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Long term characterization of aerosol optical properties: Implications for radiative forcing over the desert region of Jodhpur, India

机译:气溶胶光学特性的长期表征:对印度焦特布尔沙漠地区辐射强迫的影响

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AOT data for eight years period (2004-2012) using the MICROTOPS II Sun photometer has been used to study the wavelength dependent optical characteristics of aerosols over Jodhpur, situated in the desert region in NW India. The daily mean AOT at 500 nm for the present study period was 0.66 +/- 0.14 with an average Angstrom exponent as 0.71 +/- 0.20. Linear regression analysis of monthly AOT and Angstrom Exponent indicated an increasing trend of both. Seasonal variations of daily AOT and alpha as well as spectral dependence of seasonal mean AOT are presented. Diurnal variation of AOT and a in different season is studied. Impact of dust storm events on the aerosol characteristics over Jodhpur during the study period is studied. AOT values derived from MICROTOPS II were cross checked with Sun Sky Radiometer (Model POM-01, Prede Inc.) data for the period from May 2011 to April 2012 and were found to be in good agreement. Short wave aerosol radiative forcing (ARF) was computed for one year period of May 2011 to April 2012. Spectral variation of AOT, SSA and ASP showed more AOT and ASP during pre monsoon period when SSA was comparatively low; indicating towards more prevalence of coarse size absorbing dust in this period. The ARF at SUF and TOA was negative during all the seasons indicating dominance of scattering type aerosols mainly dust particles whereas that at ATM was positive in all the seasons indicating heating of the atmosphere, especially more during pre monsoon (+40.5 W/m(2)) than during rest of the year (+19.5 W/m(2)). A high degree of correlation between ARF at the SUF with AOT (R-2 = 0.94) indicated that ARF is a strong function of AOT. The radiative forcing efficiency inferred to scattering nature of aerosols at SUF (-4.2 W/m(2)/AOD) and TOA (-63.2 W/m(2)/AOD) indicating cooling at surface and top of the atmosphere whereas, there was warming of the atmosphere in between (+59 W/m(2)/AOD). The atmospheric heating rates varied from 0.49 K/day in post monsoon to 1.13 K/day in pre monsoon. This study has enabled us to understand the long term nature and physical characteristics of atmospheric aerosols over Jodhpur. (C) 2015 Elsevier Ltd. All rights reserved.
机译:使用MICROTOPS II太阳光度计的八年(2004-2012)的AOT数据已用于研究位于印度西北沙漠地区焦特布尔上空气溶胶的波长依赖性光学特性。在本研究期间,在500 nm处的日平均AOT为0.66 +/- 0.14,平均埃指数为0.71 +/- 0.20。每月AOT和Angstrom指数的线性回归分析表明两者均呈上升趋势。介绍了每日AOT和alpha的季节性变化以及季节性平均AOT的光谱依赖性。研究了不同季节AOT和a的日变化。在研究期间,研究了沙尘暴事件对焦特布尔上空气溶胶特征的影响。使用MICROTOPS II得出的AOT值与2011年5月至2012年4月期间的Sun Sky辐射计(型号POM-01,Prede Inc.)进行了交叉核对,发现结果吻合良好。计算了2011年5月至2012年4月的一年中的短波气溶胶辐射强迫(ARF)。AOT,SSA和ASP的光谱变化表明,在季风期间,SSA相对较低时,AOT和ASP有所增加。这表明在此期间,较普遍的是粗粒吸尘。 SUF和TOA的ARF在所有季节均为负值,表明散射型气溶胶主要是尘埃颗粒,而ATM的ARF在所有季节均为正值,表明大气变热,尤其是在季风之前(+40.5 W / m(2 )),而不是一年中的其余时间(+19.5 W / m(2))。 SUF处的ARF与AOT之间的高度相关性(R-2 = 0.94)表明ARF是AOT的强大功能。辐射强迫效率推断为SUF(-4.2 W / m(2)/ AOD)和TOA(-63.2 W / m(2)/ AOD)时气溶胶的散射性质,表明大气表面和顶部已经冷却,而那里大气温度在(+59 W / m(2)/ AOD)之间。大气加热速率从季风后的0.49 K /天到季风前的1.13 K /天不等。这项研究使我们能够了解焦特布尔上空气溶胶的长期性质和物理特征。 (C)2015 Elsevier Ltd.保留所有权利。

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