Dikarev, V.; Preuß, O.; Solanki, S.; Krüger, H.; Krivov, A.: The Local Dust Foregrounds in the Microwave Sky. I. Thermal Emission Spectra. Astrophysical Journal 705, pp. 670 - 682 (2009)
Dikarev, V.; Preuss, O.; Solanki, S. K.; Krüger, H.; Krivov, A.: Understanding the WMAP results: low-order multipoles and dust in the vicinity of the solar system. Earth, Moon and Planets 102, pp. 555 - 561 (2007)
Preuss, O.; Solanki, S. K.; Haugan, M. P.; Jordan, S.: Gravity-induced birefringence within the framework of Poincaré gauge theory. Physical Review D 72, p. 042001 (2005)
Preuss, O.; Haugan, M. P.; Solanki, S. K.; Jordan, S.: An astronomical search for evidence of new physics: Limits on gravity-induced birefringence from the magnetic white dwarf RE J0317-853. Physical Review D 70 (6), 067101 (2004)
Preuss, O.; Schüssler, M.; Holzwarth, V.; Solanki, S. K.: Distribution of magnetically confined circumstellar matter in oblique rotators. Astronomy and Astrophysics 417, pp. 987 - 992 (2004)
Solanki, S. K.; Preuss, O.; Haugan, M.; Gandorfer, A.; Povel, H. P.; Steiner, P.; Stucki, K.; Bernasconi, P. N.; Soltau, D.: Solar constraints on new couplings between electromagnetism and gravity. Physical Review D 69, 062001 (2004)
Neiner, C.; Geers, V. C.; Henrichs, H. F.; Floquet, M.; Frémat, Y. H.; Hubert, A. M.; Preuss, O.; Wiersema, K.: Discovery of a magnetic field in the Slowly Pulsating B star ζ Cassiopeiae. Astronomy and Astrophysics 406 (3), pp. 1019 - 1031 (2003)
Neiner, C.; Henrichs, H. F.; Floquet, M.; Fremat, Y.; Preuss, O.; Hubert, A. M.; Geers, V. C.; Tijani, A. H.; Nichols, J. S.; Jankov, S.: Rotation, pulsations and magnetic field in V 2052 Ophiuchi: A new He-strong star. Astronomy and Astrophysics 411 (3), pp. 565 - 579 (2003)
Neiner, C.; Hubert, A. M.; Frémat, Y.; Floquet, M.; Jankov, S.; Preuss, O.; Henrichs, H. F.; Zorec, J.: Rotation and magnetic field in the Be star ω Orionis. Astronomy and Astrophysics 409 (1), pp. 275 - 286 (2003)
Laemmerzahl, C.; Preuss, O.; Dittus, H.: Is the physics within the Solar system really understood? In: Lasers, Clocks, and Drag-Free: Technologies for Future Exploration in Space and Tests of Gravity (Ed. Laemmerzahl, C.). (2006)
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".