First quasi-Lagrangian in situ measurements of Antarctic Polar springtime ozone: Observed ozone loss rates from the Concordiasi long-duration balloon campaign

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Abstract

We present ozone measurements made using state-of-the-art ultraviolet photometers onboard three long-duration stratospheric balloons launched as part of the Concordiasi campaign in austral spring 2010. Ozone loss rates calculated by matching air parcels sampled at different times and places during the polar spring are in agreement with rates previously derived from ozonesonde measurements, for the vortex average, ranging between 2 and 7 ppbv per sunlit hour or between 25 and 110 ppbv per day. However, the geographical coverage of these long-duration stratospheric balloon platforms provides new insights into the temporal and spatial patterns of ozone loss over Antarctica. Very large ozone loss rates of up to 230 ppbv per day (16 ppbv per sunlit hour) are observed for air masses that are downwind of the Antarctic Peninsula and/or over the East Antarctic region. The ozone loss rate maximum downstream of the Antarctic Peninsula region is consistent with high PSC occurrence from CALIPSO and large ClO abundances from MLS satellite observations for 12-22 September 2010, and with a chemical box model simulation using JPL 2011 kinetics with full chlorine activation.

Figures

  • Table 1. Details of balloon flights analysed for ozone loss rates
  • Figure 1. The flight paths of the three ozone Concordiasi balloons are displayed.
  • Figure 2. Ozone and potential temperature along the trajectory of each of the ozone instrumented Concordiasi balloons. Clearly measured is the ozone loss under perturbed springtime conditions. The diurnal heating and cooling of the balloon is evident in the potential temperature variations.
  • Figure 3. Ozone loss per sunlit hour for all of the matches for each of the ozone instrumented Concordiasi balloon flights. The matches are binned into the longitude quadrant of their end match (blue 0– 90◦ E, turquoise 90–180◦ E, yellow 90–180◦W and red 0–90◦W). While each match requires the potential temperature to be within 1 K, all matches with an initial or end match within ±5 days are binned to give the ozone versus sunlit hour regression shown. This way a match ending on day 263 will be represented in both the 260 and 265 data points above. The colour bar is used to indicate the potential temperature of the ozone observations as plotted with dots on the map. The error bars represent the standard error of each regression fit, and the coloured numbers are the number of matches used in the regression fitting. Also shown are simulated ozone loss rates calculated by running a chemical box model along the longest match trajectory for each time bin (black line). The box model assumes ClOx =Cly and JPL 2011 kinetics.
  • Figure 4. As Fig. 3 but for ozone loss per day.
  • Figure 5. Ozone losses binned according to the mean latitude of the match.
  • Figure 6. Ozone loss according to mean normalised PV of the match.
  • Figure 7. Microwave Limb Sounder ClO data retrieved on the 68.13 hPa level over the 10 day periods used for the four ozone loss calculations in Figs. 3 and 4.

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APA

Schofield, R., Avallone, L. M., Kalnajs, L. E., Hertzog, A., Wohltmann, I., & Rex, M. (2015). First quasi-Lagrangian in situ measurements of Antarctic Polar springtime ozone: Observed ozone loss rates from the Concordiasi long-duration balloon campaign. Atmospheric Chemistry and Physics, 15(5), 2463–2472. https://doi.org/10.5194/acp-15-2463-2015

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