Abstract. As a consequence of extreme heat and drought,
record-breaking wildfires developed and ravaged south-eastern Australia
during the fire season 2019–2020. The fire strength reached its paroxysmal
phase at the turn of the year 2019–2020. During this phase, pyrocumulonimbus clouds (pyroCb) developed and injected biomass burning aerosols and gases into the
upper troposphere and lower stratosphere (UTLS). The UTLS aerosol layer was
massively perturbed by these fires, with aerosol extinction increased by a
factor of 3 in the visible spectral range in the Southern Hemisphere, with
respect to a background atmosphere, and stratospheric aerosol optical depth
reaching values as large as 0.015 in February 2020. Using the best available
description of this event by observations, we estimate the radiative forcing
(RF) of such perturbations of the Southern Hemispheric aerosol layer. We use
offline radiative transfer modelling driven by observed information of the
aerosol extinction perturbation and its spectral variability obtained from
limb satellite measurements. Based on hypotheses on the absorptivity and the
angular scattering properties of the aerosol layer, the regional (at three
latitude bands in the Southern Hemisphere) clear-sky TOA (top-of-atmosphere)
RF is found varying from small positive values to relatively large negative
values (up to −2.0 W m−2), and the regional clear-sky surface RF is
found to be consistently negative and reaching large values (up to −4.5 W m−2). We argue that clear-sky positive values are unlikely for this
event, if the ageing/mixing of the biomass burning plume is mirrored by the
evolution of its optical properties. Our best estimate for the area-weighted
global-equivalent clear-sky RF is -0.35±0.21 (TOA RF) and
-0.94±0.26 W m−2 (surface RF), thus the strongest documented for
a fire event and of comparable magnitude with the strongest volcanic
eruptions of the post-Pinatubo era. The surplus of RF at the surface, with
respect to TOA, is due to absorption within the plume that has contributed
to the generation of ascending smoke vortices in the stratosphere. Highly
reflective underlying surfaces, like clouds, can nevertheless swap negative
to positive TOA RF, with global average RF as high as +1.0 W m−2
assuming highly absorbing particles.