The effects of smoke and dust aerosols on UV-B radiation in Australia from ground-based and satellite measurements

Olga V. Kalashnikova; Franklin P. Mills; Annmarie Eldering; Don Anderson; Ross Mitchell

doi:10.1117/12.617443

12 September 2005 The effects of smoke and dust aerosols on UV-B radiation in Australia from ground-based and satellite measurements

Olga V. Kalashnikova, Franklin P. Mills, Annmarie Eldering, Don Anderson, Ross Mitchell

Author Affiliations +

Proceedings Volume 5886, Ultraviolet Ground- and Space-based Measurements, Models, and Effects V; 58860R (2005) https://doi.org/10.1117/12.617443
Event: Optics and Photonics 2005, 2005, San Diego, California, United States

Abstract

An understanding of the effect of aerosols on biologically- and photochemically-active UV radiation reaching the Earth's surface is important for many ongoing climate, biophysical, and air pollution studies. In particular, estimates of the UV characteristics of the most common Australian aerosols will be valuable inputs to UV Index forecasts, air quality studies, and assessments of the impact of regional environmental changes. Based on MODIS fire maps and MISR aerosol property retrievals, we have analyzed the climatological distributions of Australian dust and smoke particles and have identified sites where collocated ground-based UV-B and ozone measurements were available during episodes of relatively high aerosol activity. Since at least June 2003, overhead ozone and surface UV spectra (285-450 nm) have been measured routinely at Darwin and Alice Springs in Australia by the Australian Bureau of Meteorology (BoM). Using collocated AERONET sunphotometer measurements at Darwin and collocated BoM sunphotometer measurements at Darwin and Alice Springs, we identified several episodes of relatively high aerosol activity that could be used to study the effects of dust and smoke on the UV-B solar irradiance at the Earth's surface. To assess smoke effect we compared the measured UV irradiances at Darwin with irradiancies simulated with the LibRadtran radiative transfer model for aerosol-free conditions. We found that for otherwise similar atmospheric conditions, aerosols reduced the UVB irradiance by 50% near the fire source and up to 15% downwind. We also found the effect of smoke particles to be 5 to 10% larger in the UV-B part of the spectrum. For the selected period at Darwin, changes in the aerosol loadings gave larger variations in the surface UV irradiances than previously reported changes seen in the ozone column. We are continuing similar investigations for the Alice Springs site to assess spectral differences between smoke and dust aerosols.

Citation Download Citation

Olga V. Kalashnikova, Franklin P. Mills, Annmarie Eldering, Don Anderson, and Ross Mitchell "The effects of smoke and dust aerosols on UV-B radiation in Australia from ground-based and satellite measurements", Proc. SPIE 5886, Ultraviolet Ground- and Space-based Measurements, Models, and Effects V, 58860R (12 September 2005); https://doi.org/10.1117/12.617443

ACCESS THE FULL ARTICLE

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

;

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE