D. Keuer
Leibniz Association
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Featured researches published by D. Keuer.
Journal of Atmospheric and Solar-Terrestrial Physics | 2002
Peter Hoffmann; W. Singer; D. Keuer
Abstract Continuous wind observations allow detailed investigations of the upper mesosphere circulation in winter and its coupling with the lower atmosphere. During winter the mesospheric/lower thermospheric wind field is characterized by a strong variability. Causes of this behaviour are planetary wave activity and related stratospheric warming events. Reversals of the dominating eastward directed mean zonal winds in winter to summerly westward directed winds are often observed in connection with stratospheric warmings. In particular, the amplitude and duration of these wind reversals are closely related to disturbances of the dynamical regime of the upper stratosphere. The occurrence of long-period wind oscillations and wind reversals in the mesosphere and lower thermosphere in relation to planetary wave activity and circulation disturbances in the stratosphere has been studied for 12 winters covering the years 1989–2000 on the basis of MF radar wind observations at Juliusruh (55°N, since 1989) and Andenes (69°N, since 1998). Mesospheric wind oscillations with long-periods between 10 and 18 days are observed during the presence of enhanced planetary wave activity in the stratosphere and are combined with a reversal of the meridional temperature gradient of the stratosphere or with upper stratospheric warmings.
Journal of Atmospheric and Solar-Terrestrial Physics | 2001
M. Zecha; J. Röttger; W. Singer; Peter Hoffmann; D. Keuer
Abstract Observations of polar mesosphere summer echoes (PMSE) were performed with the ALOMAR SOUSY VHF radar in the Doppler beam swinging (DBS) and the spaced antenna (SA) mode. This radar is located in polar regions at 69°N, 16°E in Andenes, Norway. After a summary of the basic features of PMSE and the system lay-out, we will come to the analysis of PMSE irregularity structures. Differences of the signal power observed with the DBS and the smaller SA antenna configuration point to a dominance of a scattering process of PMSE irregularities rather than to specular reflection. The SA method yields a more pronounced aspect sensitivity than the DBS method which points towards fairly anisotropic PMSE irregularities in the smaller volume sensed by the SA set-up. These anisotropic irregularity layers are frequently inclined towards the horizontal by a few degrees. There are wave and instability events which change the layer structure, their inclination and also the velocity components. When the layer inclination is not horizontal, a leakage of the horizontal velocity into the vertical velocity is manifest. It is shown that this can be corrected by using the measured zenith and azimuth angles of signal arrival and by calculating the leakage of the horizontal velocity components. This procedure yields improved estimates of the velocity components in vertical direction. Finally, some thoughts how to explain such observations of highly anisotropic and inhomogeneous PMSE irregularity structures are summarized.
Geophysical Research Letters | 1999
Christine Kremp; Uwe Berger; Peter Hoffmann; D. Keuer; Gerd R. Sonnemann
Mean MF-radar prevailing mesospheric wind data over Juliusruh (54.6°N, 13.4°E) for 8 years (1990–1997) have been compared with daytime averaged winds obtained from calculations using the Cologne global three-dimensional dynamic model of the middle atmosphere COMMA. The altitude-seasonal cross section shows that the model reflects the seasonal zonal wind pattern fairly well. The mesospheric summer and especially the winter winds are somewhat weaker in the observations. The model results are better reflected by measurements over Saskatoon (52°N, 107°W). The height of the observed maximum of the summer jet occurs more than 5 km above that one inferred from the model calculations. The long-term averages of the zonal winds will not be significantly changed if the periods with stratospheric warming events, which can lead to short term wind reversals at mesospheric heights during the winter months, are eliminated from the observational basis. The daytime averaged meridional wind component matches the observations over Juliusruh partly and agrees also with the published results obtained from measurements over Saskatoon.
Journal of Atmospheric and Solar-Terrestrial Physics | 1997
R. Schminder; D. Kürschner; Werner Singer; Peter Hoffmann; D. Keuer; J. Bremer
Abstract A joint analysis of LF and MF wind profiler data of Central Europe for the height range from 75 to 105 km for 7 years, obtained from daily measurements and overlapping in height and time, makes it possible to represent reliable height-time cross-sections for some wind field parameters. Interesting details are the great summer zonal prevailing wind gradient which reaches, on average, 3 m s−1 km−1 and a relatively height-invariable vertical wave length (about 50 km) of the semidiurnal tidal wind component in winter, seen clearly in the vertical phase gradient.
Journal of Atmospheric and Solar-Terrestrial Physics | 2007
Peter Hoffmann; Werner Singer; D. Keuer; W. K. Hocking; Markus Kunze; Yasuhiro Murayama
Annales Geophysicae | 2007
D. Keuer; Peter Hoffmann; Werner Singer; J. Bremer
Archive | 2006
Ch. Jacobi; C. Viehweg; D. Kürschner; Werner Singer; Peter Hoffmann; D. Keuer
Archive | 2008
Peter Hoffmann; Werner Singer; Erich Becker; Ralph Latteck; D. Keuer
Archive | 1997
Peter Hoffmann; Werner Singer; D. Keuer; J. Bremer; R. Rüster
Archive | 1995
D. Keuer; Werner Singer; Peter Hoffmann