Shkuratov, Y. G.; Grynko, Y. S.: Light scattering by media composed of semitransparent particles of different shapes in ray optics approximation: consequences for spectroscopy, photometry, and polarimetry of planetary regoliths. Icarus 173 (1), pp. 16 - 28 (2005)
Grynko, Y.; Jockers, K.; Schwenn, R.: The phase curve of cometary dust: Observations of comet 96P/Machholz 1 at large phase angle with the SOHO LASCO C3 coronagraph. Astronomy and Astrophysics 427 (2), pp. 755 - 761 (2004)
Grynko, Y.; Shkuratov, Y.: Scattering matrix calculated in geometric optics approximation for semitransparent particles faceted with various shapes. Journal of Quantitative Spectroscopy & Radiative Transfer 78, pp. 319 - 340 (2003)
Grynko, Y.: Light scattering by cometary dust particles with sizes large compared to the wavelength of light. Dissertation, Georg-August-Universität Göttingen (2005)
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, ...