the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Impact of Spectral Aerosol Radiative Forcing at the Izaña Observatory during the August 2023 Extreme Wildfires
Abstract. Extreme wildfires represent a highly variable source of atmospheric aerosols with potentially strong impacts on surface solar radiation. In August 2023, an exceptional wildfire on Tenerife (Canary Islands, Spain) reached the neighbourhoods of the Izana Observatory (IZO, 2400 m a.s.l.). This near-source configuration enabled a rare observational characterisation of the spectral radiative effects of biomass-burning aerosols. During the most intense phases of the event (17–18 August), aerosol optical depth (AOD) at 500 nm reached extreme values of 3.63 and 2.25, respectively, with Angstrom Exponent (AE) above, indicating a strong dominance of fine-mode smoke particles. Spectral measurements of global-horizontal, direct-normal and diffuse-horizontal solar irradiance (300–1100 nm) show a pronounced attenuation of direct and global irradiances, particularly in the visible range, together with a strong enhancement of diffuse radiation. Relative to clean-sky conditions, daily global irradiance decreased by 21–27 %, while direct-normal irradiance was reduced by 72–99 %. Spectral aerosol radiative forcing and radiative forcing efficiency at the surface were quantified using radiative transfer simulations under pristine atmospheric conditions as a reference. The integrated spectral radiative forcing (300–1100 nm) for global irradiance reached -395 and -299 W m−2 on 17 and 18 August, respectively, indicating strong surface cooling dominated by scattering processes. Maximum forcing and efficiency occurred in the visible spectral range, consistent with the optical properties of freshly emitted smoke aerosols. At the same time, increases in the amount of present particles, equivalent black carbon (eBC) and greenhouse gases (CO2, CH4 and CO) confirm the direct influence of the wildfire plume on atmospheric composition at IZO. These observations provide one of the few detailed spectral assessments of surface radiative forcing by extreme biomass-burning aerosols at a high-altitude site and highlight the need to accurately represent fine-mode smoke aerosols in radiative transfer and climate models.
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Status: open (until 10 Mar 2026)
- RC1: 'Comment on egusphere-2026-306', Anonymous Referee #1, 23 Feb 2026 reply
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Reviewer comment on egusphere-2026-306 “Impact of Spectral Aerosol Radiative Forcing at the Izaña Observatory during the August 2023 Extreme Wildfires” by Garcia et a.
Reviewer recommendation: Accept with minor revisions
General comment:
The study by Garcia et al. captures a rare near-source wildfire event at a well-instrumented high-altitude observatory, providing valuable spectral radiative forcing data that is scarce in the literature. Du to the wide range of columnar, vertical, is situ aerosol and trace gas instrument at the Izaña Observatory (IZO) it is a comprehensive multi-instrument approach with rigorous methodology and significant results.
Specific comments
Missing aerosol absorption properties: The authors note (line 122) that AERONET inversion products (SSA, asymmetry parameter) were unavailable. This is a significant limitation since: SSA is crucial for distinguishing scattering vs. absorption effects. Without SSA, the conclusion that "scattering processes" dominate relies primarily on the positive diffuse forcing rather than direct measurement. Recommendation: Discuss this limitation more explicitly and consider whether MAAP absorption data could partially compensate
Limited temporal coverage: Analysis mostly focuses on two specific times (11:56 and 15:46 UTC). While understandable for detailed spectral analysis, a diurnal evolution of radiative forcing would strengthen the analysis. Recommendation: Consider adding a figure showing temporal evolution of integrated radiative forcing throughout the two days
The comparison between 17 and 18 August would probably benefit from an analysis of measurement variability during each event.
Minor comments:
Overall Assessment:
This is a valuable contribution documenting an extreme biomass burning event with rare spectral detail. The main scientific conclusions are sound, but the paper would benefit from a clearer discussion of limitations, particularly regarding missing SSA data. The multi-instrument approach is a major strength that validates the findings across independent measurement techniques. With the revisions outlined above the manuscript should be suitable for publication.