Titov, D. V.; Markiewicz, W. J.; Thomas, N.; Keller, H. U.; Sablotny, R. M.; Tomasko, M. G.; Lemmon, M. T.; Smith, P. H.: Measurements of the atmospheric water vapor on Mars by the Imager for Mars Pathfinder. Journal Geophysical Research 104, pp. 9019 - 9026 (1999)
Markiewicz, W. J.; Skorov, Y.; Keller, H. U.: The shape of a sublimating ice surface at the bottom of a non-volatie cylinder: Monte Carlo simulations and 2-D analysis. Advances in Space Research 21, pp. 1599 - 1602 (1998)
Markiewicz, W. J.; Skorov, Y. V.; Keller, H. U.; Kömle, N. I.: Evolution of ice surfaces within porous near-surface layers on cometary nuclei. Planetary and Space Science 46, pp. 357 - 366 (1998)
Petrova, E. V.; Markiewicz, W. J.: Optical properties of morning-ice-haze and cloud particles and the photometry of Mars. Solar System Research 32 (6), pp. 469 - 479 (1998)
Eggers, S.; Keller, H. U.; Kroupa, P.; Markiewicz, W. J.: Origin and dynamics of comets and star formation. Planetary and Space Science 45, pp. 1099 - 1104 (1997)
Petrova, E. V.; Markiewicz, W. J.: Light scattering by nonspherical particles: A modification of the statistical model and application to the Martian aerosol. Solar System Res. 31, pp. 369 - 376 (1997)
Thomas, N.; Keller, H. U.; Markiewicz, W. J.; Smith, P. H.: Observations of Martian aerosols with the Imager for Mars Pathfinder. Advances in Space Research 19, pp. 1271 - 1276 (1997)
Wuttke, M. W.; Keller, H. U.; Markiewicz, W. J.; Petrova, E.; Richter, K.; Thomas, N.: Properties of the Mars atmosphere: A revised analysis of Phobos/KRFM data. Planetary and Space Science 45, pp. 281 - 288 (1997)
Petrova, E.; Keller, H. U.; Markiewicz, W. J.; Thomas, N.; Wuttke, M. W.: Ice, hazes, and clouds in the Martian atmosphere as derived from the PHOBOS/KRFM data. Planetary and Space Science 44, pp. 1163 - 1176 (1996)
Keller, H. U.; Knollenberg, J.; Markiewicz, W. J.: Collimation of cometary dust jets and filaments. Planetary and Space Science 42, pp. 367 - 382 (1994)
Keller, H. U.; Blum, J.; Donn, B.; Goresy, A. E.; Fechtig, H.; Feuerbacher, B. P.; Grün, E.; Ip, W. -. H.; Kochan, H.; Mann, I.et al.; Markiewicz, W. J.; Metzler, K.; Morfill, G. E.; Ratke, L.; Rott, M.; Schwehm, G.; Weidenschilling, S. J.: CODAG - Dust agglomeration experiment in micro-gravity. Advances in Space Research 13 (7), pp. 73 - 76 (1993)
Kochan, H.; Markiewicz, W. J.; Keller, H. U.: KOSI: Gas drag derived from ice/dust-particle trajectories. Geophysical Research Letters 18 (2), pp. 273 - 276 (1991)
Markiewicz, W. J.; Mizuno, H.; Völk, H. J.: Turbulende induced relative velocity between two grains. Astronomy and Astrophysics 242, pp. 286 - 289 (1991)
Markiewicz, W. J.; Drury, L. O. C.; Völk, H. J.: Diffuse particle acceleration in spherically symmetric shock waves: supernova remnant origin of cosmic rays. Astronomy and Astrophysics 236, pp. 487 - 502 (1990)
Drury, L. O. C.; Markiewicz, W. J.; Völk, H. J.: Simplified models for the evolution of supernova remnants including particle acceleration. Astronomy and Astrophysics 225, pp. 179 - 191 (1989)
Mizuno, H.; Markiewicz, W. J.; Völk, H. J.: Grain growth in turbulent protoplanetary accretion disks. Astronomy and Astrophysics 195, pp. 183 - 192 (1988)
Markiewicz, W. J.; Aldridge, K.: Dielectrophoretic, thermal instability in a spherical shell of fluid. Geophys. Astrophys. Fluid Dynamics 21, pp. 225 - 236 (1982)
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, ...