Wilhelm, K.; Cosmovici, C. B.; Delamere, W. A.; Huebner, W. F.; Keller, H. U.; Reitsema, H.; Schmidt, H. U.; Whipple, F. L.: A three-dimensional model of the nucleus of Comet Halley. In: ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet, pp. 367 - 369 (Eds. Battrick, B.; Rolfe, E. J.; Reinhard, R.). ESA Publ. Div., Noordwijk (1986)
Wilhelm, K.: Quantitative Spectroscopy of the Solar Atmosphere. Dynamic Sun: I. MHD Waves and Confined Transients in the Magnetised Atmosphere, Varanasi, India (2016)
Wilhelm, K.: Bhola N. Dwivedi - 25 Years of Cooperation with SUMER. Dynamic Sun: I. MHD Waves and Confined Transients in the Magnetised Atmosphere, Varanasi, India (2016)
Rao, Y. K.; Kayshap, P.; Srivastava, A. K.; Wilhelm, K.; Dwivedi, B. N.: Multi-line Spectroscopic Analyses of the Dynamical Cool Loops Using Interface Region Imaging Spectrometer (IRIS) Observations. IAU Symposia 340: Long-term datasets for the understanding of solar and stellar magnetic cycles, Jaipur, India (2018)
Wilhelm, K.; Marsch, E.; Dwivedi, B.; Feldman, U.: Observations of the Sun at vacuumu-ultravioletwavelengths form space. Part II: Results and interpretations. Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany (2007)
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, ...