Preprints
https://doi.org/10.5194/amt-2021-171
https://doi.org/10.5194/amt-2021-171

  23 Jun 2021

23 Jun 2021

Review status: a revised version of this preprint was accepted for the journal AMT and is expected to appear here in due course.

Correction of wind bias for the lidar on-board Aeolus using telescope temperatures

Fabian Weiler1, Michael Rennie2, Thomas Kanitz3, Lars Isaksen2, Elena Checa3, Jos de Kloe4, Ngozi Okunde4, and Oliver Reitebuch1 Fabian Weiler et al.
  • 1Deutsches Zentrum für Luft- und Raumfahrt, Institut für Physik der Atmosphäre, Oberpfaffenhofen, Germany
  • 2European Centre for Medium-Range Weather Forecasts, Shinfield Park, Reading RG2 9AX, United Kingdom
  • 3European Space Agency-ESTEC, Keplerlaan 1, Noordwijk NL-2201 AZ, The Netherlands
  • 4Royal Netherlands Meteorological Institute (KNMI), Utrechtseweg 297, 3731 GA De Bilt, The Netherlands

Abstract. The European Space Agency satellite Aeolus provides continuous profiles of the horizontal line-of-sight wind component at a global scale. It was successfully launched into space in August 2018 with the goal to improve numerical weather prediction (NWP). Aeolus data has already been successfully assimilated into several NWP models and has already helped to significantly improve the quality of weather forecasts. To achieve this major milestone the identification and correction of several systematic error sources was necessary. One of them is related to small temperatures fluctuations across the 1.5 m diameter primary mirror of the telescope which cause varying wind biases along the orbit of up to 8 m/s. This paper presents a detailed overview of the influence of the telescope temperature variations on the Aeolus wind products and describes the approach to correct for this systematic error source in the operational near-real-time (NRT) processing. It was shown that the telescope temperature variations along the orbit are due to changes of the top-of-atmosphere short- and long-wave radiation of the Earth and the response of the telescope’s thermal control system to that. To correct for this effect ECMWF model-equivalent winds are used as bias reference to describe the wind bias in a multiple linear regression model as a function of various temperature sensors located on the primary telescope mirror. This correction scheme has been in operational use at ECMWF since April 2020 and is capable of reducing a large part of the telescope-induced wind bias. In cases where the influence of the temperature variations is particularly strong it was shown that the bias correction can improve the orbital bias variation by up to 53 %. Moreover, it was demonstrated that the approach of using ECMWF model-equivalent winds is justified by the fact that the global bias of models u-component winds w.r.t to radiosondes is smaller than 0.3 m/s. However, this paper also presents the alternative of using Aeolus ground return winds which serve as zero wind reference in the multiple linear regression model. The results show that the approach based on ground return winds only performs 10.8 % worse than the ECMWF model-based approach and thus has good potential for future applications for upcoming reprocessing campaigns or even in the NRT processing of Aeolus wind products.

Fabian Weiler et al.

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on amt-2021-171', Anonymous Referee #1, 31 Jul 2021
    • AC1: 'Reply on RC1', Fabian Weiler, 07 Sep 2021
  • RC2: 'Comment on amt-2021-171', Anonymous Referee #2, 19 Aug 2021
    • AC2: 'Reply on RC2', Fabian Weiler, 07 Sep 2021

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on amt-2021-171', Anonymous Referee #1, 31 Jul 2021
    • AC1: 'Reply on RC1', Fabian Weiler, 07 Sep 2021
  • RC2: 'Comment on amt-2021-171', Anonymous Referee #2, 19 Aug 2021
    • AC2: 'Reply on RC2', Fabian Weiler, 07 Sep 2021

Fabian Weiler et al.

Fabian Weiler et al.

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Short summary
This paper summarizes the identification and correction of one of the most important systematic error sources for the wind measurements of the ESA satellite Aeolus. It depicts the effects of small temperature variations of the primary telescope mirror on the quality of the wind products and describes the approach to correct for it in the near-real-time processing. Moreover, the performance of the correction approach is assessed and alternative approaches are discussed.