Abstract

Abstract. The multiannual global mean of aerosol optical depth at 550 nm (AOD550) over land is ∼ 0.19, and that over oceans is ∼ 0.13. About 45 % of the Earth surface shows AOD550 smaller than 0.1. There is a need for measurement techniques that are optimized to measure aerosol optical properties under low AOD conditions. We present an inherently calibrated retrieval (i.e., no need for radiance calibration) to simultaneously measure AOD and the aerosol phase function parameter, g, based on measurements of azimuth distributions of the Raman scattering probability (RSP), the near-absolute rotational Raman scattering (RRS) intensity. We employ radiative transfer model simulations to show that for solar azimuth RSP measurements at solar elevation and solar zenith angle (SZA) smaller than 80°, RSP is insensitive to the vertical distribution of aerosols and maximally sensitive to changes in AOD and g under near-molecular scattering conditions. The University of Colorado two-dimensional Multi-AXis Differential Optical Absorption Spectroscopy (CU 2-D-MAX-DOAS) instrument was deployed as part of the Two Column Aerosol Project (TCAP) at Cape Cod, MA, during the summer of 2012 to measure direct sun spectra and RSP from scattered light spectra at solar relative azimuth angles (SRAAs) between 5 and 170°. During two case study days with (1) high aerosol load (17 July, 0.3 < AOD430 < 0.6) and (2) near-molecular scattering conditions (22 July, AOD430 < 0.13) we compare RSP-based retrievals of AOD430 and g with data from a co-located CIMEL sun photometer, Multi-Filter Rotating Shadowband Radiometer (MFRSR), and an airborne High Spectral Resolution Lidar (HSRL-2). The average difference (relative to DOAS) for AOD430 is +0.012 ± 0.023 (CIMEL), −0.012 ± 0.024 (MFRSR), −0.011 ± 0.014 (HSRL-2), and +0.023 ± 0.013 (CIMELAOD − MFRSRAOD) and yields the following expressions for correlations between different instruments: DOASAOD = −(0.019 ± 0.006) + (1.03 ± 0.02) × CIMELAOD (R2 = 0.98), DOASAOD = −(0.006 ± 0.005) + (1.08 ± 0.02) × MFRSRAOD (R2 = 0.98), and CIMELAOD = (0.013 ± 0.004) + (1.05 ± 0.01) × MFRSRAOD (R2 = 0.99). The average g measured by DOAS on both days was 0.66 ± 0.03, with a difference of 0.014 ± 0.05 compared to CIMEL. Active steps to minimize the error in the RSP help to reduce the uncertainty in retrievals of AOD and g. As AOD decreases and SZA increases, the RSP signal-to-noise ratio increases. At AOD430 ∼ 0.4 and 0.10 the absolute AOD errors are ∼ 0.014 and 0.003 at 70° SZA and 0.02 and 0.004 at 35° SZA. Inherently calibrated, precise AOD and g measurements are useful to better characterize the aerosol direct effect in urban polluted and remote pristine environments.

Highlights

  • Atmospheric aerosol particles play a key role in the energy balance of Earth’s atmosphere (IPCC, 2013)

  • In order to assess the Raman scattering probability (RSP) contribution in the direct sun spectra we use three different approaches: (1) a Langley plot type method, where the differential RSP (dRSP) obtained with direct sun spectra as reference spectrum is plotted as a function of the solar zenith angle (SZA); (2) by interpolating the dRSP measured with small solar relative azimuth angles (SRAAs) to the 0◦; and (3) from RTM simulations

  • The extrapolation to air mass factor (AMF) = 0 yields the absolute value of the RSP contained in the reference spectrum (RSP value if there were no atmosphere), which is determined as 0.0053 ± 0.0007 by this method

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Summary

Introduction

Atmospheric aerosol particles play a key role in the energy balance of Earth’s atmosphere (IPCC, 2013). McComiskey et al (2008) studied the sensitivity of aerosol direct radiative forcing using representative uncertainties in currently established methods to measure aerosol optical properties. For a typical AOD uncertainty of 0.01 (best case scenario expected for newly calibrated ground-based radiometric instrument in the visible spectra range; Eck et al, 1999; Holben et al, 1998), the error in the aerosol direct forcing is about 0.6 W m−2 (top of the atmosphere) and 1.3 W m−2 (surface) for a solar zenith angle (SZA) of 45◦ (McComiskey et al, 2008). Low AOD conditions are projected to be more prevalent in the future (Westervelt et al, 2015) Under these conditions, measurements of AOD with higher accuracy and precision are even more desirable

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