Kossacki, K. J.; Szutowicz, S.: Comet 67P/Churyumov-Gerasimenko: Modeling of orientation and structure. Planetary and Space Science 54 (1), pp. 15 - 27 (2006)
Kossacki, K. J.; Markiewicz, W. J.; Smith, M. D.: Surface temperature of Martian regolith with polygonal features: influence of the subsurface water ice. Planetary and Space Science 51, pp. 569 - 580 (2003)
Kossacki, K. J.; Markiewicz, W. J.: Martian seasonal CO2 ice in polygonal troughs in southern polar region: role of the distribution of subsurface H2O Ice. Icarus 160, pp. 73 - 85 (2002)
Kossacki, K. J.; Markiewicz, W. J.; Keller, H. U.: Effect of surface roughness on ice distribution in the south subpolar region of Mars. Planetary and Space Science 49, pp. 437 - 445 (2001)
Kossacki, K. J.; Markiewicz, W. J.; Skorov, Y.; Kömle, N. I.: Sublimation coefficient of water ice under simulated cometary-like conditions. Planetary and Space Science 47, pp. 1521 - 1530 (1999)
Markiewicz, W. J.; Kossacki, K. J.; Keller, H. U.: Effect of surface roughness on ice distribution in the south subpolar region of Mars. In: The Second International Conference on Mars Polar Science and Exploration, LPI Contribution No. 1057, pp. 127 - 128 (Eds. Björnsson, H.; Clifford, S.; Paige, D.; Thorsteinsson, T.). Lunar and Planetary Institute (2000)
Markiewicz, W. J.; Kossacki, K. J.; Keller, H. U.: Smale scale trench in the Martian soil: Conditions for condensation of atmospheric volatiles at the Mars Polar Lander site. In: First International Conference on Mars Polar Science and Exploration, pp. 25 - 27 (Eds. Clifford, S.; Fisher, D.; Rice, J.). Lunar and Planetary Institute, Houston, TX (1998)
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, ...