Chatzistergos, T.; Ermolli, I.; Solanki, S. K.; Krivova, N. A.: Exploiting four historical Ca II K spectroheliogram archives. Publications of the astronomical society of the pacific 504, pp. 227 - 231 (2016)
Ghosh, A.; Chatterjee, S.; Khan, A. R.; Tripathi, D.; Ramaprakash, A. N.; Banerjee, D.; Chordia, P.; Gandorfer, A. M.; Krivova, N.; Nandy, D.et al.; Rajarshi, C.; Solanki, S. K.; Sriram, S.: The Solar Ultraviolet Imaging Telescope onboard Aditya-L1. In: Proc. SPIE 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, Vol. 9905, 990503 (Eds. den Herder, J.-W. A.; Takahashi, T.; Bautz, M.). Edinburgh, United Kingdom (2016)
Norris, C. M.; Beeck, B.; Unruh, Y.; Solanki, S.; Yeo, K. L.; Krivova, N.: Modelling the Spectral Contrasts of Stellar Faculae. In: The 19th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (CS19), Uppsala, Sweden, 06-10 June 2016, Vol. CS19, 63 (Ed. Feiden, G. A.). (2016)
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)
Danilovic, S.; Solanki, S. K.; Livingston, W.; Krivova, N. A.; Vince, I.: Magnetic source of the solar cycle variation of the Mn I 539.4 nm line. In: Modern solar facilities-Advanced Solar Science, pp. 189 - 192 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen, Göttingen (2007)
Ermolli, I.; Tlatov, A.; Solanki, S. K.; Krivova, N. A.; Singh, J.: Solar Activity and Irradiance Studies with Ca II Spectroheliograms: Potential and Problems. In: The Physics of Chromospheric Plasmas, p. 533 (Eds. Heinzel, P.; Dorotovič, I.; Rutten, R. J.). ASP, San Francisco (2007)
Seleznyov, A. D.; Krivova, N. A.; Solanki, S. K.: Understanding solar variability as groundwork for planet transit detection. In: Stars as Suns: Activity, Evolution, and Planets, p. CD-815-CD-819 (Eds. Dupree, A. K.; Benz, A. O.). Cambridge Univ. Press (2004)
Krivova, N. A.; Solanki, S. K.: Solar total and spectral irradiance: Modelling and a possible impact on climate. In: Proceedings ISCS 2003 Symposium: ``Solar Variability as an Input to the Earth's Environment'', pp. 275 - 284 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2003)
Seleznyov, A. D.; Solanki, S. K.; Krivova, N. A.: On the origin of solar variability, with an application to the search for extrasolar planets. In: Proc. Workshop ``Toward other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets'', pp. 589 - 593 (Ed. Battrick, B.). ESA Publ. Div., Noordwijk (2003)
Solanki, S. K.; Krivova, N. A.: Cycles and cyclicities of the Sun. In: Proc. Workshop ``Interplay Between Periodic, Cyclic and Stochastic Variability in Selected Areas of the H-R Diagram, pp. 423 - 432 (Ed. Sterken, C.). (2003)
Solanki, S. K.; Seleznyov, A. D.; Krivova, N. A.: Solar irradiance fluctuations on short timescales. In: Proceedings ISCS 2003 Symposium: ``Solar Variability as an Input to the Earth's Environment'', pp. 285 - 288 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2003)
Krivova, N. A.: Dust in young solar systems. In: Dust in the Solar System and Other Planetary Systems, pp. 201 - 216 (Eds. Green; F., S.; others). Elsevier (2002)
Krivova, N. A.; Solanki, S. K.; Fligge, M.: How large is the Sun's total magnetic flux. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 461 - 464 (Ed. Sawaya-Lacoste, H.). ESA Publications Division, Noordwijk (2002)
Krivova, N. A.; Solanki S., K.; Fligge, M.: Total solar magnetic flux: dependence on spatial resolution of magnetograms. In: Proc. SOHO-11 Symposium `From Solar Min to Max: Half a Solar Cycle with SOHO', pp. 155 - 158 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (2002)
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)
Wu, C.-J.; Usoskin, G.; Krivova, N. A.; Kovaltsov, A. G.: Solar Irradiance Reconstruction over Holocene: A Consistent Multi-proxy Series. The many Sclaes of the Universe: Galaxies, their Suns, and their Planets. Annual Meeting of the German Astronomical Society, Göttingen (2018)
Wu, C.-J.; Usoskin, G.; Krivova, N. A.; Kovaltsov, A. G.: Solar Irradiance Reconstruction over Holocene: A Consistent Multi-proxy Series. Rocks & Stars II Conference, Göttingen (2018)
Wu, C.-J.; Usoskin, I.G.; Krivova, N. A.; Kovaltsov, G.A.: Solar Irradiance in the Holocene: A Consistent Multi-proxy Reconstruction. 1st Paleoclimate Modelling Intercomparison Project (PMIP4) conference
, Stockholm (2018)
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".