The response of superpressure balloons to gravity wave motions

Superpressure balloons (SPB), which float on constant density (isopycnic) surfaces, provide a unique way of measuring the properties of atmospheric gravity waves (GW) as a function of wave intrinsic frequency. Here we devise a quasi-analytic method of investigating the SPB response to GW mot...

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Main Authors: R. A. Vincent, A. Hertzog
Format: Article
Language:English
Published: Copernicus Publications 2014-04-01
Series:Atmospheric Measurement Techniques
Online Access:http://www.atmos-meas-tech.net/7/1043/2014/amt-7-1043-2014.pdf
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spelling doaj-a736d2c89de948619a55449d2690c8bd2020-11-24T23:45:47ZengCopernicus PublicationsAtmospheric Measurement Techniques1867-13811867-85482014-04-01741043105510.5194/amt-7-1043-2014The response of superpressure balloons to gravity wave motionsR. A. Vincent0A. Hertzog1Physics Department, University of Adelaide, Adelaide 5005, AustraliaLaboratoire de Meteorologie Dynamique, &Eacute;cole Polytechnique, Palaiseau, FranceSuperpressure balloons (SPB), which float on constant density (isopycnic) surfaces, provide a unique way of measuring the properties of atmospheric gravity waves (GW) as a function of wave intrinsic frequency. Here we devise a quasi-analytic method of investigating the SPB response to GW motions. It is shown that the results agree well with more rigorous numerical simulations of balloon motions and provide a better understanding of the response of SPB to GW, especially at high frequencies. The methodology is applied to ascertain the accuracy of GW studies using 12 m diameter SPB deployed in the 2010 Concordiasi campaign in the Antarctic. In comparison with the situation in earlier campaigns, the vertical displacements of the SPB were measured directly using GPS. It is shown using a large number of Monte Carlo-type simulations with realistic instrumental noise that important wave parameters, such as momentum flux, phase speed and wavelengths, can be retrieved with good accuracy from SPB observations for intrinsic wave periods greater than ca. 10 min. The noise floor for momentum flux is estimated to be ca. 10<sup>&minus;4</sup> mPa.http://www.atmos-meas-tech.net/7/1043/2014/amt-7-1043-2014.pdf
collection DOAJ
language English
format Article
sources DOAJ
author R. A. Vincent
A. Hertzog
spellingShingle R. A. Vincent
A. Hertzog
The response of superpressure balloons to gravity wave motions
Atmospheric Measurement Techniques
author_facet R. A. Vincent
A. Hertzog
author_sort R. A. Vincent
title The response of superpressure balloons to gravity wave motions
title_short The response of superpressure balloons to gravity wave motions
title_full The response of superpressure balloons to gravity wave motions
title_fullStr The response of superpressure balloons to gravity wave motions
title_full_unstemmed The response of superpressure balloons to gravity wave motions
title_sort response of superpressure balloons to gravity wave motions
publisher Copernicus Publications
series Atmospheric Measurement Techniques
issn 1867-1381
1867-8548
publishDate 2014-04-01
description Superpressure balloons (SPB), which float on constant density (isopycnic) surfaces, provide a unique way of measuring the properties of atmospheric gravity waves (GW) as a function of wave intrinsic frequency. Here we devise a quasi-analytic method of investigating the SPB response to GW motions. It is shown that the results agree well with more rigorous numerical simulations of balloon motions and provide a better understanding of the response of SPB to GW, especially at high frequencies. The methodology is applied to ascertain the accuracy of GW studies using 12 m diameter SPB deployed in the 2010 Concordiasi campaign in the Antarctic. In comparison with the situation in earlier campaigns, the vertical displacements of the SPB were measured directly using GPS. It is shown using a large number of Monte Carlo-type simulations with realistic instrumental noise that important wave parameters, such as momentum flux, phase speed and wavelengths, can be retrieved with good accuracy from SPB observations for intrinsic wave periods greater than ca. 10 min. The noise floor for momentum flux is estimated to be ca. 10<sup>&minus;4</sup> mPa.
url http://www.atmos-meas-tech.net/7/1043/2014/amt-7-1043-2014.pdf
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