Retrieval of aerosol single-scattering albedo and polarized phase function from polarized sun-photometer measurements for Zanjan's atmosphere
Open Access
Atmospheric
Measurement
Techniques
Atmos. Meas. Tech., 6, 2659–2669, 2013
www.atmos-meas-tech.net/6/2659/2013/
doi:10.5194/amt-6-2659-2013
© Author(s) 2013. CC Attribution 3.0 License.
Retrieval of aerosol single-scattering albedo and polarized phase
function from polarized sun-photometer measurements for Zanjan’s
atmosphere
A. Bayat1 , H. R. Khalesifard1,2 , and A. Masoumi3
1 Department of Physics, Institute for Advanced Studies in Basic Sciences (IASBS), Zanjan 45137-66731, Iran
2 Center for Climate Change and Global Warming, Institute for Advanced Studies in Basic Sciences (IASBS),
Zanjan 45137-66731, Iran
3 Department of Physics, Faculty of Sciences, University of Zanjan, Zanjan 45371-38791, Iran
Correspondence to: A. Bayat ()
Received: 14 March 2013 – Published in Atmos. Meas. Tech. Discuss.: 4 April 2013
Revised: 2 September 2013 – Accepted: 4 September 2013 – Published: 15 October 2013
Abstract. The polarized phase function of atmospheric
aerosols has been investigated for the atmosphere of Zanjan,
a city in northwest Iran. To do this, aerosol optical depth,
Ångström exponent, single-scattering albedo, and polarized
phase function have been retrieved from the measurements
of a Cimel CE 318-2 polarized sun-photometer from February 2010 to December 2012. The results show that the maximum value of aerosol polarized phase function as well as the
polarized phase function retrieved for a specific scattering
angle (i.e., 60◦ ) are strongly correlated (R = 0.95 and 0.95,
respectively) with the Ångström exponent. The latter has a
meaningful variation with respect to the changes in the complex refractive index of the atmospheric aerosols. Furthermore the polarized phase function shows a moderate negative correlation with respect to the atmospheric aerosol optical depth and single-scattering albedo (R = −0.76 and −0.33,
respectively). Therefore the polarized phase function can be
regarded as a key parameter to characterize the atmospheric
particles of the region – a populated city in the semi-arid area
and surrounded by some dust sources of the Earth’s dust belt.
1
Introduction
Physical and optical properties of the atmospheric aerosols
are from the major uncertainties in the global climate
changes (IPCC, 2007). In order to reduce the lack of extensive and reliable information about aerosols and their im-
pacts on atmosphere, they have been widely investigated
by ground-based measurements and satellite remote sensing suites (Heintzenberg et al., 1997; Kaufman et al., 2002).
Ground-based measurements are ideal for reliable and continuous derivation of local aerosol optical and physical properties due to negligible effects of surface background on the
measurements, and satellite measurements provide less accurate information about aerosols but in a global coverage
(Holben et al., 1998; Dubovik et al., 2002). Satellite remote
sensing and ground-based measurements are complementary
methods to study aerosols properties and their effects on
climate. They have been investigated by using active (e.g.,
spaceborne and ground-based lidars) (Bösenberg et al., 2003;
Winker et al., 2007) and passive (e.g., spaceborne spectrometers and ground-based sun-photometers) instruments (Holben et al., 1998; Prospero et al., 2002; Ginoux et al., 2012).
Iran is located within Earth’s so-called dust belt. Many
cities in the western, eastern, southern, and central parts of
this country have been subjected to dust events of different
strengths, especially during the recent years. Previous observations show that the Tigris–Euphrates basin in the west,
the Arabian Peninsula in the south and southwest, and the
arid region between the Caspian and Aral seas in the north
are the main external sources for the observed dust activities in this region (Prospero et al., 2002; Leon and Legrand,
2003; Goudie et al., 2006; Bayat et al., 2011; Abdi et al.,
2011, 2012; Sabetghadam et al., 2012; Masoumi et al., 2013).
There are also some minor active dust sources inside the
Published by Copernicus Publications on behalf of the European Geosciences Union.
2660
Iranian Plateau (Abdi et al., 2011, 2012; Masoumi et al.,
2013). Zanjan, a city in northwest Iran, is located in a mountainous region at 36.70◦ N, 48.51◦ E, and 1800 m above the
mean sea level (a.m.s.l). Based on the recordings of Zanjan’s
Meteorological office, the average of sunlight hours for this
city is more than 7 h per day (Samimi et al., 1997). Considering the geographical location as well as the climatological
conditions and lack of measured data for the region, groundbased measurements in this city provide valuable information
on the dust activities as well as aerosol types and their optical
and physical properties.
Aerosol classification using ground-based remote sensing
techniques can help to improve the estimation of aerosol radiative impact on climate and the accuracy of satellite retrievals (Dubovik et al., 2002; Cattrall et al., 2005; Giles
et al., 2012). Various methods based on aerosol optical and
physical properties have been used to classify different types
of aerosols from ground-based sun-photometer (SPM) measurements. The extinction of sunlight by aerosols when it
passes vertically through the atmosphere from the top of
the atmosphere to the surface is called the aerosol optical
depth (τa ). This parameter and its spectral dependence with
respect to wavelength (i.e., the Ångström exponent, α) are
the commonly used parameters to distinguish the dominant
aerosol types (e.g., Toledano et al., 2007; Kalapureddy et al.,
2009; Bayat et al., 2011; Boselli et al., 2012; Masoumi et al.,
2013). Studies (Gobbi et al., 2007; Basart et al., 2009) have
shown that the derivative of α or the spectral difference of
α-wavelength pairs together with τa and the particle’s effective radius can be used to infer different aerosol types.
In other works, variations of aerosol single-scattering albedo
(the ratio of scattering to extinction coefficients of particles,
ω0 ) with respect to their sizes have been used to distinguish
aerosol types (Omar et al., 2005; Mielonen et al., 2009; Lee
et al., 2010; Russell et al., 2010; Giles et al., 2012). As a
result of the mentioned methods, τa , α, ω0 , and size distributions retrieved from non-polarized measurements of SPM
are commonly used to categorize different types of aerosols,
but the polarization ones are mainly neglected.
Polarized sky radiance resulting from interaction between
sunlight and atmospheric particles strongly depends on the
presence of aerosols in the atmosphere, and can be monitored by looking at the aerosol polarized phase function,
qa (2) (Vermeulen et al., 2000; Li et al., 2004, 2006). The
qa (2) is indicative of the linear polarization of the scattered
light that has been generated by the atmospheric aerosols (Li
et al., 2004). Based on the relationship between the polarized sky radiance measured by SPM and its theoretical estimation from applying the Mie scattering theory, (...truncated)