https://iopscience.iop.org/article/10.1088/1748-9326/ada2ae/meta

*Authors*
Ansar Lemon, David W. Keith and Steven C Albers

*23 December 2024*

*Abstract*
Stratospheric aerosol injection (SAI) could change the sky's appearance.
This could play a role in shaping public perception of SAI. Noticeability
depends strongly on tropospheric aerosol optical depth (AOD) and the amount
of SAI used. We aim to quantify the noticeability of changes in sky color
and brightness due to SAI. We use a 3-D visible light radiative transfer
package to generate cloudless sky images during high sun, sunset, and
twilight under SAI from the reference point of a ground observer. We
consider three aerosol types: H2SO4, CaCO3, and diamond. We consider
stratospheric aerosol loadings required to produce radiative forcings of
-1, -2, and -4 W m-2. We use population density and AOD data to compute the
distribution of AODs people experience and then simulate sky images for the
10th, 50th, and 90th percentiles of that distribution. We compare the
simulated changes in color and brightness to experimental measurements of
minimum thresholds humans can detect. The three aerosol types cause similar
changes, except most notably the diamond aerosol increases brightness of
the solar aureole by roughly three to five times less than do H2SO4 or
CaCO3. During high sun, sky whitening from sulfate SAI at -2 W m-2 is
undetectable for roughly half of observers chosen randomly from the global
population. For the remainder of the population, we expect whitening to
still be unnoticeable for all but perhaps the most astute observers aided
by color samples. Brightening and enlargement of the solar aureole is the
most visible feature during high sun for H2SO4 and CaCO3, while changes
near twilight would be the most noticeable impact of SAI. We cannot
evaluate the fraction of the population who would notice these changes.

*Source: IOP Science*

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