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Ceilometer, sun photometer and ozonometer measurements of the aerosol optical depth, angstrom coefficients, water vapor and total ozone content over Sofia (Bulgaria)

机译:CeiLometer,Sun Photeter和Ozonometer测量气溶胶光学深度,埃菲亚(保加利亚)的羊杆系数,水蒸气和全臭氧含量

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This article presents the results of a study related to variations in aerosol optical depth, total ozone content, water vapor content and angstrom coefficients from three experimental campaigns carried out in June 2010, June 201 land June 2012 at three sites in the city of Sofia (Institute of Electronics, Astronomical Observatory in the Borisova Gradina Park and National Institute of Geophysics, Geodesy and Geography (NIGGG)). A ceilometer CHM15k, two sun photometers Microtops II and an automatic meteorological station were used during the experiments. The height of the mixing layer varied from 1500m to 2500 (3000)m during the measurements. The height of the residual layer ranged from 800m to 2000m. The stable boundary layer extended to 200-400m over the campaigns. The aerosol optical depth (AOD) at wavelength λ = 500nm ranged from 0.38 to 0.66 in the first campaign and from 0.24 to 0.55 in the second one and from 0.11 to 0.23 in the third one. Corresponding ranges for the water vapor content (WVC) were 1.26cm to 2.6cm. Different types of aerosol optical depth and water vapor content behavior were observed. Additional resource of information about the origin of the aerosol layers detected by the ceilometer CHM15k offered the HYSPLIT (HYbrid Single-Particle Lagrangian Integrated Trajectory) model. The calculations of backward air mass trajectories give a plot of the road that the air mass traversed for a chosen time period before to arrive to the location of Sofia city. The total ozone content (TOC) varied from 240 DU to 370 DU during the campaigns. The ground - based observation from ozonemeter Microtops II with satellite observation of Ozone Monitor Instruments (OMI) over Sofia (Bulgaria) are compared. Our results have implications for the further study of regional climate variability.
机译:本文介绍了与2010年6月在2010年6月,2012年6月2010年6月在2012年6月在索非亚市的三个地点进行的三个实验活动中进行的气溶胶光学深度的变化,总臭氧含量,水蒸气含量和抗埃系数的研究结果。博伊奥多瓦毕戈马公园和国家地球物理研究所的天文天文学研究所,大地测量和地理(Niggg))。在实验期间使用了天线仪CHM15K,两个太阳光度下微型电池II和自动气象站。在测量期间,混合层的高度在1500m至2500(3000)m中变化。残留层的高度范围为800米至2000米。稳定的边界层通过广告系列扩展到200-400M。波长λ= 500nm处的气溶胶光学深度(AOD)在第一个运动中的0.38至0.66范围为0.38至0.66,在第三个活动中的0.24至0.55次和0.11至0.23。水蒸气含量(WVC)的相应范围为1.26cm至2.6cm。观察到不同类型的气溶胶光学深度和水蒸气含量行为。 Ceilometer CHM15K检测到的气溶胶层的起源的额外资源提供了Hysplit(混合单粒子拉格朗日集成轨迹)模型。向后空气质量轨迹的计算给出了在索非亚城市的所选时间段的空气质量遍历的空气质量。在广告系列期间,总臭氧内容(TOC)从240 du到370 du不同。比较臭氧监测仪(OMI)卫星观察臭氧检测臭氧仪(保加利亚)的地面观察。我们的结果对区域气候变异性的进一步研究有影响。

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