Optical and chemical properties of aerosols transported to Mount Bachelor during spring 2010

We report on springtime 2010 observations of aerosol optical properties and size‐resolved elemental composition from Mount Bachelor Observatory (MBO; 2763 meters above sea level). Observations included multiwavelength aerosol scattering and absorption, made with a nephelometer and a particle soot ab...

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Published inJournal of Geophysical Research Vol. 116; no. D18
Main Authors Fischer, E. V., Perry, K. D., Jaffe, D. A.
Format Journal Article
LanguageEnglish
Published Washington Blackwell Publishing Ltd 27.09.2011
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Abstract We report on springtime 2010 observations of aerosol optical properties and size‐resolved elemental composition from Mount Bachelor Observatory (MBO; 2763 meters above sea level). Observations included multiwavelength aerosol scattering and absorption, made with a nephelometer and a particle soot absorption photometer, and size‐resolved composition, made using a rotating DRUM impactor with substrates analyzed by synchrotron X‐ray fluorescence. Our main tool for investigating variability in composition was empirical orthogonal function (EOF) analysis. In April, dust and sulfate explained 96% of the variance in the observed fine composition and accounted for the majority of the fine mode scattering. Three coincident Cloud‐Aerosol Lidar and Infrared Pathfinder Satellite Observation overpasses also identified aerosol layers classified as dust or polluted dust over MBO. Later in the spring, we deduce that organics and nitrate comprised more than 50% of the submicrometer aerosol mass. We used the EOF analysis to identify systematic relationships between composition and optical properties. We observed dust accompanied by anthropogenic pollutants including sulfate. When present, dust aerosol controlled ∼30% of the variability in the wavelength dependence of fine mode scattering. Many of the samples containing sulfate had absorption Ångstrom exponents near 1, suggesting black carbon was also present. Most of the sulfate was in the fine mode, but sulfate was also observed on coarse aerosols, and we inferred that much of the coarse sulfur was coated on the dust or had formed CaSO4 during transport. The relationships between Fe, Ca, Al, and Si observed at MBO were consistent with previous observations of Asian dust transported to North America. Key Points Tropospheric aerosol optical properties and chemistry are presented Dust and sulfate explained 96% of the variance in the spring fine composition Inorganic components account for 50%–100% of the aerosol scattering
AbstractList Tropospheric aerosol optical properties and chemistry are presented Dust and sulfate explained 96% of the variance in the spring fine composition Inorganic components account for 50%-100% of the aerosol scattering We report on springtime 2010 observations of aerosol optical properties and size-resolved elemental composition from Mount Bachelor Observatory (MBO; 2763 meters above sea level). Observations included multiwavelength aerosol scattering and absorption, made with a nephelometer and a particle soot absorption photometer, and size-resolved composition, made using a rotating DRUM impactor with substrates analyzed by synchrotron X-ray fluorescence. Our main tool for investigating variability in composition was empirical orthogonal function (EOF) analysis. In April, dust and sulfate explained 96% of the variance in the observed fine composition and accounted for the majority of the fine mode scattering. Three coincident Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation overpasses also identified aerosol layers classified as dust or polluted dust over MBO. Later in the spring, we deduce that organics and nitrate comprised more than 50% of the submicrometer aerosol mass. We used the EOF analysis to identify systematic relationships between composition and optical properties. We observed dust accompanied by anthropogenic pollutants including sulfate. When present, dust aerosol controlled ~30% of the variability in the wavelength dependence of fine mode scattering. Many of the samples containing sulfate had absorption Aangstrom exponents near 1, suggesting black carbon was also present. Most of the sulfate was in the fine mode, but sulfate was also observed on coarse aerosols, and we inferred that much of the coarse sulfur was coated on the dust or had formed CaSO4 during transport. The relationships between Fe, Ca, Al, and Si observed at MBO were consistent with previous observations of Asian dust transported to North America.
Tropospheric aerosol optical properties and chemistry are presented Dust and sulfate explained 96% of the variance in the spring fine composition Inorganic components account for 50%100% of the aerosol scattering We report on springtime 2010 observations of aerosol optical properties and size-resolved elemental composition from Mount Bachelor Observatory (MBO; 2763 meters above sea level). Observations included multiwavelength aerosol scattering and absorption, made with a nephelometer and a particle soot absorption photometer, and size-resolved composition, made using a rotating DRUM impactor with substrates analyzed by synchrotron X-ray fluorescence. Our main tool for investigating variability in composition was empirical orthogonal function (EOF) analysis. In April, dust and sulfate explained 96% of the variance in the observed fine composition and accounted for the majority of the fine mode scattering. Three coincident Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation overpasses also identified aerosol layers classified as dust or polluted dust over MBO. Later in the spring, we deduce that organics and nitrate comprised more than 50% of the submicrometer aerosol mass. We used the EOF analysis to identify systematic relationships between composition and optical properties. We observed dust accompanied by anthropogenic pollutants including sulfate. When present, dust aerosol controlled ~30% of the variability in the wavelength dependence of fine mode scattering. Many of the samples containing sulfate had absorption Ångstrom exponents near 1, suggesting black carbon was also present. Most of the sulfate was in the fine mode, but sulfate was also observed on coarse aerosols, and we inferred that much of the coarse sulfur was coated on the dust or had formed CaSO4 during transport. The relationships between Fe, Ca, Al, and Si observed at MBO were consistent with previous observations of Asian dust transported to North America.
We report on springtime 2010 observations of aerosol optical properties and size‐resolved elemental composition from Mount Bachelor Observatory (MBO; 2763 meters above sea level). Observations included multiwavelength aerosol scattering and absorption, made with a nephelometer and a particle soot absorption photometer, and size‐resolved composition, made using a rotating DRUM impactor with substrates analyzed by synchrotron X‐ray fluorescence. Our main tool for investigating variability in composition was empirical orthogonal function (EOF) analysis. In April, dust and sulfate explained 96% of the variance in the observed fine composition and accounted for the majority of the fine mode scattering. Three coincident Cloud‐Aerosol Lidar and Infrared Pathfinder Satellite Observation overpasses also identified aerosol layers classified as dust or polluted dust over MBO. Later in the spring, we deduce that organics and nitrate comprised more than 50% of the submicrometer aerosol mass. We used the EOF analysis to identify systematic relationships between composition and optical properties. We observed dust accompanied by anthropogenic pollutants including sulfate. When present, dust aerosol controlled ∼30% of the variability in the wavelength dependence of fine mode scattering. Many of the samples containing sulfate had absorption Ångstrom exponents near 1, suggesting black carbon was also present. Most of the sulfate was in the fine mode, but sulfate was also observed on coarse aerosols, and we inferred that much of the coarse sulfur was coated on the dust or had formed CaSO4 during transport. The relationships between Fe, Ca, Al, and Si observed at MBO were consistent with previous observations of Asian dust transported to North America. Key Points Tropospheric aerosol optical properties and chemistry are presented Dust and sulfate explained 96% of the variance in the spring fine composition Inorganic components account for 50%–100% of the aerosol scattering
ArticleNumber D18202
Author Jaffe, D. A.
Fischer, E. V.
Perry, K. D.
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Snippet We report on springtime 2010 observations of aerosol optical properties and size‐resolved elemental composition from Mount Bachelor Observatory (MBO; 2763...
Tropospheric aerosol optical properties and chemistry are presented Dust and sulfate explained 96% of the variance in the spring fine composition Inorganic...
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crossref
wiley
istex
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Publisher
SubjectTerms Absorption
aerosol chemistry
aerosol optical properties
Aerosols
Air pollution
Anthropogenic factors
Atmospheric aerosols
Atmospheric sciences
Black carbon
Chemical composition
Chemical properties
Dust
Geochemistry
Geophysics
Lidar
long-range transport
Optical properties
Photometers
Sulfates
Sulfur
X-ray fluorescence
Title Optical and chemical properties of aerosols transported to Mount Bachelor during spring 2010
URI https://api.istex.fr/ark:/67375/WNG-446QKM81-T/fulltext.pdf
https://onlinelibrary.wiley.com/doi/abs/10.1029%2F2011JD015932
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