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@ARTICLE{Hindley:868088,
author = {Hindley, Neil P. and Wright, Corwin J. and Smith, Nathan D.
and Hoffmann, Lars and Holt, Laura A. and Alexander, M. Joan
and Moffat-Griffin, Tracy and Mitchell, Nicholas J.},
title = {{G}ravity waves in the winter stratosphere over the
{S}outhern {O}cean: high-resolution satellite observations
and 3-{D} spectral analysis},
journal = {Atmospheric chemistry and physics},
volume = {19},
number = {24},
issn = {1680-7324},
address = {Katlenburg-Lindau},
publisher = {EGU},
reportid = {FZJ-2019-06679},
pages = {15377 - 15414},
year = {2019},
abstract = {Atmospheric gravity waves play a key role in the transfer
of energy and momentum between layers of the Earth's
atmosphere. However, nearly all general circulation models
(GCMs) seriously under-represent the momentum fluxes of
gravity waves at latitudes near 60∘ S, which can lead to
significant biases. A prominent example of this is the
“cold pole problem”, where modelled winter stratospheres
are unrealistically cold. There is thus a need for
large-scale measurements of gravity wave fluxes near
60∘ S, and indeed globally, to test and constrain GCMs.
Such measurements are notoriously difficult, because they
require 3-D observations of wave properties if the fluxes
are to be estimated without using significant limiting
assumptions. Here we use 3-D satellite measurements of
stratospheric gravity waves from NASA's Atmospheric Infrared
Sounder (AIRS) Aqua instrument. We present the first
extended application of a 3-D Stockwell transform (3DST)
method to determine localised gravity wave amplitudes,
wavelengths and directions of propagation around the entire
region of the Southern Ocean near 60∘ S during austral
winter 2010. We first validate our method using a synthetic
wavefield and two case studies of real gravity waves over
the southern Andes and the island of South Georgia. A new
technique to overcome wave amplitude attenuation problems in
previous methods is also presented. We then characterise
large-scale gravity wave occurrence frequencies, directional
momentum fluxes and short-timescale intermittency over the
entire Southern Ocean. Our results show that highest wave
occurrence frequencies, amplitudes and momentum fluxes are
observed in the stratosphere over the mountains of the
southern Andes and Antarctic Peninsula. However, we find
that around $60 \%–80 \%$ of total zonal-mean momentum
flux is located over the open Southern Ocean during
June–August, where a large “belt” of increased wave
occurrence frequencies, amplitudes and fluxes is observed.
Our results also suggest significant short-timescale
variability of fluxes from both orographic and
non-orographic sources in the region. A particularly
striking result is a widespread convergence of gravity wave
momentum fluxes towards latitudes around 60∘ S from the
north and south. We propose that this convergence, which is
observed at nearly all longitudes during winter, could
account for a significant part of the under-represented flux
in GCMs at these latitudes.},
cin = {JSC},
ddc = {550},
cid = {I:(DE-Juel1)JSC-20090406},
pnm = {511 - Computational Science and Mathematical Methods
(POF3-511)},
pid = {G:(DE-HGF)POF3-511},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000503444400003},
doi = {10.5194/acp-19-15377-2019},
url = {https://juser.fz-juelich.de/record/868088},
}