Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder

<p>Stratospheric Inferred Winds (SIW) is a Swedish mini sub-millimeter limb sounder selected for the 2nd InnoSat platform, with launch planned for around 2022. It is intended to fill the altitude gap between 30 and 70&thinsp;km in atmospheric wind measurements and also aims at pursuing...

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Main Authors: P. Baron, D. Murtagh, P. Eriksson, J. Mendrok, S. Ochiai, K. Pérot, H. Sagawa, M. Suzuki
Format: Article
Language:English
Published: Copernicus Publications 2018-07-01
Series:Atmospheric Measurement Techniques
Online Access:https://www.atmos-meas-tech.net/11/4545/2018/amt-11-4545-2018.pdf
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spelling doaj-02be7593a9a54ac59856b88a6df2972b2020-11-24T21:54:14ZengCopernicus PublicationsAtmospheric Measurement Techniques1867-13811867-85482018-07-01114545456610.5194/amt-11-4545-2018Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounderP. Baron0D. Murtagh1P. Eriksson2J. Mendrok3S. Ochiai4K. Pérot5H. Sagawa6M. Suzuki7National Institute of Information and Communications Technology, 4-2-1 Nukui-kitamachi, Koganei, Tokyo 184-8795, Japan Department of Space, Earth and Environment, Chalmers University of Technology, 41296 Gothenburg, SwedenDepartment of Space, Earth and Environment, Chalmers University of Technology, 41296 Gothenburg, SwedenDepartment of Space, Earth and Environment, Chalmers University of Technology, 41296 Gothenburg, SwedenNational Institute of Information and Communications Technology, 4-2-1 Nukui-kitamachi, Koganei, Tokyo 184-8795, Japan Department of Space, Earth and Environment, Chalmers University of Technology, 41296 Gothenburg, SwedenDivision of Science, Kyoto Sangyo University, Kyoto, Japan Japan Aerospace Exploration Agency, Tsukuba, 305-8505 Japan<p>Stratospheric Inferred Winds (SIW) is a Swedish mini sub-millimeter limb sounder selected for the 2nd InnoSat platform, with launch planned for around 2022. It is intended to fill the altitude gap between 30 and 70&thinsp;km in atmospheric wind measurements and also aims at pursuing the limb observations of temperature and key atmospheric constituents between 10 and 90&thinsp;km when current satellite missions will probably come to an end. Line-of-sight winds are retrieved from the Doppler shift of molecular emission lines introduced by the wind field. Observations will be performed with two antennas pointing toward the limb in perpendicular directions in order to reconstruct the 2-D horizontal wind vector. Each antenna has a vertical field of view (FOV) of 5&thinsp;km. The chosen spectral band, near 655&thinsp;GHz, contains a dense group of strong O<sub>3</sub> lines suitable for exploiting the small amount of wind information in stratospheric spectra. Using both sidebands of the heterodyne receiver, a large number of chemical species will be measured, including O<sub>3</sub> isotopologues, H<sub>2</sub>O, HDO, HCl, ClO, N<sub>2</sub>O, HNO<sub>3</sub>, NO, NO<sub>2</sub>, HCN, CH<sub>3</sub>CN and HO<sub>2</sub>. This paper presents a simulation study that assesses measurement performance. The line-of-sight winds are retrieved between 30 and 90&thinsp;km with the best sensitivity between 35 and 70&thinsp;km, where the precision (1<i>σ</i>) is 5–10&thinsp;m s<sup>−1</sup> for a single scan. Similar performance can be obtained during day and night conditions except in the lower mesosphere, where the photo-dissociation of O<sub>3</sub> in daytime reduces the sensitivity by 50&thinsp;% near 70&thinsp;km. Profiles of O<sub>3</sub>, H<sub>2</sub>O and temperature are retrieved with high precision up to 50&thinsp;km ( &lt; 1&thinsp;%,  &lt; 2&thinsp;%, 1&thinsp;K, respectively). Systematic errors due to uncertainties in spectroscopic parameters, in the radiometer sideband ratio and in the radiance calibration process are investigated. A large wind retrieval bias of 10–30&thinsp;m s<sup>−1</sup> between 30 and 40&thinsp;km could be induced by the air-broadening parameter uncertainties of O<sub>3</sub> lines. This highlights the need for good knowledge of these parameters and for studying methods to mitigate the retrieval bias.</p>https://www.atmos-meas-tech.net/11/4545/2018/amt-11-4545-2018.pdf
collection DOAJ
language English
format Article
sources DOAJ
author P. Baron
D. Murtagh
P. Eriksson
J. Mendrok
S. Ochiai
K. Pérot
H. Sagawa
M. Suzuki
spellingShingle P. Baron
D. Murtagh
P. Eriksson
J. Mendrok
S. Ochiai
K. Pérot
H. Sagawa
M. Suzuki
Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder
Atmospheric Measurement Techniques
author_facet P. Baron
D. Murtagh
P. Eriksson
J. Mendrok
S. Ochiai
K. Pérot
H. Sagawa
M. Suzuki
author_sort P. Baron
title Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder
title_short Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder
title_full Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder
title_fullStr Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder
title_full_unstemmed Simulation study for the Stratospheric Inferred Winds (SIW) sub-millimeter limb sounder
title_sort simulation study for the stratospheric inferred winds (siw) sub-millimeter limb sounder
publisher Copernicus Publications
series Atmospheric Measurement Techniques
issn 1867-1381
1867-8548
publishDate 2018-07-01
description <p>Stratospheric Inferred Winds (SIW) is a Swedish mini sub-millimeter limb sounder selected for the 2nd InnoSat platform, with launch planned for around 2022. It is intended to fill the altitude gap between 30 and 70&thinsp;km in atmospheric wind measurements and also aims at pursuing the limb observations of temperature and key atmospheric constituents between 10 and 90&thinsp;km when current satellite missions will probably come to an end. Line-of-sight winds are retrieved from the Doppler shift of molecular emission lines introduced by the wind field. Observations will be performed with two antennas pointing toward the limb in perpendicular directions in order to reconstruct the 2-D horizontal wind vector. Each antenna has a vertical field of view (FOV) of 5&thinsp;km. The chosen spectral band, near 655&thinsp;GHz, contains a dense group of strong O<sub>3</sub> lines suitable for exploiting the small amount of wind information in stratospheric spectra. Using both sidebands of the heterodyne receiver, a large number of chemical species will be measured, including O<sub>3</sub> isotopologues, H<sub>2</sub>O, HDO, HCl, ClO, N<sub>2</sub>O, HNO<sub>3</sub>, NO, NO<sub>2</sub>, HCN, CH<sub>3</sub>CN and HO<sub>2</sub>. This paper presents a simulation study that assesses measurement performance. The line-of-sight winds are retrieved between 30 and 90&thinsp;km with the best sensitivity between 35 and 70&thinsp;km, where the precision (1<i>σ</i>) is 5–10&thinsp;m s<sup>−1</sup> for a single scan. Similar performance can be obtained during day and night conditions except in the lower mesosphere, where the photo-dissociation of O<sub>3</sub> in daytime reduces the sensitivity by 50&thinsp;% near 70&thinsp;km. Profiles of O<sub>3</sub>, H<sub>2</sub>O and temperature are retrieved with high precision up to 50&thinsp;km ( &lt; 1&thinsp;%,  &lt; 2&thinsp;%, 1&thinsp;K, respectively). Systematic errors due to uncertainties in spectroscopic parameters, in the radiometer sideband ratio and in the radiance calibration process are investigated. A large wind retrieval bias of 10–30&thinsp;m s<sup>−1</sup> between 30 and 40&thinsp;km could be induced by the air-broadening parameter uncertainties of O<sub>3</sub> lines. This highlights the need for good knowledge of these parameters and for studying methods to mitigate the retrieval bias.</p>
url https://www.atmos-meas-tech.net/11/4545/2018/amt-11-4545-2018.pdf
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