Steinhagen, H.; Christoph, A.; Czechowsky, P.; Görsdorf, U.; Gube-Lenhardt, M.; Lippmann, J.; Neisser, J.; Rüster, R.; Schmidt, G.; Wergen, W.et al.; Yoe, J. G.: Field campaign for the comparison of SOUSY radar wind measurements with rawinsonde and model data. Annales Geophysicae 12 (8), pp. 746 - 764 (1994)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Spatial variability of the aspect sensitivity of VHF radar echoes in the troposphere and lower stratosphere during jet stream passages. Annales Geophysicae 12 (8), pp. 733 - 745 (1994)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Temporal and Spatial Variability of Aspect Sensitivity of VHF Radar Echoes in the Lower Atmosphere. Annales Geophysicae 12, pp. 733 - 745 (1993)
Yoe, J. G.; Rüster, R.: VHF Doppler Radar Opservations of Vertical Velocities in the Vicinity of the Jet Stream. Monthly Weather Rev. 120 (10), pp. 2378 - 2382 (1992)
Yoe, J. G.; Czechowsky, P.; Rüster, R.; Schmidt, G.: Spatial and temporal variability of the aspect sensitivity of VHF radar echoes in the troposphere and lower stratosphere during jet stream passages. In: Solar-Terrestrial Energy Program, Proc. 6th Workshop on Techhnical and Scientific Aspects of MST Radar, Chung-Li/Taiwan 1993, pp. 66 - 70 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1994)
Yoe, J. G.; Rüster, R.; Schmidt, G.: Measurement of momentum fluxes in the troposphere and stratosphere during jet sream passages using the SOUSY VHF. In: Proc. 5th Workshop on Technical and Scientific Aspects of MSt Radar,, Aberystwyth, United Kingdom 1991, pp. 150 - 155 (Ed. Edwards, B.). SCOSTEP, Secret., Boulder (1992)
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, ...