Bockelée-Morvan, D.; Biver, N.; Schambeau, C. A.; Crovisier, J.; Opitom, C.; de Val Borro, M.; Lellouch, E.; Hartogh, P.; Vandenbussche, B.; Jehin, E.et al.; Kidger, M.; Küppers, M.; Lis, D. C.; Moreno, R.; Szutowicz, S.; Zakharov, V.: Water, hydrogen cyanide, carbon monoxide, and dust production from distant comet 29P/Schwassmann-Wachmann 1. Astronomy and Astrophysics 664, p. A95 (2022)
Mathew, S. K.; Zakharov, V.; Solanki, S. K.: Stray light correction and contrast analysis of Hinode broad-band images. Astronomy and Astrophysics 501, pp. L19 - L22 (2009)
Zakharov, V.; Gandorfer, A.; Solanki, S. K.; Löfdahl, A.: Erratum in ``A comparative study of the contrast of solar magnetic elements in CN and CH'' (vol 437, pg L43, 2005). Astronomy and Astrophysics 461 (2), p. 695 - 695 (2007)
Zakharov, V.; Gandorfer, A.; Solanki, S. K.; Löfdahl, M.: A comparative study of the contrast of solar magnetic elements in CN and CH. Astronomy and Astrophysics 437, pp. L43 - L46 (2005)
Cameron, R.; Vögler, A.; Schüssler, M.; Zakharov, V.: Simulations of solar pores. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Eds. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
Zakharov, V.: Diagnostic of the solar photosphere with high spatial resolution using CH, CN and continuum spectral bands. Dissertation, Georg-August-Universität Göttingen (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".