Net radiative effects of dust in the tropical North Atlantic based on integrated satellite observations and in situ measurements

In this study, we integrate recent in situ measurements with satellite retrievals of dust physical and radiative properties to quantify dust direct radiative effects on shortwave (SW) and longwave (LW) radiation (denoted as DRE SW and DRE LW , respectively) in the tropical North Atlantic during the...

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Bibliographic Details
Published in:Atmospheric Chemistry and Physics
Main Authors: Song, Qianqian, Zhang, Zhibo, Yu, Hongbin, Kato, Seiji, Yang, Ping, Colarco, Peter, Remer, Lorraine A., Ryder, Claire L.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/acp-18-11303-2018
https://www.atmos-chem-phys.net/18/11303/2018/
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Summary:In this study, we integrate recent in situ measurements with satellite retrievals of dust physical and radiative properties to quantify dust direct radiative effects on shortwave (SW) and longwave (LW) radiation (denoted as DRE SW and DRE LW , respectively) in the tropical North Atlantic during the summer months from 2007 to 2010. Through linear regression of the CERES-measured top-of-atmosphere (TOA) flux versus satellite aerosol optical depth (AOD) retrievals, we estimate the instantaneous DRE SW efficiency at the TOA to be <math xmlns="http://www.w3.org/1998/Math/MathML" id="M4" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">49.7</mn><mo>±</mo><mn mathvariant="normal">7.1</mn></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="58pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="a94bbb0d8cb5fdcbdd5b1f2762c588ec"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-18-11303-2018-ie00001.svg" width="58pt" height="10pt" src="acp-18-11303-2018-ie00001.png"/></svg:svg> W m −2 AOD −1 and <math xmlns="http://www.w3.org/1998/Math/MathML" id="M7" display="inline" overflow="scroll" dspmath="mathml"><mrow><mo>-</mo><mn mathvariant="normal">36.5</mn><mo>±</mo><mn mathvariant="normal">4.8</mn></mrow></math> <svg:svg xmlns:svg="http://www.w3.org/2000/svg" width="58pt" height="10pt" class="svg-formula" dspmath="mathimg" md5hash="21b020b4081686d3ee9d8906d0032ec7"><svg:image xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="acp-18-11303-2018-ie00002.svg" width="58pt" height="10pt" src="acp-18-11303-2018-ie00002.png"/></svg:svg> W m −2 AOD −1 based on AOD from MODIS and CALIOP, respectively. We then perform various sensitivity studies based on recent measurements of dust particle size distribution (PSD), refractive index, and particle shape distribution to determine how the dust microphysical and optical properties affect DRE estimates and its agreement with the above-mentioned satellite-derived DREs. Our analysis shows that a good agreement with the observation-based estimates of instantaneous DRE SW and DRE LW can be achieved through a combination of recently observed PSD with substantial presence of coarse particles, a less absorptive SW refractive index, and spheroid shapes. Based on this optimal combination of dust physical properties we further estimate the diurnal mean dust DRE SW in the region of −10 W m −2 at TOA and −26 W m −2 at the surface, respectively, of which ∼ 30 % is canceled out by the positive DRE LW . This yields a net DRE of about −6.9 and −18.3 W m −2 at TOA and the surface, respectively. Our study suggests that the LW flux contains useful information on dust particle size, which could be used together with SW observations to achieve a more holistic understanding of the dust radiative effect.