, S. K.: Distribution of magnetic flux on the solar surface and low-degree p-modes. Mon. Not. Roy. Astron. Soc 313, pp. 411 - 422 (2000)
Solanki, S. K.; Fligge, M.; Pulkkinen, P.; Hoyng, P.: Cyclic evolution of sunspots: Gleaning new results from old data. J. Astrophys. Astron. 21, pp. 163 - 165 (2000)
Solanki, S. K.; Schüssler, M.; Fligge, M.: Evolution of the Sun's large-scale magnetic field since the Maunder minimum. Nature 408, pp. 445 - 447 (2000)
Stucki, K.; Solanki, S. K.; Schühle, U.; Rüedi, I.: On the relationship between shift and intensity of ultraviolet lines in coronal holes and the quiet Sun. Astronomy and Astrophysics 362, pp. L49 - L52 (2000)
Stucki, K.; Solanki, S. K.; Schühle, U.; Rüedi, I.; Wilhelm, K.; Stenflo, J. O.; Brkovic, A.; Huber, M. C. E.: Comparison of far-ultraviolet emission lines formed in coronal holes and the quiet Sun. Astronomy and Astrophysics 363, pp. 1145 - 1154 (2000)
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.