{"title":"Comparison of Ozone Amounts Measured at Delhi (28I/2°N), Srinagar (34°N) and Tateno (36°N) in 1957~58","authors":"R., N. Kulkarni, P. Angreji, K. Ramanathan","doi":"10.2467/mripapers1950.10.2_85","DOIUrl":null,"url":null,"abstract":"A new ozone station was established in Kashmir (34°N) in 1955 in a region where double tropopauses are frequent in winter and spring. In this paper, a comparison is made of the ozone amounts measured at Delhi (281/2°N) and Srinagar (34°N) in India and at Tateno (36°N) in Japan in 1957-58. The ozone amounts at Tateno are much larger than at Srinagar although the latitude of Tateno is only 2° greater than that of Srinagar. It is recalled that at Zi-Ka-Wei and Cairo, which are at lower latitndes than Srinagar, significantly higher ozone values had been recorded in winter. It is thus evident that there is a large geographical influence on the total ozone amount measured at a place. Apparently, the Himalayas and the Indian summer monsoon exert a strong depressing influence on the ozone amount south of the Himalayas and incursions of the cold Siberian anti-cyclone tend to bring with it larger amounts of ozone over China and Japan. The seasonal variation of ozone over N. India was of an unusual character in 1957. A summary of the results of the ozone measurements made in India prior to 1954 was given by RAMANATHAN (1954) at the Rome Meeting of the International Association of Meteorology. The day-to-day variations of ozone are small during most of the year and surface weather conditions do not seem to affect them. In December to April, however, there are significant variations of ozone over Mt. Abu and New Delhi, this being the period when active western disturbances move across N. India. The transition from the autumn minimum of ozone to the comparatively high values in winter and spring takes place in a succession of surges, the first surge approximately coinciding with the onset of strong upper westerlies over N. India. Some pronounced surges are associated with the passage of deep troughs of low pressure at 6 and 9 km. The rise of ozone during a surge takes place when northwesterly winds are replacing the southwesterlies, but once the northwesterlies get settled, the ozone amount begins to fall. However, ozone fluctuations could not be * Paper presented at the International Ozone Symposium at Oxford in July 1959. 86R. N. Kulkarni, P. D. Angreji and K. R. Ramanathan Vol. X No. 2 explained in terms of shifts in wind direction at pilot balloon levels. Middle latitude variations of ozone associated with waves in the upper atmosphere are observable even at latitudes down to 20°N in winter and spring. The association of ozone changes with western disturbances was confirmed from later observations made at Delhi, Mt. Abu and Quetta. Since 1955, observations on the total amount of ozone and its vertical distribution have been made at Srinagar (34°N) at a latitude where double tropopauses are frequent. An ozone observing station was established at Srinagar in May 1955 by transferring a DOBSON'S spectrophotometer there. The optical wedges of the spectrophotometer were recalibrated and the constants determined. Frequent checks of calibration were made in the subsequent period. The present paper contains a summary of the results of the ozone observations so far analysed. It was decided to use the afternoon ozone amounts observed on the wavelength pair 3114/3324 (CC') for the present study. The ozone values were calculated and corrected for haze in the manner suggested by RAMANATHAN and KARANDIKAR (1949) . All the ozone values have been converted to VIGROUX'S level of ozone absorption coefficient a for uniformity. 1. Day-to-day variation of ozone In Fig. 1 the daily ozone values over three Indian stations, Mt. Abu (24°N), New Delhi (28V2°N) and Srinagar (34°N) for the year 1957-58 are given. The daily ozone amounts over Tateno (36°N) (1957-58) in Japan have also been included in the diagram. 1959 Comparison of Ozone Amounts Measured in 1957-58 87 A striking feature of this diagram is that although the latitude of Tateno differs only by 2° from that of Srinagar, the ozone values over Tateno are much higher than those over Srinagar in the winter and spring months. The fluctuations in the ozone content over Tateno are also markedly larger than those over Srinagar. In August to October, however, the ozone content over Tateno is only a little larger than that over the north Indian stations. The Tateno ozone starts separating from the Indian values in December and the difference increases rapidly. 2. Seasonal variation of ozone Fig. 2 gives the ten-day mean ozone values at Tateno, Srinagar, New Delhi and Mt. Abu from July 1955 to December 1958. (1) In general, the seasonal variation conforms to the normal variation appropriate to middle latitudes with maxima in winter and spring and minima in summer","PeriodicalId":39821,"journal":{"name":"Papers in Meteorology and Geophysics","volume":"1 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2012-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.2467/mripapers1950.10.2_85","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Papers in Meteorology and Geophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.2467/mripapers1950.10.2_85","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Earth and Planetary Sciences","Score":null,"Total":0}
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Abstract
A new ozone station was established in Kashmir (34°N) in 1955 in a region where double tropopauses are frequent in winter and spring. In this paper, a comparison is made of the ozone amounts measured at Delhi (281/2°N) and Srinagar (34°N) in India and at Tateno (36°N) in Japan in 1957-58. The ozone amounts at Tateno are much larger than at Srinagar although the latitude of Tateno is only 2° greater than that of Srinagar. It is recalled that at Zi-Ka-Wei and Cairo, which are at lower latitndes than Srinagar, significantly higher ozone values had been recorded in winter. It is thus evident that there is a large geographical influence on the total ozone amount measured at a place. Apparently, the Himalayas and the Indian summer monsoon exert a strong depressing influence on the ozone amount south of the Himalayas and incursions of the cold Siberian anti-cyclone tend to bring with it larger amounts of ozone over China and Japan. The seasonal variation of ozone over N. India was of an unusual character in 1957. A summary of the results of the ozone measurements made in India prior to 1954 was given by RAMANATHAN (1954) at the Rome Meeting of the International Association of Meteorology. The day-to-day variations of ozone are small during most of the year and surface weather conditions do not seem to affect them. In December to April, however, there are significant variations of ozone over Mt. Abu and New Delhi, this being the period when active western disturbances move across N. India. The transition from the autumn minimum of ozone to the comparatively high values in winter and spring takes place in a succession of surges, the first surge approximately coinciding with the onset of strong upper westerlies over N. India. Some pronounced surges are associated with the passage of deep troughs of low pressure at 6 and 9 km. The rise of ozone during a surge takes place when northwesterly winds are replacing the southwesterlies, but once the northwesterlies get settled, the ozone amount begins to fall. However, ozone fluctuations could not be * Paper presented at the International Ozone Symposium at Oxford in July 1959. 86R. N. Kulkarni, P. D. Angreji and K. R. Ramanathan Vol. X No. 2 explained in terms of shifts in wind direction at pilot balloon levels. Middle latitude variations of ozone associated with waves in the upper atmosphere are observable even at latitudes down to 20°N in winter and spring. The association of ozone changes with western disturbances was confirmed from later observations made at Delhi, Mt. Abu and Quetta. Since 1955, observations on the total amount of ozone and its vertical distribution have been made at Srinagar (34°N) at a latitude where double tropopauses are frequent. An ozone observing station was established at Srinagar in May 1955 by transferring a DOBSON'S spectrophotometer there. The optical wedges of the spectrophotometer were recalibrated and the constants determined. Frequent checks of calibration were made in the subsequent period. The present paper contains a summary of the results of the ozone observations so far analysed. It was decided to use the afternoon ozone amounts observed on the wavelength pair 3114/3324 (CC') for the present study. The ozone values were calculated and corrected for haze in the manner suggested by RAMANATHAN and KARANDIKAR (1949) . All the ozone values have been converted to VIGROUX'S level of ozone absorption coefficient a for uniformity. 1. Day-to-day variation of ozone In Fig. 1 the daily ozone values over three Indian stations, Mt. Abu (24°N), New Delhi (28V2°N) and Srinagar (34°N) for the year 1957-58 are given. The daily ozone amounts over Tateno (36°N) (1957-58) in Japan have also been included in the diagram. 1959 Comparison of Ozone Amounts Measured in 1957-58 87 A striking feature of this diagram is that although the latitude of Tateno differs only by 2° from that of Srinagar, the ozone values over Tateno are much higher than those over Srinagar in the winter and spring months. The fluctuations in the ozone content over Tateno are also markedly larger than those over Srinagar. In August to October, however, the ozone content over Tateno is only a little larger than that over the north Indian stations. The Tateno ozone starts separating from the Indian values in December and the difference increases rapidly. 2. Seasonal variation of ozone Fig. 2 gives the ten-day mean ozone values at Tateno, Srinagar, New Delhi and Mt. Abu from July 1955 to December 1958. (1) In general, the seasonal variation conforms to the normal variation appropriate to middle latitudes with maxima in winter and spring and minima in summer
1955年在冬季和春季双对流层频繁出现的克什米尔(34°N)地区建立了一个新的臭氧站。本文比较了1957- 1958年印度德里(281/2°N)和斯利那加(34°N)和日本馆野(36°N)的臭氧量。Tateno的臭氧量比斯利那加大得多,尽管它的纬度只比斯利那加大2°。回顾,在比斯利那加纬度低的梓嘉卫和开罗,冬季记录到的臭氧值明显较高。由此可见,一个地方所测得的臭氧总量受地理因素的影响很大。显然,喜马拉雅山和印度夏季风对喜马拉雅山以南的臭氧量有很强的抑制作用,而寒冷的西伯利亚反气旋的入侵往往会带来中国和日本上空更大的臭氧量。1957年印度北部上空臭氧的季节变化具有不寻常的特征。RAMANATHAN(1954)在国际气象协会罗马会议上总结了1954年以前在印度进行的臭氧测量结果。在一年中的大部分时间里,臭氧的日常变化很小,地表天气条件似乎对它们没有影响。然而,在12月至4月,在阿布山和新德里上空的臭氧有显著的变化,这是活跃的西方扰动穿过印度北部的时期。臭氧从秋季最小值到冬季和春季相对较高值的转变发生在一连串的浪涌中,第一次浪涌大约与印度北部强高空西风带的出现一致。一些明显的浪涌与6公里和9公里处的低压槽通过有关。当西北风取代西南风时,臭氧量就会上升,但一旦西北风稳定下来,臭氧量就会开始下降。1959年7月在牛津举行的国际臭氧研讨会上发表的论文。86 r。N. Kulkarni, P. D. Angreji和K. R. Ramanathan在第X卷第2卷中解释了引航气球高度风向的变化。在冬季和春季,即使在低至20°N的纬度地区,也可观测到与高层大气波有关的臭氧中纬度变化。后来在德里、阿布山和奎达进行的观测证实了臭氧变化与西方扰动的联系。自1955年以来,在斯利那加(34°N)这个双对流层频繁出现的纬度,对臭氧总量及其垂直分布进行了观测。1955年5月,在斯利那加建立了一个臭氧观测站,将多布森分光光度计转移到那里。重新校准了分光光度计的光楔并测定了常数。在随后的一段时间里,经常检查校准。本文载有迄今分析的臭氧观测结果的摘要。决定在本研究中使用在波长对3114/3324 (CC’)上观测到的下午臭氧量。臭氧值是按照RAMANATHAN和KARANDIKAR(1949)提出的方法计算和校正的。为了均匀起见,所有臭氧值都转换为VIGROUX的臭氧吸收系数a水平。1. 图1给出了1957- 1958年印度三个站点的日臭氧值,分别是阿布山(24°N)、新德里(28V2°N)和斯利那加(34°N)。图中还包括了日本馆野(36°N)上空1957- 1958年的日臭氧量。1959年1957- 1958年臭氧量的比较87该图的一个显著特征是,尽管Tateno的纬度与斯利那加的纬度只相差2°,但在冬季和春季,Tateno的臭氧值远高于斯利那加。Tateno上空臭氧含量的波动也明显大于斯利那加上空。然而,8月至10月,馆野上空的臭氧含量仅略高于印度北部监测站。12月,馆野臭氧开始与印度值分离,差异迅速扩大。2. 图2为1955年7月至1958年12月在泰特诺、斯利那加、新德里和阿布山的10天平均臭氧值。(1)总体上,季节变化符合适合中纬度地区的正常变化规律,冬春季最大,夏季最小