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An Overview of Investigations Into the Permeability of the Antarctic Vortex Using Loon Balloon Trajectory Data Overview New 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. References 1. Friedrich, L.S.; McDonald, A.J.; Bodeker, G.E.; Cooper, K.E.; Lewis, J. and Paterson, A.J., A comparison of Loon balloon obse rva tions 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 E kh 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 obs ervations 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 strato sph eric polar vortex, Atmos. Chem. Phys., doi:10.5194/acp - 18 - 8065 - 2018, 2018.

An Overview of Investigations Into the Permeability of the ...An Overview of Investigations Into the Permeability of the Antarctic Vortex Using Loon Balloon Trajectory Data Overview

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Page 1: An Overview of Investigations Into the Permeability of the ...An Overview of Investigations Into the Permeability of the Antarctic Vortex Using Loon Balloon Trajectory Data Overview

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.