An improvement of wind velocity estimation from radar Doppler spectra in the upper mesosphere

We have developed a new parameter estimation method for Doppler wind spectra in the mesosphere observed with an MST radar such as the MU radar in the DBS (Doppler Beam Swinging) mode. Off-line incoherent integration of the Doppler spectra is carried out with a new algorithm excluding contami...

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Bibliographic Details
Main Authors: S. Takeda, T. Nakamura, T. Tsuda
Format: Article
Language:English
Published: Copernicus Publications 2001-08-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/19/837/2001/angeo-19-837-2001.pdf
Description
Summary:We have developed a new parameter estimation method for Doppler wind spectra in the mesosphere observed with an MST radar such as the MU radar in the DBS (Doppler Beam Swinging) mode. Off-line incoherent integration of the Doppler spectra is carried out with a new algorithm excluding contamination by strong meteor echoes. At the same time, initial values on a least square fitting of the Gaussian function are derived using a larger number of integration of the spectra for a longer time and for multiple heights. As a result, a significant improvement has been achieved with the probability of a successful fitting and parameter estimation above 80 km. The top height for the wind estimation has been improved to around 95 km. A comparison between the MU radar and the High Resolution Doppler Imager (HRDI) on the UARS satellite is shown and the capability of the new method for a validation of a future satellite mission is suggested.<br><br><b>Key words. </b>Meteorology and atmospheric dynamics (middle atmosphere dynamics) – Radio science (remote sensing; signal processing)
ISSN:0992-7689
1432-0576