TY - JOUR
T1 - Classification of MODIS fire emission data based on aerosol absorption Angstrom exponent retrieved from AERONET data
AU - Ningombam, Shantikumar S.
AU - Khatri, Pradeep
AU - Larson, E. J.L.
AU - Dumka, Umesh Chandra
AU - Sarangi, Chandan
AU - Vineeth, R.
N1 - Funding Information:
The authors are thankful to the anonymous Reviewers for providing constructive comments which have improved the manuscript significantly. The AERONET data used in the present work are taken from 55 sites across the globe from the website: https://aeronet.gsfc.nasa.gov . The authors are thankful to the PI, Co-PIs and their staff of the respective AERONET sites who maintain the data for scientific use. We acknowledge the use of data products or imagery from the Land, Atmosphere Near real-time Capability for EOS (LANCE) system operated by the NASA/GSFC/Earth Science Data and Information System (ESDIS) with funding provided by NASA/HQ. We are also gratefully acknowledge all the team members of MEERA-2 for providing the data sets used in this work. SSN thanks the Ministry of Earth Sciences , Government of India for providing a financial support under the project grant number: MoES/16/02/2021-RDESS . CS acknowledges support from the New Faculty Initiation Grant (project number CE/20-21/065/NFIG/008961 ) and the use of the computing resources of HPC from Indian Institute of Technology Madras.
Funding Information:
The authors are thankful to the anonymous Reviewers for providing constructive comments which have improved the manuscript significantly. The AERONET data used in the present work are taken from 55 sites across the globe from the website: https://aeronet.gsfc.nasa.gov. The authors are thankful to the PI, Co-PIs and their staff of the respective AERONET sites who maintain the data for scientific use. We acknowledge the use of data products or imagery from the Land, Atmosphere Near real-time Capability for EOS (LANCE) system operated by the NASA/GSFC/Earth Science Data and Information System (ESDIS) with funding provided by NASA/HQ. We are also gratefully acknowledge all the team members of MEERA-2 for providing the data sets used in this work. SSN thanks the Ministry of Earth Sciences, Government of India for providing a financial support under the project grant number: MoES/16/02/2021-RDESS. CS acknowledges support from the New Faculty Initiation Grant (project number CE/20-21/065/NFIG/008961) and the use of the computing resources of HPC from Indian Institute of Technology Madras.
Publisher Copyright:
© 2022 Elsevier B.V.
PY - 2023/2/1
Y1 - 2023/2/1
N2 - Biomass burning emits a large quantity of gaseous pollutants and aerosols into the atmosphere, which perturbs the regional and global climate and has significant impacts on air quality and human health. In order to understand the temporal and spatial distributions of biomass burning and its contribution to aerosol optical and radiative impacts, we examined fire emission data and its contribution to aerosol optical and radiative impacts over six major hot-spot continents/sub-continents across the globe, namely North-Central (NC) Africa, South America, US-Hawaii, South Asia, South East Asia, and Australia-New Zealand, using long-term satellites, ground-based and re-analysis data during 2000–2021. The selected six sites contributed ∼70% of total global fire data. The classification of biomass burning, such as pre, active, and post burning phases, was performed based on the Absorption Angstrom Exponent (AAE) estimated from 55 AERONET (AErosol RObotic NETwork) stations. The study found the highest contribution of fire count (55 %) during the active burning phase followed by post (36 %) and pre (8 %) burning phases. Such high fire counts were associated with high absorption aerosol optical depth (AAOD) during the active fire event. Strong dominance of fine and coarse mode mixed aerosols were also observed during active and post fire regimes. High AAOD and low Extinction Angstrom Exponent (EAE) over NC Africa during the fire events suggested presence of mineral dust mixed with biomass burning aerosols. Brightness temperature, fire radiative power and fire count were also dominated by the active burning followed by post and pre burning phases. The maximum heating rate of 3.15 K day−1 was observed during the active fire events. The heating rate profile shows clear variations for three different fire regimes with the highest value of 1.80 K day−1 at ∼750 hPa altitude during the active fire event.
AB - Biomass burning emits a large quantity of gaseous pollutants and aerosols into the atmosphere, which perturbs the regional and global climate and has significant impacts on air quality and human health. In order to understand the temporal and spatial distributions of biomass burning and its contribution to aerosol optical and radiative impacts, we examined fire emission data and its contribution to aerosol optical and radiative impacts over six major hot-spot continents/sub-continents across the globe, namely North-Central (NC) Africa, South America, US-Hawaii, South Asia, South East Asia, and Australia-New Zealand, using long-term satellites, ground-based and re-analysis data during 2000–2021. The selected six sites contributed ∼70% of total global fire data. The classification of biomass burning, such as pre, active, and post burning phases, was performed based on the Absorption Angstrom Exponent (AAE) estimated from 55 AERONET (AErosol RObotic NETwork) stations. The study found the highest contribution of fire count (55 %) during the active burning phase followed by post (36 %) and pre (8 %) burning phases. Such high fire counts were associated with high absorption aerosol optical depth (AAOD) during the active fire event. Strong dominance of fine and coarse mode mixed aerosols were also observed during active and post fire regimes. High AAOD and low Extinction Angstrom Exponent (EAE) over NC Africa during the fire events suggested presence of mineral dust mixed with biomass burning aerosols. Brightness temperature, fire radiative power and fire count were also dominated by the active burning followed by post and pre burning phases. The maximum heating rate of 3.15 K day−1 was observed during the active fire events. The heating rate profile shows clear variations for three different fire regimes with the highest value of 1.80 K day−1 at ∼750 hPa altitude during the active fire event.
KW - Absorption angstrom exponent
KW - Aerosol optical depth
KW - Biomass burning
KW - Fire-radiative
KW - Heating rate
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U2 - 10.1016/j.scitotenv.2022.159898
DO - 10.1016/j.scitotenv.2022.159898
M3 - Article
C2 - 36343809
AN - SCOPUS:85141749900
SN - 0048-9697
VL - 858
JO - Science of the Total Environment
JF - Science of the Total Environment
M1 - 159898
ER -