Markiewicz, W. J.; Keller, H. U.; Thomas, N.; Titov, D.; Forget, F.: Optical properties of the Martian aerosols in the visible spectral range. Advances in Space Research 29 (2), pp. 175 - 181 (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)
Skorov, Y. V.; Kömle, N. I.; Keller, H. U.; Kargl, G.; Markiewicz, W. J.: A model of heat and mass transfer in a porous cometary nucleus based on a kinetic treatment of mass flow. Icarus 153 (1), pp. 180 - 196 (2001)
Skorov, Y. V.; Markiewicz, W. J.; Basilevsky, A. T.; Keller, H. U.: Stability of water ice under a porous nonvolatile layer: implications to the south polar layered deposits of Mars. Planetary and Space Science 49 (1), pp. 59 - 63 (2001)
Smith, P. H.; Reynolds, R.; Weinberg, J.; Friedmann, T.; Lemmon, M. T.; Tanner, R.; Reid, R. J.; Marcialis, R. L.; Bos, B. J.; Oquest, C.et al.; Keller, H. U.; Markiewicz, W. J.; Kramm, R.; Gliem, F.; Rueffer, P.: The MVACS surface stereo imager on Mars Polar Lander. Journal Geophysical Research 106, pp. 17589 - 17608 (2001)
Huebner, W. F.; Markiewicz, W. J.: The temperature and bulk flow speed of a gas effusing or evaporating from a surface into a void after reestablishment of collisional equilibrium. Icarus 148 (2), pp. 594 - 596 (2000)
Thomas, N.; Jorda, L.; Markiewicz, W. J.: Effect of diffuse sky brightness on the spectrophotometry of rough Martian surfaces. Journal Geophysical Research 105 (E11), pp. 26739 - 26744 (2000)
Titov, D. V.; Markiewicz, W. J.; Thomas, N.; Keller, H. U.; Tomasko, M. G.; Lemmon, M.; Smith, P. H.: On the optical studies of the atmospheric water vapour from the surface of Mars. Planetary and Space Science 48 (15), pp. 1423 - 1427 (2000)
Basilevsky, A. T.; Markiewicz, W. J.; Thomas, N.; Keller, H. U.: Morphologies of rocks within and near the Rock Garden at the Mars Pathfinder landing site. Journal Geophysical Research 104, pp. 8617 - 8636 (1999)
Basilevsky, A. T.; Markiewicz, W. J.; Thomas, N.; Keller, H. U.: Morphology of the APXS analyzed Rocks at the Pathfinder site. Solar System Research 33, pp. 170 - 186 (1999)
Basilevsky, A. T.; Markiewicz, W. J.; Thomas, N.; Keller, H. U.: Surface material and landscape characteristics at the Mars Polar Lander Site: A consideration and prediction. Solar System Res. 33, p. 439 (1999)
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.; Sablotny, R. M.; Keller, H. U.; Thomas, N.: Optical properties of the Martian aerosols as derived from Imager for Mars Pathfinder midday sky brightness data. Journal Geophysical Research 104, pp. 9009 - 9017 (1999)
Markiewicz, W. J.; Sablotny, R. M.; Keller, H. U.; Thomas, N.; Titov, D. V.; Smith, P. H.: Optical properties of the Martian aerosols as derived from Imager for Mars Pathfinder midday sky brightness data. Journal Geophysical Research 104, pp. 9009 - 9017 (1999)
Thomas, N.; Markiewicz, W. J.; Sablotny, R. M.; Wuttke, M. W.; Keller, H. U.; Johnson, J. R.; Reid, R. J.; Smith, P. H.: The color of the Martian sky and its influence on the illumination of the Martian surface. Journal Geophysical Research 104, pp. 8795 - 8808 (1999)
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, ...