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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 15, issue 6
Ann. Geophys., 15, 805–812, 1997
https://doi.org/10.1007/s00585-997-0805-8
© European Geosciences Union 1997
Ann. Geophys., 15, 805–812, 1997
https://doi.org/10.1007/s00585-997-0805-8
© European Geosciences Union 1997

  30 Jun 1997

30 Jun 1997

A statistical study of underestimates of wind speeds by VHF radar

L. Thomas, I. Astin*, and R. M. Worthington L. Thomas et al.
  • Department of Physics, University of Wales, Aberystwyth, Dyfed, SY23 3BZ, UK
  • *Now at the NERC Environmental Systems Science Centre, University of Reading, Whitenights, P.O. Box 227, Reading, RG6 6AB, UK

Abstract. Comparisons are made between horizontal wind measurements carried out using a VHF-radar system at Aberystwyth (52.4°N, 4.1°W) and radiosondes launched from Aberporth, some 50 km to the south-west. The radar wind results are derived from Doppler wind measurements at zenith angles of 6° in two orthogonal planes and in the vertical direction. Measurements on a total of 398 days over a 2-year period are considered, but the major part of the study involves a statistical analysis of data collected during 75 radiosonde flights selected to minimise the spatial separation of the two sets of measurements. Whereas good agreement is found between the two sets of wind direction, radar-derived wind speeds show underestimates of 4–6% compared with radiosonde values over the height range 4–14 km. Studies of the characteristics of this discrepancy in wind speeds have concentrated on its directional dependence, the effects of the spatial separation of the two sets of measurements, and the influence of any uncertainty in the radar measurements of vertical velocities. The aspect sensitivity of radar echoes has previously been suggested as a cause of underestimates of wind speeds by VHF radar. The present statistical treatment and case-studies show that an appropriate correction can be applied using estimates of the effective radar beam angle derived from a comparison of echo powers at zenith angles of 4.2° and 8.5°.

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