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)
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".