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 km in atmospheric wind measurements and also aims at pursuing...
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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 km in atmospheric wind measurements and also aims at pursuing the limb observations of temperature and key atmospheric constituents between 10 and 90 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 km. The chosen spectral band, near 655 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 km with the best sensitivity between 35 and 70 km, where the precision (1<i>σ</i>) is 5–10 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 % near 70 km. Profiles of O<sub>3</sub>, H<sub>2</sub>O and temperature are retrieved with high precision up to 50 km ( < 1 %, < 2 %, 1 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 m s<sup>−1</sup> between 30 and 40 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 km in atmospheric wind measurements and also aims at pursuing
the limb observations of temperature and key atmospheric constituents between
10 and 90 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 km. The chosen spectral band, near
655 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 km with the best
sensitivity between 35 and 70 km, where the precision (1<i>σ</i>) is
5–10 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 % near 70 km. Profiles of O<sub>3</sub>, H<sub>2</sub>O and
temperature are retrieved with high precision up to 50 km
( < 1 %, < 2 %, 1 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 m s<sup>−1</sup> between 30 and 40 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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