Source: Thomas Pagano, NASA/JPL-Caltech
Published: July 9, 2019

The Antarctic Vortex forms early in polar winter and is relatively isolated from the air in the southern midlatitudes. The extreme cold of the vortex allows microscopic-sized ice particles to form in the stratosphere. Chemical reactions occur on the surfaces of these cloud particles (known as Polar Stratospheric Clouds or PSCs) in a way that transforms stable "inactive" chlorine reservoirs into "active" chlorine molecules, after sunlight returns to the polar regions in late winter and early spring.

Ozone is then rapidly destroyed in a catalytic fashion - that is, by chemical cycles that regenerate active chlorine (with bromine compounds also involved) many times around. Ozone only returns to normal values after the vortex is broken up and midlatitude air is able to enter the sky over Antarctica — replenishing ozone and converting the active chlorine back to an inactive form.

Visualization Approach

This visualization is a plot of an isosurface of ozone volume mixing ratio at 5 x 10^-7 parts per million. The isosurface becomes transparent above 18 kilometers. The altitude is scaled by 100 and offset by 10 kilometers. The altitude scale assumes a standard pressure to altitude conversion and is not a critical factor—-but it allows the isosurface to be plotted on the globe.

Frames in the visualization movie alternate between ascending and descending satellite orbits, with a 12-hour period between ascending and descending. Data gaps have been filled and the data are smoothed on a 3x3 grid and oversampled from 1x1 degree to 0.25 x 0.25 degree.