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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...