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Solar eclipse induced changes in surface ozone at Ahmedabad

机译:日食引起艾哈迈达巴德表面臭氧的变化

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Measurements of surface ozone and related gases were made at Ahmedabad during the solar eclipse of 24 Oct. 1995. The maximum obscurity at Ahmedabad was 79.2%. The diurnal increase in ozone concentration due to photo-oxidation of pollutants like CO, CH_4 and non-methane hydrocarbons (NMHCs) observed on normal days after the sunrise was not observed until the time of maximum obscuration. In fact, there was a decrease in ozone concentration in the range of 18-21% at the maximum phase. Ozone levels were found to be lower even after the eclipse due to loss and delay in ozone production. The eclipse conditions were simulated in a photochemical box model which was used to calculate ozone changes. The model shows a decrease of ozone by about 16% as compared to a control day at the time of maximum obscuration. The model also shows significant role of boundary layer variations in the morning hours.
机译:1995年10月24日日蚀期间,在艾哈迈达巴德进行了表面臭氧和相关气体的测量。艾哈迈达巴德的最大暗度为79.2%。直到最大遮盖时间,才观察到在日出后的正常天中由于诸如CO,CH_4和非甲烷碳氢化合物(NMHCs)之类的污染物的光氧化而使臭氧浓度日增。实际上,在最大阶段,臭氧浓度降低了18-21%。即使在月食之后,由于臭氧的损失和延迟生产,也发现臭氧水平较低。在光化学箱模型中模拟日食条件,该模型用于计算臭氧变化。该模型显示,与最大遮盖时的控制日相比,臭氧减少了约16%。该模型还显示了边界层变化在早晨的重要作用。

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