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)
Mathew, S. K.; Martínez Pillet, V.; Solanki, S. K.; Krivova, N. A.: Properties of sunspots in cycle 23. I. Dependence of brightness on sunspot size and cycle phase. Astronomy and Astrophysics 465, pp. 291 - 304 (2007)
Mathew, S. K.; Lagg, A.; Solanki, S. K.; Collados, M.; Berdyugina, S.; Krupp, N.; Woch, J.; Frutiger, C.: Inversion of 1.5 μm spectral data of a sunspot. In: Proc. ``Probing the Sun with High Resolution'' (Eds. Venkatkrishnan, S.; Tripathy, S. C.; Venkatkrishnan, P. V.). Alpha Science, Pangbourne (2002)
Mathew, S. K.; Solanki, S. K.; the VIM Team: A Fabry-Perot Etalon Filter System for a Visible Light Imager and Magnetograph on-board Solar Orbiter. In: Proc. ``Probing the Sun with High Resolution'' (Eds. Tripathy, S. V. S. C.; Venkatkrishnan, P. V.). Alpha Science, Pangbourne (2002)
Mathew, S. K.; Solanki, S. K.; Lagg, A.; Collados, M.; Berdyugina, S.; Frutiger, C.; Krupp, N.; Woch, J.: Thermal-magnetic relation of a sunspot from the inversion of IR spectral data. In: 1st Potsdam Thinkshop on Sunspots and Starspots Poster Proceedings, pp. 117 - 118 (Eds. Strassmeier, K. G.; Washuettl, A.). Brandenburgische Universitätsdruckerei, Golm (2002)
Mathew, S. K.; Solanki, S. K.; Lagg, A.; Collados, M.; Berdyugina, S.; Frutiger, C.; Krupp, N.; Woch, J.: Thermal-magnetic relation of a sunspot as inferred from inversion of 1.5 μm spectral data. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 501 - 504 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
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, ...