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An Overview of Investigations Into the Permeability of the Antarctic Vortex Using Loon Balloon
Trajectory Data
OverviewNew Zealand Marsden-funded project → The permeability of the
Antarctic vortex. Location information from super-pressure Loon
balloons used to analyze wind fields in the Southern Hemisphere
mid-latitude stratosphere. First assess quality of several reanalyses
(ref 1). Balloon GPS location data used to derive winds which were
then compared with values from the reanalyses interpolated to the
balloon times and locations (Figure 1).
Greg Bodeker
Jonathan Conway
Adrian McDonald
AGU 2019 – Poster A33Q-2930
Figure 1: Wind speeds measured from Loon flight #
263 along with interpolated (re)analysis winds. Note
the tendency for the balloon winds to oscillate about
the (re)analysis winds.
References1. Friedrich, L.S.; McDonald, A.J.; Bodeker, G.E.; Cooper, K.E.; Lewis, J. and Paterson, A.J., A comparison of Loon balloon observations and
stratospheric reanalyses products, Atmos. Chem. Phys., doi:10.5194/acp-17-855-2017, 2017.
Figure 2: Trajectory separations
as a function of time.
Comparisons between Loon trajectories and calculated
from trajectory model applied to reanalysis winds;
MERRA-2 winds generate the most accurate simulated
trajectories (Figure 2). Developed method to correct Loon
temperatures to account for solar radiative heating of
balloon (Figure 3) based on the following equation:
In second study (ref 2), analyzed horizontal velocity
spectra from the balloons’ quasi-intrinsic frame: showed
evidence of persistent peak in intrinsic wind spectrum
around inertial frequency (Figure 4 and 5). In Southern
Hemisphere mid-latitudes, amplitude of horizontal velocity
perturbations larger than previously seen in polar super-
pressure balloon campaigns. Rotary spectral analysis
showed near-circular anti-cyclonic rotation of horizontal
wind perturbations dominate around the inertial frequency.
Analyses of the Loon data spurred further investigations
into the structure of meridional impermeability across the
vortex edge (Figure 6)
Figure 3: An example of the differences
between Loon measured temperatures and
those extracted from NCEP/CFSR reanalysis
at the time and location of the Loon
measurements. The temperature differences
have been disaggregated by solar zenith
angle (SZA). The solid red line shows the
mean difference in each SZA bin while the
blue line shows the modelled differences
obtained by fitting equation 1 to the
differences.
Figure 4: (left) the paths of six super-pressure Loon balloons
following their launch on 28 February 2014 from the central South
Island of New Zealand. Circles denote the position of the balloons at
00 UTC. The altitude and horizontal wind speeds of each balloon
are also shown. (right) another example of 4 Loon balloons
launched on 7 July 2014 showing similar persistent peak in the
intrinsic wind spectrum around the inertial frequency.
Figure 6: Trajectory
analysis from NCEP/CFSR
reanalyses showing the
likelihood of vortex crossing
events in each month
(coloured histograms)
overlaid on contour plots of
meridional impermeability –
darker regions show where
the vortex edge is less
permeable to meridional
transport and/or mixing.
Large year-to-year
differences are apparent.
The bifurcation in the vortex
impermeability is detailed in
ref 3.
Figure 5: Log‐mean spectral amplitudes of
Ekh binned using R(f) for (a, b) latitudes
between 30°S and 45°S and (c, d) 45°-
60°S, for (left‐hand column) 8‐ and
(right‐hand column) 4‐day periods. Number
of individual segments contributing to bin
averages given in legend panels. Strongest
anti-cyclonic rotation more common in
balloon flight segments with weak zonal
winds and during the austral summer.
2. Conway, J.P.; Bodeker, G.E.; Waugh, D.W.; Murphy, D.J.; Cameron, C. and Lewis, J., Using Project Loon super-pressure balloon observations to investigate the inertial
peak in the intrinsic wind spectrum in the mid-latitude stratosphere, J. Geophys. Res., doi:10.1029/2018JD030195, 2019.
3. Conway, J.; Bodeker, G.E. and Cameron, C., Bifurcation of potential vorticity gradients across the Southern Hemisphere stratospheric polar vortex, Atmos. Chem. Phys.,
doi:10.5194/acp-18-8065-2018, 2018.