Physics
Scientific paper
Feb 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007georl..3403818n&link_type=abstract
Geophysical Research Letters, Volume 34, Issue 3, CiteID L03818
Physics
10
Atmospheric Composition And Structure: Troposphere: Composition And Chemistry, Atmospheric Composition And Structure: Aerosols And Particles (0345, 4801, 4906), Global Change: Atmosphere (0315, 0325)
Scientific paper
Biomass burning is a major source of air pollutants, some of which are also climate forcing agents. We investigate the sensitivity of direct radiative forcing due to tropospheric ozone and aerosols (carbonaceous and sulfate) to a marginal reduction in their (or their precursor) emissions from major biomass burning regions. We find that the largest negative global forcing is for 10% emission reductions in tropical regions, including Africa (-4.1 mWm-2 from gas and -4.1 mWm-2 from aerosols), and South America (-3.0 mWm-2 from gas and -2.8 mWm-2 from aerosols). We estimate that a unit reduction in the amount of biomass burned in India produces the largest negative ozone and aerosol forcing. Our analysis indicates that reducing biomass burning emissions causes negative global radiative forcing due to ozone and aerosols; however, regional differences need to be considered when evaluating controls on biomass burning to mitigate global climate change.
Horowitz Larry W.
Mauzerall Denise L.
Naik Vaishali
Oppenheimer Michael
Ramaswamy Venkatachalam
No associations
LandOfFree
On the sensitivity of radiative forcing from biomass burning aerosols and ozone to emission location does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the sensitivity of radiative forcing from biomass burning aerosols and ozone to emission location, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the sensitivity of radiative forcing from biomass burning aerosols and ozone to emission location will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-739807