Jungclaus, J. H.; Bard, E.; Baroni, M.; Braconnot, P.; Cao, J.; Chini, L. P.; Egorova, T.; Evans, M.; González-Rouco, J. F.; Goosse, H.et al.; Hurtt, G. C.; Joos, F.; Kaplan, J. O.; Khodri, M.; Goldewijk, K. K.; Krivova, N. A.; LeGrande, A. N.; Lorenz, S. J.; Luterbacher, J.; Man, W.; Maycock, A. C.; Meinshausen, M.; Moberg, A.; Muscheler, R.; Nehrbass-Ahles, C.; Otto-Bliesner, B. I.; Phipps, S. J.; Pongratz, J.; Rozanov, E.; Schmidt, G. A.; Schmidt, H.; Schmutz, W.; Schurer, A.; Shapiro, A.; Sigl, M.; Smerdon, J. E.; Solanki, S. K.; Timmreck, C.; Toohey, M.; Usoskin, I. G.; Wagner, S.; Wu, C.-J.; Yeo, K. L.; Zanchettin, D.; Zhang, Q.; Zorita, E.: The PMIP4 contribution to CMIP6 – Part 3: The last millennium, scientific objective, and experimental design for the PMIP4 past1000 simulations. Geoscientific Model Development 10, pp. 4005 - 4033 (2017)
Tagirov, R. V.; Shapiro, A. I.; Schmutz, W.: NESSY: NLTE spectral synthesis code for solar and stellar atmospheres. Astronomy and Astrophysics 603, A27 (2017)
Thuillier, G.; Zhu, P.; Shapiro, A. I.; Sofia, S.; Tagirov, R.; van Ruymbeke, M.; Perrin, J.-M.; Sukhodolov, T.; Schmutz, W.: Solar disc radius determined from observations made during eclipses with bolometric and photometric instruments on board the PICARD satellite. Astronomy and Astrophysics 603, A28 (2017)
Shapiro, A. I.; Solanki, S. K.; Krivova, N. A.; Tagirov, R. V.; Schmutz, W. K.: The role of the Fraunhofer lines in solar brightness variability. Astronomy and Astrophysics 581, A116 (2015)
Thuillier, G.; Harder, J. W.; Shapiro, A.; Woods, T. N.; Perrin, J.-M.; Snow, M.; Sukhodolov, T.; Schmutz, W.: The Infrared Solar Spectrum Measured by the SOLSPEC Spectrometer Onboard the International Space Station. Solar Physics 290, pp. 1581 - 1600 (2015)
Shapiro, A.; Peter, H.; Solanki, S. K.: The Sun's Atmosphere. In: The Sun as a Guide to Stellar Physics, pp. 59 - 85 (Eds. Engvold, O.; Vial, .-C.; Skumanich, A.). Elsevier, Amsterdam (2019)
Kopp, G.; Shapiro, A.: FM9 - Solar Irradiance: Physics-Based Advances. In: Proceedings of the International Astronomical Union, Vol. 14, pp. 331 - 332. (2020)
Gröbner, J.; Kazadzis, S.; Kouremeti, N.; Doppler, L.; Tagirov, R.; Shapiro, A.: Spectral solar variations during the eclipse of March 20th, 2015 at two European sites. In: AIP Conference Proceedings, Vol. 1810, 080008. American Institute of Physics (2017)
Yeo, K. L.; Shapiro, A. I.; Krivova, N. A.; Solanki, S. K.: Modelling solar and stellar brightness variabilities. In: Coimbra Solar Physics Meeting: Ground-based Solar Observations in the Space Instrumentation Era, Vol. 504, pp. 273 - 286. (2016)
Cessateur, G.; Werner Schmutz, W.; Shapiro, A.: The solar irradiance: observations and modelling. European Geosciences Union General Assembly, Vienna, Austria (2015)
Shapiro, A.; Solanki, S.; Krivova, N.: Solar brightness variability in the stellar context. Second SOLARNET Meeting on "Solar and stellar magnetic activity, Palermo, Italy (2015)
Shapiro, A.; Solanki, S.; Krivova, N.: Brightness variations of the Sun and Sun-like stars. Solar-Stellar Connection Workshop, Sandbjerg, Denmark (2015)
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".