Energetic particle induced intra-seasonal variability of ozone inside the Antarctic polar vortex observed in satellite data

Measurements from 2002 to 2011 by three independent satellite instruments, namely MIPAS, SABER, and SMR on board the ENVISAT, TIMED, and Odin satellites are used to investigate the intra-seasonal variability of stratospheric and mesospheric O-3 volume mixing ratio (vmr) inside the Antarctic polar vortex due to solar and geomagnetic activity. In this study, we individually analysed the relative O-3 vmr variations between maximum and minimum conditions of a number of solar and geomagnetic indices (F10.7 cm solar radio flux, Ap index, >= 2 MeV electron flux). The indices are 26-day averages centred at 1 April, 1 May, and 1 June while O-3 is based on 26-day running means from 1 April to 1 November at altitudes from 20 to 70 km. During solar quiet time from 2005 to 2010, the composite of all three instruments reveals an apparent negative O-3 signal associated to the geomagnetic activity (Ap index) around 1 April, on average reaching amplitudes between -5 and -10% of the respective O-3 background. The O-3 response exceeds the significance level of 95% and propagates downwards throughout the polar winter from the stratopause down to similar to 25 km. These observed results are in good qualitative agreement with the O-3 vmr pattern simulated with a three-dimensional chemistry-transport model, which includes particle impact ionisation.