Unruh, Y. C.; Knaack, R.; Fligge, M.; Solanki, S. K.: Are the Sun's brightness variations really tamer than those of other comparable solar-type stars? In: Cool Stars, Stellar Systems and the Sun XI, pp. CD - 748 (Eds. López, G.; J., R.; Rebolo; R.; Osorio, Z. et al.). Astronomical Society of the Pacific, San Francisco (2001)
Fligge, M.; Solanki, S. K.; Meunier, N.; Unruh, Y. C.: Solar surface magnetism and the increase of solar irradiance between activity minimum and maximum. In: Proc. 1st Solar & Space Weather Euroconference ``The Solar Cycle and Terrestrial Climate'', Santa Cruz de Tenerife, Spain, pp. 117 - 121 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2000)
Knaack, R.; Fligge, M.; Solanki, S. K.; Unruh, Y. C.: The influence of an inclined rotation axis on solar irradiance variations. In: Proc. Workshop on ``The Sun and Sun-like Stars'', pp. 45 - 52 (Eds. Jankovics, I.; Kovács, J.; Vincze, I. J.). Gothard Astrophysical Observatory, Szombathely, Hungary (2000)
Ortiz, A.; Solanki, S. K.; Fligge, M.; Domingo, V.; Sanahuja, B.: On the contrast of faculae and small magnetic features. In: Proc. 1st Solar & Space Weather Euroconference ``The Solar Cycle and Terrestrial Climate'', Santa Cruz de Tenerife, Spain, pp. 399 - 402 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2000)
Solanki, S. K.; Fligge, M.: Long-term changes in solar irradiance. In: Proc. 1st Solar & Space Weather Euroconference ``The Solar Cycle and Terrestrial Climate'', Santa Cruz de Tenerife, Spain, pp. 51 - 60 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2000)
Brkovic, A.; Rüedi, I.; Solanki, S. K.: Characteristics of blinkers observed with CDS. In: Proc. 8th SOHO Workshop ``Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona'', Paris, France, 22-25 June 1999, pp. 191 - 195 (Eds. Vial, J.-C.; Kaldeich-Schürmann, B.). ESA Publ. Div., Noordwijk (1999)
Landini, M.; Brkovic, A.; Landi, E.; Rüedi, I.; Solanki, S. K.: Loop models from SOHO observations. In: Proc. 8th SOHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona', Paris, France, 22-25 June 1999, pp. 423 - 428 (Eds. Vial, J.-C.; Kaldeich-Schürmann, B.). ESA Publ. Div., Noordwijk (1999)
Solanki, S. K.: Magnetic field structuring. In: Proc. 8th SOHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona', Paris, France, 22-25 June 1999, pp. 25 - 34 (Eds. Vial, J.-C.; Kaldeich-Schürmann, B.). ESA Publ. Div., Noordwijk (1999)
Stucki, K.; Solanki, S. K.; Rüedi, I.; Schühle, U.: Relationship between line shift and intensity inside coronal holes. In: Proc. 8th SOHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona', Paris, France, 22-25 June 1999, pp. 633 - 637 (Eds. Vial, J.-C.; Kaldeich-Schürmann, B.). ESA Publ. Div., Noordwijk (1999)
Horbury, T. S.; Auchere, F.; Antonucci, E.; Berghmans, D.; Bruno, R.; Carlsson, M.; del Toro Iniesta, J. C.; Fludra, A.; Harra, L.; Hassler, D.et al.; Heinzel, P.; Howard, R. A.; Krucker, S.; Livi, S. A.; Long, D.; Louarn, P.; Maksimovic, M.; Mueller, D.; Owen, C. J.; Peter, H.; Rochus, P. L.; Rodriguez-Pacheco, J.; Romoli, M.; Schühle, U.; Solanki, S. K.; Teriaca, L.; Wimmer-Schweingruber, R. F.; Zouganelis, Y.; Laker, R.: Solar Orbiter: connecting remote sensing and in situ measurements. AGU Fall Meeting, Online (2020)
Löptien, B.; Lagg, A.; van Noort, M.; Solanki, S. K.: Relating the magnetic field strength with the umbra-penumbra boundary in sunspots. SolarPolarization Workshop 9, Göttingen, Germany (2019)
Usoskin, I.; Wu, C.-J.; Krivova, N. A.; Solanki, S. K.; Kovaltsov, G.; Baroni, M.; Bard, E.: Cosmic-ray variability on the multi-millennial time scale: A new multi-proxy reconstruction. 36th International Cosmic Ray Conference (ICRC2019), Madison, WI, USA (2019)
Yeo, K. L.; Krivova, N. A.; Solanki, S. K.: Solar radiative forcing. IAPSO-IAMAS-IAGA Joint Assembly. Good Hope for Earth Sciences - IAPSO-IAMAS-IAGA Joint Assembly 2017, Cape Town, South Africa (2018)
Albert, K.; Hirzberger, J.; Gandorfer, A.; Woch, J.; Solanki, S. K.; Michalik, H.: Autonomous data reduction for the space-borne spectropolarimeter PHI. Annual meeting of the German Astrophysical Society 2017 - The many Scales of the Universe: Galaxies, their Suns, and their Planets, Göttingen, Germany (2017)
Albert, K.; Hirzberger, J.; Gandorfer, A.; Woch, J.; Solanki, S. K.; Michalik, H.: Autonomous flat field acquisition and correction techniques for the space-borne spectropolarimeter PHI. Rocks and Stars II, Göttingen, Germany (2017)
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".