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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Copernicus Publications
2014-04-01
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Series: | Atmospheric Measurement Techniques |
Online Access: | http://www.atmos-meas-tech.net/7/1043/2014/amt-7-1043-2014.pdf |
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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, École 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>−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>−4</sup> mPa. |
url |
http://www.atmos-meas-tech.net/7/1043/2014/amt-7-1043-2014.pdf |
work_keys_str_mv |
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