Stucki, K.; Solanki, S. K.; Pike, C. D.; Schühle, U.; Rüedi, I.; Pauluhn, A.; Brkovic, A.: Properties of ultraviolet lines observed with Coronal Diagnostic Spectrometer (CDS/SOHO) in coronal holes and the quiet Sun. Astronomy and Astrophysics 381, pp. 653 - 667 (2002)
Pauluhn, A.; Rüedi, I.; Solanki, S. K.; Lang, J.; Schühle, U.; Wilhelm, K.; Thompson, W. T.; Hollandt, J.; Huber, M. C. E.: Intercalibration of SUMER and CDS on SOHO. II. SUMER A and B detectors and CDS NIS. Applied Optics 40, pp. 6292 - 6300 (2001)
Pauluhn, A.; Solanki, S. K.; Schühle, U.; Wilhelm, K.; Lang, J.; Thompson, W. T.; Rüedi, I.; Hollandt, J.; Huber, M. C. E.: Comparison of quiet-Sun radiances measured by CDS and SUMER on SOHO. Space Science Reviews 97, pp. 63 - 66 (2001)
Schühle, U.; Pauluhn, A.; Hollandt, J.; Lemaire, P.; Wilhelm, K.: Radiance variations of vacuum-ultraviolet emission lines of the quiet Sun observed with SUMER on SOHO. Physics and Chemistry of the Earth C, 25 (C), pp. 429 - 432 (2000)
Schühle, U.; Wilhelm, K.; Hollandt, J.; Lemaire, P.; Pauluhn, A.: Radiance variations of the quiet Sun at far-ultraviolet wavelengths. Astronomy and Astrophysics 354, pp. L71 - L74 (2000)
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Pauluhn, A.; Solanki, S. K.: Dependence of UV radiance of the quiet Sun on the solar cycle. In: Proc. SOHO 11 Symposium, ``From Solar Min to Max: Half a Solar Cycle with SOHO'', pp. 227 - 230 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
Pauluhn, A.; Solanki, S. K.: Surface magnetic fields and UV radiance of the quiet Sun. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 521 - 524 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Pauluhn, A.; Schühle, U.; Solanki, S. K.; Rüedi, I.; Lang, J.; Pike, C. D.; Thompson, W. T.; Huber, M. C. E.: Radiance of solar spectral lines observed with CDS and SUMER on SOHO. In: Cool Stars, Stellar Systems and the Sun XI, pp. CD - 721 (Eds. López, G.; J., R.; Rebolo; R.; Osorio, Z. et al.). Astronomical Society of the Pacific, San Francisco (2001)
Pauluhn, A.; Solanki, S. K.; Rüedi, I.; Landi, E.; Schühle, U.: Statistical features of the quiet Sun in EUV. In: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from SOHO and Other Space Missions, pp. 416 - 418 (Eds. Brekke, P.; Fleck, B.; Gurman, J. B.). (2001)
Schühle, U.; Hollandt, J.; Pauluhn, A.; Wilhelm, K.: Mid-term radiance variation of far-ultraviolet emission lines from quiet-Sun areas. In: Proc. 1st Solar & Space Weather Euroconference, `The Solar Cycle and Terrestrial Climate', Santa Cruz de Tenerife, Tenerife, Spain, 25-29 September 2000, pp. 427 - 430. ESA Publ. Div., Noordwijk (2000)
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".