Chilson, P. B.; Czechowsky, P.; Schmidt, G.: VHF aspect sensitivity measurements using frequency domain interferometry. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, p. 18 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Chilson, P. B.; Czechowsky, P.; Schmidt, G.: A comparison of ambipolar diffusion coefficients near the mesopause as determined by VHF radar and UV lidar observations. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 286 - 289 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Chilson, P. B.; Muschinski, A.; Schmidt, G.: Simultaneous observations of a jet stream passage using VHF FDI and a microbarometer. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 113 - 116 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Muschinski, A.; Chilson, P. B.; Schmidt, G.; Hollmann, R.: FDI measurements with the SOUSY VHF Radar: A comparison between the time series of layer altitudes and Doppler shifts. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 407 - 410 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Singer, W.; Keuer, D.; Hoffmann, P.; Czechowsky, P.; Schmidt, G.: The ALOMAR SOUSY radar: Technical design and further developments. In: Solar-Terrestrial Energy Program, Proc. 7th Workshop on Technical and Scientific Aspects of MST Radar, Hilton Head Island/USA 1995, pp. 473 - 476 (Ed. Edwards, B.). SCOSTEP Secret., Boulder (1996)
Singer, W.; Keuer, D.; Hoffmann, P.; Czechowsky, P.; Schmidt, G.: The ALOMAR-SOUSY Radar: Technical design and further developments. In: Proc. 12th ESA Symp. on Rocket and Balloon Programmes & Related Research, Lillehammer/Norway 1995, pp. 409 - 415. ESA Publ. Div., Noordwijk (1995)
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)
Czechowsky, P.; Inhester, B.; Klostermeyer, J.; Rüster, R.; Schmidt, G.: Simultaneous radar and lidar observations during the DYANA-campaign. In: Proc. 10th ESA Symposium on European Rocket and Balloon Programmes and Related Research, pp. 399 - 405. ESA Publ. Div., Noordwijk (1991)
Schmidt, G.; Rüster, R.; Czechowsky, P.: Complementary code and digital filtering for detection of weak VHF radar signals from the mesosphere. In: Handbook for MAP, p. 338. (1983)
Czechowsky, P.; Rüster, R.; Schmidt, G.: VHF-radar observations of structures and their dynamics in the stratosphere and mesosphere. Am. Met. Soc., pp. 588 - 592 (1980)
Schmidt, G.; Brekke, A.; Czechowsky, P.; Hall, C. M.; Widdel, H. U.: Spatial Extent and Persistance of Mesospheric Turbulent Layers. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1985)
Czechowsky, P.; Schmidt, G.; Rüster, R.: The mobile SOUSY-Doppler Radar - Technical design and first results. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1983)
Die ESA-Mission JUICE soll ab 2030 das Jupitersystem erkunden. Nach Vorbeiflügen an Europa und Callisto wird die Raumsonde erstmals in der Geschichte der Raumfahrt in eine Umlaufbahn um den Mond Ganymed einschwenken.
Das Submillimetre Wave Instrument (SWI) wird die Galileischen Monde, die Chemie, die Meteorologie und die Struktur der mittleren Jupiter-Atmosphäre, sowie atmosphärische und magnetosphärische Kopplungsprozesse untersuchen.
Mars Express ist eine ESA Mission zum Mars. Sie hat eine Nutzlast an Bord, die in der Lage ist, die bisher gründlichste Suche nach flüssigem Wasser, das unerlässlich ist für Leben wie wir es kennen, auf dem roten Planeten durchzuführen.
Ein Überblick über alle Arbeits- und Forschungsgruppen der Abteilung für Planetenwissenschaften: Atmosphären der Planeten, Inneres der Planeten, Kleine Körper und Kometen, Oberflächen der Planeten, Plasmaumgebung der Planeten.