TY - JOUR
T1 - Case study of absorption aerosol optical depth closure of black carbon over the East China Sea
AU - Koike, M.
AU - Moteki, N.
AU - Khatri, P.
AU - Takamura, T.
AU - Takegawa, N.
AU - Kondo, Y.
AU - Hashioka, H.
AU - Matsui, H.
AU - Shimizu, A.
AU - Sugimoto, N.
N1 - Funding Information:
We are indebted to all A-FORCE participants for their cooperation and support. Special thanks are due to the flight and ground crews of the DAS King Air aircraft for helping make this effort a success. We thank Ikuyo Oshima for her contributions to the data analyses. We also thank Kouji Adachi at the Meteorological Research Institute, Japan, for providing electron tomography information of BC and useful comments. We also thank Yugo Kanaya at the Japan Agency for Marine-Earth Science and Technology (JAMSTEC) for providing COSMOS BC data and Teruyuki Nakajima at the Atmosphere and Ocean Research Institute, University of Tokyo, for his useful comments and suggestions. This study was supported by the Ministry of Education, Culture, Sports, Science, and Technology (MEXT) in Japan (Grant-in-Aid for Scientific Research (S) and GRENE Arctic Climate Change Research Project), the strategic international cooperative program of the Japan Science and Technology Agency (JST), and the global environment research fund of the Japanese Ministry of the Environment (2A-1101).
Publisher Copyright:
© 2013. American Geophysical Union. All rights reserved.
PY - 2014/1/16
Y1 - 2014/1/16
N2 - Absorption aerosol optical depth (AAOD) measurements made by sun-sky photometers are currently the only constraint available for estimates of the global radiative forcing of black carbon (BC), but their validation studies are limited. In this paper, we report the first attempt to compare AAODs derived from single-particle soot photometer (SP2) and ground-based sun-sky photometer (sky radiometer, SKYNET) measurements. During the Aerosol Radiative Forcing in East Asia (A-FORCE) experiments, BC size distribution and mixing state vertical profiles were measured using an SP2 on board a research aircraft near the Fukue Observatory (32.8°N, 128.7°E) over the East China Sea in spring 2009 and late winter 2013. The aerosol extinction coefficients (bext) and single scattering albedo (SSA) at 500 nm were calculated based on aerosol size distribution and detailed BC mixing state information. The calculated aerosol optical depth (AOD) agreed well with the sky radiometer measurements (2 ± 6%) when dust loadings were low (lidar-derived nonspherical particle contribution to AOD less than 20%). However, under these low-dust conditions, the AAODs obtained from sky radiometer measurements were only half of the in situ estimates. When dust loadings were high, the sky radiometer measurements showed systematically higher AAODs even when all coarse particles were assumed to be dust for in situ measurements. These results indicate that there are considerable uncertainties in AAOD measurements. Uncertainties in the BC refractive index, optical calculations from in situ data, and sky radiometer retrieval analyses are discussed.
AB - Absorption aerosol optical depth (AAOD) measurements made by sun-sky photometers are currently the only constraint available for estimates of the global radiative forcing of black carbon (BC), but their validation studies are limited. In this paper, we report the first attempt to compare AAODs derived from single-particle soot photometer (SP2) and ground-based sun-sky photometer (sky radiometer, SKYNET) measurements. During the Aerosol Radiative Forcing in East Asia (A-FORCE) experiments, BC size distribution and mixing state vertical profiles were measured using an SP2 on board a research aircraft near the Fukue Observatory (32.8°N, 128.7°E) over the East China Sea in spring 2009 and late winter 2013. The aerosol extinction coefficients (bext) and single scattering albedo (SSA) at 500 nm were calculated based on aerosol size distribution and detailed BC mixing state information. The calculated aerosol optical depth (AOD) agreed well with the sky radiometer measurements (2 ± 6%) when dust loadings were low (lidar-derived nonspherical particle contribution to AOD less than 20%). However, under these low-dust conditions, the AAODs obtained from sky radiometer measurements were only half of the in situ estimates. When dust loadings were high, the sky radiometer measurements showed systematically higher AAODs even when all coarse particles were assumed to be dust for in situ measurements. These results indicate that there are considerable uncertainties in AAOD measurements. Uncertainties in the BC refractive index, optical calculations from in situ data, and sky radiometer retrieval analyses are discussed.
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U2 - 10.1002/2013JD020163
DO - 10.1002/2013JD020163
M3 - Article
AN - SCOPUS:84893975087
VL - 119
SP - 122
EP - 136
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
SN - 0148-0227
IS - 1
ER -