Klostermeyer, J.: Comment on ``Neutral air turbulence and temperatures in the vicinity of polar mesosphere summer echoes'' by F.-J. Lübken, M. Rapp, and P. Hoffmann. Journal Geophysical Research 108 (D11), 4330 (2003)
Klostermeyer, J.: Polar mesospheric clouds at the South Pole: Simulations and implications for the mesopause region. Mem. British Astronom. Ass. 45, pp. 9.1 - 9.6 (2002)
Klostermeyer, J.: Effect of tidal variability on the mean diurnal variation of noctilucent clouds. Journal Geophysical Research 106, pp. 9749 - 9755 (2001)
Klostermeyer, J.: A simple model of the ice particle size distribution in noctilucent clouds. Journal Geophysical Research 103 (D22), pp. 28743 - 28752 (1998)
Klostermeyer, J.: The effect of ice particles on Thomson scattering from the polar summer mesopause region. Geophysical Research Letters 21, pp. 2721 - 2724 (1994)
Klostermeyer, J.: The formation of layered structures by parametric instability of finite-amplitude gravity waves. Advances in Space Research 12 (10), pp. (10) 203 - (10) 206 (1992)
Yi, F.; Klostermeyer, J.; Rüster, R.: VHF radar observation of gravity wave critical layers in the mid-latitude summer mesopause region. Geophysical Research Letters 18, pp. 697 - 700 (1991)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
For PhD students whose project is already funded and who are applying for admission to the IMPRS, or for applicants who want to bring their own funding and their own project idea to the IMPRS.
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.
The Solar Lower Atmosphere and Magnetism (SLAM) group covers many exciting subjects in solar physics, focussing on the development and testing of highly novel solar instrumentation, reduction and analysis of highest quality solar observations, or improving and developing advanced techniques for the analysis of solar observations.