期刊
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
卷 193, 期 -, 页码 -出版社
PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.jastp.2019.105061
关键词
Solar radiation; Aerosols; Haze/foggy; Dust; Radiative effect
Short-wave incoming solar radiation and aerosol optical characteristics were examined at New Delhi, in the western Indo-Gangetic Basin (IGB) for the period from March 2010 to June 2012 to understand their possible association in different sky conditions along with their radiative implications. During the study period, solar radiation varied between 65 and 624 Wm(-2), with a seasonal mean of 419 +/- 34, 328 +/- 32, 308 +/- 54 and 306. 56 Wm(-2), respectively in the summer, monsoon, post-monsoon and winter periods. Inter-annually, the magnitude of solar radiation was similar to 19% and 23% higher during 2012 as compared to 2011 and 2010. Aerosol optical Depth (AOD) varied between 0.11 and 2.4 (mean: 0.69 +/- 0.38) whereas Angstr_om Exponent (AE) was between 0.46 and 1.81 (mean: 0.8 +/- 0.28) during the entire study period. The solar radiation was found to be significantly correlated with the AOD (R = -0.22) and AE (R = -0.45). The mean characteristics of solar radiation and aerosol optical parameters were found to differ significantly in different sky conditions, which were used to examine their possible implications to direct radiative effect (DRE). The DRE at the surface was as high as about -19 W m(-2) during clear sky day, which was similar to 16 and 48 W m(-2) higher than that of haze/foggy and dusty days, respectively.
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