Enhancement of atmospheric radiation by an aerosol layer
Abstract
The presence of a stratospheric haze layer may produce increases in both the actinic flux and the irradiance below this layer. Such haze layers result from the injection of aerosol‐forming material into the stratosphere by volcanic eruptions. Simple heuristic arguments show that the increase in flux below the haze layer, relative to a clear sky case, is a consequence of “photon trapping.” We explore the magnitude of these flux perturbations, as a function of aerosol properties and illumination conditions, with a new radiative transfer model that can accurately compute fluxes in an inhomogeneous atmosphere with nonconservative scatterers having arbitrary phase function. One calculated consequence of the El Chichon volcanic eruption is an increase in the midday surface actinic flux at 20°N latitude, summer, by as much as 45% at 2900 Å. This increase in flux in the UV‐B wavelength range was caused entirely by aerosol scattering, without any reduction in the overhead ozone column.
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In CESM2(WACCM6), photolysis rates are calculated using lookup tables that account for the overhead ozone column and clouds but exclude the effects of aerosols, thereby reducing the effect SAI aerosols could have on tropospheric photochemistry and ozone.
“in CESM2(WACCM6) photolysis rates are calculated using lookup tables, taking into account the overhead ozone column and clouds but excluding the effects of aerosols, thereby reducing the effect SAI aerosols could have on tropospheric photochemistry and ozone.”
From Air quality impacts of stratospheric aerosol injections are likely small and mainly driven by changes in climate, not aerosol settling (2026) · cites this paper as Michelangeli et al., 1992
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- Authors
- Michelangeli, D. V., Allen, M., Yung, Y. L., Shia, R., Crisp, D., & Eluszkiewicz, J.
- Affiliations
- California Institute of Technology (US)
- Venue
- Journal of Geophysical Research: Atmospheres
- Publisher
- American Geophysical Union (AGU)
- Published
- 1992-01-20
- Volume
- 97
- Issue
- D1
- Pages
- 865-874
- ISSN
- 0148-0227 (ISSN-L)
- OpenAlex
- W2013432358
- Cited by
- 83
- References
- 25
- Citations by year
- 2026: 1 · 2024: 1 · 2023: 1 · 2022: 1 · 2021: 2 · 2020: 1 · 2018: 1 · 2016: 2 · 2013: 1 · 2012: 1
- FWCI
- 12.03
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Journal of Geophysical Research Atmospheres (publishedVersion)
- PubMed (publishedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- Funders
- California Institute of Technology
- Topics
- Physical Sciences › Environmental Science › Global and Planetary Change › Atmospheric aerosols and clouds
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Atmospheric Ozone and Climate
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Atmospheric chemistry and aerosols
- Keywords
- stratospheric haze, volcanic aerosols, photon trapping, actinic flux, UV-B radiation, aerosol light scattering, radiative transfer modeling, El Chichón eruption, ozone column, inhomogeneous atmosphere, phase function
- MeSH terms
- Atmosphere, Geology, Mathematics, Models, Theoretical, Ozone, Radiation, Radiometry, Scattering, Radiation, Ultraviolet Rays, Photons, Volcanic Eruptions, Geological Phenomena
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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