Application of satellite and ground-based data to investigate the UV radiative effects of Australian aerosols

dc.contributor.authorKalashnikova, Olga V
dc.contributor.authorMills, Franklin
dc.contributor.authorEldering, Annmarie
dc.contributor.authorAnderson, Don
dc.date.accessioned2015-12-08T22:37:10Z
dc.date.issued2007
dc.date.updated2015-12-08T09:55:31Z
dc.description.abstractAn 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. By analyzing climatological distributions of Australian aerosols we have identified sites where co-located ground-based UV-B and ozone measurements were available during episodes of relatively high aerosol activity. Since at least June 2003, surface UV global irradiance spectra (285-450 nm) have been measured routinely at Darwin and Alice Springs in Australia by the Australian Bureau of Meteorology (BoM). Using co-located sunphotometer measurements at Darwin and Alice Springs, we identified several episodes of relatively high aerosol activity. Aerosol air mass types were analyzed from sunphotometer-derived angstrom parameter, MODIS fire maps and MISR aerosol property retrievals. To assess aerosol effects we compared the measured UV irradiances for aerosol-loaded and clear-sky conditions with each other and with irradiances simulated using the libRadtran radiative transfer model for aerosol-free conditions. We found that for otherwise similar atmospheric conditions, smoke aerosols over Darwin reduced the surface UV irradiance by as much as 40-50% at 290-300 nm and 20-25% at 320-400 nm near active fires (aerosol optical depth, AOD, at 500 nm ∼ 0.6). Downwind of fires, the smoke aerosols over Darwin reduced the surface irradiance by 15-25% at 290-300 nm and ∼ 10% at 320-350 nm (AOD at 500 nm ∼ 0.2). The effect of smoke increased with decrease of wavelength and is strongest in the UV-B. The aerosol attenuation factors calculated for the selected cases suggest smoke over Darwin has an effect on surface 340-380 nm irradiances that is comparable to that produced by smoke over Sub-Saharan Africa. Dust activity was very low at Alice Springs during 2004, therefore we were not able to identify strong dust events to fully assess the UV effect of dust. For the cases studied, smoke aerosols seem to produce a stronger reduction in surface UV irradiances than dust aerosols.
dc.identifier.issn0034-4257
dc.identifier.urihttp://hdl.handle.net/1885/35417
dc.publisherElsevier
dc.sourceRemote Sensing of Environment
dc.subjectKeywords: Air pollution; Air quality; Climate change; Data reduction; Earth (planet); Ultraviolet radiation; Weather satellites; Australian aerosols; Climatological distributions; MISR; MODIS; Radiative transfer; UV surface irradiances; Aerosols; aerosol; dust; env Australian aerosols; MISR; MODIS; UV surface irradiances
dc.titleApplication of satellite and ground-based data to investigate the UV radiative effects of Australian aerosols
dc.typeJournal article
local.bibliographicCitation.lastpage80
local.bibliographicCitation.startpage65
local.contributor.affiliationKalashnikova, Olga V, California Institute of Technology
local.contributor.affiliationMills, Franklin, College of Medicine, Biology and Environment, ANU
local.contributor.affiliationEldering, Annmarie, California Institute of Technology Jet Propulsion Laboratory
local.contributor.affiliationAnderson, Don, Bureau of Meteorology
local.contributor.authoruidMills, Franklin, u4064907
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020201 - Atomic and Molecular Physics
local.identifier.ariespublicationu4169254xPUB124
local.identifier.citationvolume107
local.identifier.doi10.1016/j.rse.2006.07.025
local.identifier.scopusID2-s2.0-33846940935
local.type.statusPublished Version

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