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

<p>The European Space Agency (ESA) Earth Explorer satellite Aeolus provides continuous profiles of the horizontal line-of-sight wind component globally from space. It was successfully launched in August 2018 with the goal to improve numerical weather prediction (NWP). Aeolus data have already...

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Autores principales: F. Weiler, M. Rennie, T. Kanitz, L. Isaksen, E. Checa, J. de Kloe, N. Okunde, O. Reitebuch
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Publicado: Copernicus Publications 2021
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spelling oai:doaj.org-article:e3054c6892474c109eb92fedae1a263a2021-11-17T05:22:14ZCorrection of wind bias for the lidar on board Aeolus using telescope temperatures10.5194/amt-14-7167-20211867-13811867-8548https://doaj.org/article/e3054c6892474c109eb92fedae1a263a2021-11-01T00:00:00Zhttps://amt.copernicus.org/articles/14/7167/2021/amt-14-7167-2021.pdfhttps://doaj.org/toc/1867-1381https://doaj.org/toc/1867-8548<p>The European Space Agency (ESA) Earth Explorer satellite Aeolus provides continuous profiles of the horizontal line-of-sight wind component globally from space. It was successfully launched in August 2018 with the goal to improve numerical weather prediction (NWP). Aeolus data have already been successfully assimilated into several NWP models and have already helped to significantly improve the quality of weather forecasts. To achieve this major milestone the identification and correction of several systematic error sources were necessary. One of them is related to small fluctuations of the temperatures 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<span class="inline-formula"><sup>−1</sup></span>. 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 in the top-of-atmosphere reflected shortwave and outgoing longwave radiation of the Earth and the related response of the telescope's thermal control system. To correct for this effect ECMWF model-equivalent winds are used as a 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 model <span class="inline-formula"><i>u</i></span>-component winds with respect to radiosondes is smaller than 0.3 m s<span class="inline-formula"><sup>−1</sup></span>. Furthermore, this paper presents the alternative of using Aeolus ground return winds which serve as a 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 a good potential for future applications for upcoming reprocessing campaigns or even in the NRT processing of Aeolus wind products.</p>F. WeilerM. RennieT. KanitzL. IsaksenE. ChecaJ. de KloeN. OkundeO. ReitebuchCopernicus PublicationsarticleEnvironmental engineeringTA170-171Earthwork. FoundationsTA715-787ENAtmospheric Measurement Techniques, Vol 14, Pp 7167-7185 (2021)
institution DOAJ
collection DOAJ
language EN
topic Environmental engineering
TA170-171
Earthwork. Foundations
TA715-787
spellingShingle Environmental engineering
TA170-171
Earthwork. Foundations
TA715-787
F. Weiler
M. Rennie
T. Kanitz
L. Isaksen
E. Checa
J. de Kloe
N. Okunde
O. Reitebuch
Correction of wind bias for the lidar on board Aeolus using telescope temperatures
description <p>The European Space Agency (ESA) Earth Explorer satellite Aeolus provides continuous profiles of the horizontal line-of-sight wind component globally from space. It was successfully launched in August 2018 with the goal to improve numerical weather prediction (NWP). Aeolus data have already been successfully assimilated into several NWP models and have already helped to significantly improve the quality of weather forecasts. To achieve this major milestone the identification and correction of several systematic error sources were necessary. One of them is related to small fluctuations of the temperatures 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<span class="inline-formula"><sup>−1</sup></span>. 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 in the top-of-atmosphere reflected shortwave and outgoing longwave radiation of the Earth and the related response of the telescope's thermal control system. To correct for this effect ECMWF model-equivalent winds are used as a 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 model <span class="inline-formula"><i>u</i></span>-component winds with respect to radiosondes is smaller than 0.3 m s<span class="inline-formula"><sup>−1</sup></span>. Furthermore, this paper presents the alternative of using Aeolus ground return winds which serve as a 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 a good potential for future applications for upcoming reprocessing campaigns or even in the NRT processing of Aeolus wind products.</p>
format article
author F. Weiler
M. Rennie
T. Kanitz
L. Isaksen
E. Checa
J. de Kloe
N. Okunde
O. Reitebuch
author_facet F. Weiler
M. Rennie
T. Kanitz
L. Isaksen
E. Checa
J. de Kloe
N. Okunde
O. Reitebuch
author_sort F. Weiler
title Correction of wind bias for the lidar on board Aeolus using telescope temperatures
title_short Correction of wind bias for the lidar on board Aeolus using telescope temperatures
title_full Correction of wind bias for the lidar on board Aeolus using telescope temperatures
title_fullStr Correction of wind bias for the lidar on board Aeolus using telescope temperatures
title_full_unstemmed Correction of wind bias for the lidar on board Aeolus using telescope temperatures
title_sort correction of wind bias for the lidar on board aeolus using telescope temperatures
publisher Copernicus Publications
publishDate 2021
url https://doaj.org/article/e3054c6892474c109eb92fedae1a263a
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AT mrennie correctionofwindbiasforthelidaronboardaeolususingtelescopetemperatures
AT tkanitz correctionofwindbiasforthelidaronboardaeolususingtelescopetemperatures
AT lisaksen correctionofwindbiasforthelidaronboardaeolususingtelescopetemperatures
AT echeca correctionofwindbiasforthelidaronboardaeolususingtelescopetemperatures
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