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Proceedings with Extended Abstracts (single PDF file) - Radio ...

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Figure 2: Mean zonal and meridional winds (left and middle) derived from standard DBSexperiments and radial velocities (right) obtained <strong>with</strong> interleaved oblique narrow beams(HPFW=6.6 ◦ ) at 17.2 ◦ off-zenith angle during dual-beamwidth observation.The mean horizontal winds were less than 10 m/s during the whole experiment periodon April 23, 2003 (Figure 2). Since the velocities were very small the correction term forbeam and shear broadening used in the <strong>single</strong>-beamwidth method was negligible (middlepanel of Figure 3) and σ 2 turb ≈ σ 2 obs .The 3-hour mean pro<strong>file</strong> of σ 2 turb obtained from the dual-beamwidth method shownin Figure 4 depict velocity variances between 5 and about 15 m 2 /s 2 below 78 km wherecontributions from specular reflections should be small or negligible. With a mean Brunt-Vaisala frequency of 0.018 for the altitude range between 65 and 84 km based on a meantemperature pro<strong>file</strong> for April after falling sphere measurements at Andenes (Lübken,1999) these turbulent velocity variances can directly be converted into turbulent kineticenergy dissipation rates. These values between 10 and 60 mW/kg (top axis in the rightpanel of Figure 4) are in reasonable agreement <strong>with</strong> rocket observations during springtransition (Müllemann et al., 2002). The first results of simultaneous 2BW and 1BWobservations during low wind speed conditions are in good agreement. Further tests ofFigure 3: Pro<strong>file</strong>s of the observed spectral widths σ 2 obs (left) from the NW and SE narrowbeam experiments, the correction term σ 2 corr (middle) and the turbulent spectral widthσ 2 turb (right) obtained <strong>with</strong> the <strong>single</strong> beam width method.247

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