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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 22, issue 11
Ann. Geophys., 22, 3781–3788, 2004
https://doi.org/10.5194/angeo-22-3781-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue: 10th International Workshop on Technical and Scientific Aspects...

Ann. Geophys., 22, 3781–3788, 2004
https://doi.org/10.5194/angeo-22-3781-2004
© Author(s) 2004. This work is distributed under
the Creative Commons Attribution 3.0 License.

  29 Nov 2004

29 Nov 2004

Retrieval of atmospheric static stability from MST radar return signal power

D. A. Hooper1,2, J. Arvelius1, and K. Stebel1,3 D. A. Hooper et al.
  • 1Swedish Institute of Space Physics, Kiruna, Sweden
  • 2now at: Rutherford Appleton Laboratory, Chilton, Didcot, UK
  • 3now at: Norwegian Institute for Air Research, Tromsø, Norway

Abstract. An empirical technique for retrieving profiles of the square of the Brunt-Väisälä frequency, ωB2, from MST radar return signal power is presented. The validity of the technique, which is applied over the altitude range 1.0-15.7km, is limited to those altitudes at which the humidity contributions to the mean vertical gradient of generalised potential refractive index, M, can be ignored. Although this is commonly assumed to be the case above the first few kilometres of the atmosphere, it is shown that humidity contributions can be significant right up to the tropopause level. In specific circumstances, however, the technique is valid over large sections of the troposphere. Comparisons of radar- and (balloon-borne) radiosonde-derived ωB2 profiles are typically quantitatively and qualitatively well matched. However, the horizontal separation between the radar and the radiosondes (which were launched at the radar site) increases with increasing altitude. Under conditions of mountain wave activity, which can be highly localised, large discrepancies can occur at lower-stratospheric altitudes. This demonstrates the fact that radiosonde observations cannot necessarily be assumed to be representative of the atmosphere above the launch site.

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