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AGU: Journal of Geophysical Research, Atmospheres

 

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  • Atmospheric Composition and Structure: Biosphere/atmosphere interactions
  • Atmospheric Composition and Structure: Chemical kinetic and photochemical properties
  • Atmospheric Composition and Structure: Constituent sources and sinks
  • Atmospheric Composition and Structure: Pollution—urban and regional
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Abstract
Cited By (45)
 

Abstract

Evolution of gases and particles from a savanna fire in South Africa

Peter V. Hobbs

Department of Atmospheric Sciences, University of Washington, Seattle, Washington, USA

Parikhit Sinha

Department of Atmospheric Sciences, University of Washington, Seattle, Washington, USA

Robert J. Yokelson

Department of Chemistry, University of Montana, Missoula, Montana, USA

Ted J. Christian

Department of Chemistry, University of Montana, Missoula, Montana, USA

Donald R. Blake

Department of Chemistry, University of California, Irvine, California, USA

Song Gao

Department of Chemistry, University of Washington, Seattle, Washington, USA

Thomas W. Kirchstetter

Lawrence Berkeley National Laboratory, Berkeley, California, USA

Tica Novakov

Lawrence Berkeley National Laboratory, Berkeley, California, USA

Peter Pilewskie

NASA Ames Research Center, Moffett Field, California, USA

Airborne measurements of particles and gases from a 1000-ha savanna fire in South Africa are presented. These measurements represent the most extensive data set reported on the aging of biomass smoke. The measurements include total concentrations of particles (CN), particle sizes, particulate organic carbon and black carbon, light-scattering coefficients, downwelling UV fluxes, and mixing ratios for 42 trace gases and 7 particulate species. The ratios of excess nitrate, ozone, and gaseous acetic acid to excess CO increased significantly as the smoke aged over ∼40–45 min, indicating that these species were formed by photochemistry in the plume. For 17 other species, the excess mixing ratio normalized by the excess mixing ratio of CO decreased significantly with smoke age. The relative rates of decrease for a number of chemical species imply that the average OH concentration in the plume was ∼1.7 × 107 molecules cm−3. Excess CN, normalized by excess CO, decreased rapidly during the first ∼5 min of aging, probably due to coagulation, and then increased, probably due to gas-to-particle conversion. The CO-normalized concentrations of particles <1.5 μm in diameter decreased, and particles >1.5 μm diameter increased, with smoke age. The spectral depletion of solar radiation by the smoke is depicted. The downwelling UV flux near the vertical center of the plume was about two-thirds of that near the top of the plume.

Published 8 March 2003.

Citation: Hobbs, P. V., P. Sinha, R. J. Yokelson, T. J. Christian, D. R. Blake, S. Gao, T. W. Kirchstetter, T. Novakov, and P. Pilewskie (2003), Evolution of gases and particles from a savanna fire in South Africa, J. Geophys. Res., 108(D13), 8485, doi:10.1029/2002JD002352.

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