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1.
Summary The correlation matrix for the vertical ozone distribution and the temperature-ozone cross-correlation matrix, which was calculated from ozone soundings made over Berlin between 1967 and 1970, the statistical structure of the vertical ozone profile (correlation coefficients, average profiles, average standard deviation, relative variability) was derived for the three ozone seasons. The partial ozone pressure does not at all heights follow a normal distribution (e. g. at tropopause level). Generally, the correlation between tropospheric and stratospheric ozone is rather poor. In some layers the highest correlation coefficients, i.e. –0.3 and +0.4, occur in autumn (October to December) and in winter and spring (January to April). The correlation between the ozone amounts of various stratospheric layers is distinct in autumn, less distinct in summer (May to September) and entirely missing from January to April. Conspicuous cross-correlations between temperature and ozone have been found for all three seasons. a) With a negative correlation between tropospheric temperature and middle tropospheric to middle stratospheric ozone (maximum up to –0.8); b) with a rather strong positive correlation between the ozone amount and the temperature in the lower stratosphere (maximum up to +0.84); c) with a positive correlation between the ozone amount of the middle stratosphere and the temperature of the middle stratosphere (maximum up to +0.8). The highest correlation coefficients occur in autumn. 相似文献
2.
Mani A. Sreedharan C. R. Joseph P. V. Sinha S. S. 《Pure and Applied Geophysics》1973,106(1):1192-1199
A series of ozone soundings were made at New Delhi (77°E 28°N) from 21 to 30 January 1969 and 10 to 22 February 1972 to study the changes in the vertical distribution of atmospheric ozone associated with western disturbances. The sonde used was the Indian ozonesonde made in the Instruments Laboratories at Poona.In February 1972, two western disturbances moved eastwards in quick succession across the western Himalayas, the first between the 11th and 13th and the second between the 13th and 15th. Associated with the first tropospheric trough was a high-speed jet stream with wind speeds reaching 180 knots, when the tropopause descended to 304 mb over Delhi. The second trough had no high-speed jet associated with it and the tropopause was at 227 mb. Ozone maxima were observed at 350, 180 and 125 mb in addition to the main peak at 35 mb in association with the upper tropospheric troughs over Delhi and its neighbourhood. A similar lowering of the tropopause and the influx of ozone in shallow layers was observed during the passage of two upper air troughs in January 1969. The study shows that with the approach of upper tropospheric troughs and the simultaneous lowering of the tropopause there is an increased influx in shallow layers of middle latitude ozone-rich air through breaks in the tropopause, replacing the subropical ozone-poor air over the station. 相似文献
3.
Evaluations of radiosonde soundings over North America and Europe, measurements aboard commercial airlines, and permanent ozone registrations at nineteen ground-based stations between Tromsö, Norway, and Hermanus, South Africa, yield three belts of higher ozone intrusion from the stratosphera and maximum values of the annual means at about 30°N, at between 40°–45°N and at about 60°N. A marked decrease of the annual mean values of the tropospheric ozone is detected towards the equator and the pole, respectively.In the northen hemisphere the maximum of the annual cycle of the tropospheric ozone concentration occurs in spring at high latitudes and in summer at mid-latitudes.For the tropical region from 30°S to 30°N a strong asymmetry of the northern and southern hemisphere occurs. This fact is discussed in detail. The higher troposphere of the tropics seems to be a wellmixed reservoir and mainly supplied with ozone from the tropopause gap region in the northern hemisphere. The ozone distribution in the lower troposphere of the whole tropics seems to be controlled by the up and down movements of the Hadley cell. The features of large-scale and seasonal variation of tropospheric ozone are discussed in connection with the ozone circulation in the stratosphere, the dynamic processes near the tropopause and the destruction rate at the earth's surface. 相似文献
4.
Summary The accuracy of the electrochemical ozone sonde, type OSR, has been estimated by analysing tandem ozone soundings of the balloon-borne electrochemical ozone sonde OSR at the Lindenberg Observatory from May to November 1982. A negative bias, though not significant, has been observed above about 28 km for soundings having high single correction factors. Random errors are at their minimum just above the level of the maximum of ozone partial pressure, and reach their maximum in the troposphere. Except at heights above about 28 km the random error of ozone sondes is a factor 2 to 3 times less than the error of the short Umkehr method. Provided that soundings with too high correction factors are neglected, the ozone sonde OSR has an accuracy comparable to that of other Brewer type sondes.The maximum amount of information on the vertical ozone distribution can be drawn from sonde measurements in the lower stratosphere. A study is underway to improve the sensitivity of the sonde OSR and thus to further enhance its reliability. 相似文献
5.
The possibility of the influence of a powerful radiowave on the ozone concentration in the lower part of the ionospheric D region is discussed on the basis of experiments at the Sura heating facility in March 2009, the results of which were published relatively recently by a group of authors. The results, which were obtained with the use of exact equations of the mesospheric ozone photochemistry, substantially disagree with some conclusions derived by the authors but do not completely deny their hypothesis on the possible influence on the ozone of internal gravity waves formed at heights of the ionospheric E region. 相似文献
6.
The latitudinal and temporal variations in the vertical profiles of ozone over the Indian subcontinent are discussed. In the equatorial atmosphere represented by Trivandrum (8°N) and Poona (18°N), while tropospheric ozone shows marked seasonal variations, the basic pattern of the vertical distribution of ozone in the stratosphere remains practically unchanged throughout the year, with a maximum at about 28 to 26 km and a minimum just below the tropopause. The maximum total ozone occurs over Trivandrum in the summer monsoon season and the latitudinal anomaly observed over the Indian monsoon area at this time is explained as arising from the horizontal transport of ozone-rich stratospheric air from over the thermal equator to the southern regions.In the higher latitudes represented by New Delhi (28°N), the maximum occurs at 23 km. Delhi, which lies in the temperate regime in winter, shows marked day-to-day variations in association with western disturbances and the strong westerly jet stream that lies over north and central India at this time.Although the basic pattern of the vertical distribution of ozone in the equatorial atmosphere is generally the same in all seasons, significant though small changes occur in the lower stratosphere and in the troposphere. There are small perturbations in the ozone and temperature structures, distinct ozone maxima being always associated with temperature inversions. There are also large perturbances not related to temperature, ozone-depleted regions normally reflecting a stratification of either destructive processes or materials such as dust layers or clouds at these levels. Particularly interesting are the upper tropospheric levels just below the tropopause where the ozone concentration is consistently the smallest, in all seasons and at all places where soundings have been made in India. 相似文献
7.
Gordon A. Macdonald 《Bulletin of Volcanology》1954,15(1):119-179
Summit eruptions of Mauna Loa, on the Island of Hawaii, occurred in 1940 and 1949, and flank eruptions in 1942 and 1950. Lava poured out in 1940 and 1942 was about equal in amount, totaling approximately 76 million cubic meters in each eruption. The 1949 eruption was somewhat smaller, liberating approximately 59 million cubic meters. The 1950 eruption was one of the largest on record, producing five large lava flows and several smaller ones, totaling approximately 459 million cubic meters. Three of the 1950 flows entered the sea. In 1942 a lava flow threatened the city of Hilo, and was bombed from the air in an effort to divert it. Calculations indicate that the gas content of the lava extruded during the 1940 eruption probably was in the vicinity of one percent by weight of the total magma. Other calculations indicate the viscosity of fluid Hawaiian lava to be in the range of 103 to 105 poises. Temperature readings on the 1950 lava ranged from 10900 to 9000 C. Kilauea Volcano showed signs of uneasiness in 1944, with an apparent increase of magmatic pressure indicated by outward tilting of the moutain flanks and a series of earthquakes progressing toward the surface. In December 1950 a series of earthquakes accompanied a subsidence of the summit of Kilauea Volcano. 相似文献
8.
Otto Meyer 《Ocean Dynamics》1948,1(5-6):222-227
Summary In the preceding report an extract of the observations at Wingst Observatory during the years 1942 is given, to continue the corresponding tables for 1939, 1940 and 1941, which have been published in the Annalen der Hydrographie und Maritimen Meteorologie. A copy of the registrations made during a rather heavy disturbance on March 1, 1942, is added. 相似文献
9.
Ozone depression in the polar stratosphere during the energetic solar proton event on 4 August 1972 was observed by the backscattered ultraviolet (BUV) experiment on the Nimbus 4 satellite. Distinct asymmetries in the columnar ozone content, the amount of ozone depressions and their temporal variations above 4 mb level (38 km) were observed between the two hemispheres. The ozone destroying solar particles precipitate rather symmetrically into the two polar atmospheres due to the geomagnetic dipole field These asymmetries can be therefore ascribed to the differences mainly in dynamics and partly in the solar illumination and the vertical temperature structure between the summer and the winter polar atmospheres. The polar stratosphere is less disturbed and warmer in the summer hemisphere than the winter hemisphere since the propagation of planetary wave from the troposphere is inhibited by the wind system in the upper troposphere, and the air is heated by the prolonged solar insolation. Correspondingly, the temporal variations of stratospheric ozone depletion and its recovery appear to be smooth functions of time in the (northern) summer hemisphere and the undisturbed ozone amount is slighily, less than that of its counterpart. On the other hand, the tempotal variation of the upper stratospheric ozone in the winter polar atmosphere (southern hemisphere) indicates large amplitudes and irregularities due to the disturbances produced by upward propagating waves which prevail in the polar winter atmosphere. These characteristic differences between the two polar atmospheres are also evident in the vertical distributions of temperature and wind observed by balloons and rocker soundings. 相似文献
10.
Harry van Loon Gerald A. Meehl Julie M. Arblaster 《Journal of Atmospheric and Solar》2004,66(18):1767-1778
The availability of global gridded precipitation and outgoing long-wave radiation (OLR) data after 1978 makes possible an investigation of the influence of the decadal solar oscillation in the tropics during three solar maxima and two solar minima. The NCEP/NCAR reanalyses starting in the 1950s allows the inclusion of an additional two solar maxima and minima to look for consistency of response across a longer time period. In the northern summer (July–August), the major climatological tropical precipitation maxima are intensified in solar maxima compared to solar minima during the period 1979–2002. The regions of this enhanced climatological precipitation extend from the Indian monsoon to the West Pacific oceanic warm pool and farther eastwards in the Intertropical Convergence Zone of the North Pacific and North American Monsoon, to the tropical Atlantic and greater rainfall over the Sahel and central Africa. The differences between solar maxima and minima in the zonal mean temperature through the depth of the troposphere, OLR, tropospheric vertical motion, and tropopause temperature are consistent with the differences in the rainfall. The upward vertical motion is stronger in regions of enhanced tropical precipitation, tropospheric temperatures are higher, tropopause temperatures are lower, and the OLR is reduced due to higher, colder cloud tops over the areas of deeper convective rainfall in the solar maxima than in the minima. These differences between the extremes of the solar cycle suggest that an increase in solar forcing intensifies the Hadley and Walker circulations, with greater solar forcing resulting in strengthened regional climatological tropical precipitation regimes. These effects are as strong or even more pronounced when warm and cold extremes in the Southern Oscillation are removed from the analyses. Additionally, lower stratospheric temperatures and geopotential heights are higher with greater solar forcing suggesting ozone interactions with solar forcing in the upper stratosphere. 相似文献
11.
利用1979~1992年卫星TOR对流层臭氧数据库资料,以及同期太阳辐照度数据序列,考察青藏高原对流层臭氧含量变化与太阳辐射周期变化之间的关系.分析表明,青藏高原对流层臭氧分布表现出与太阳辐照度相同的变化趋势,存在着明显的太阳周期变化特征.逐月线性回归分析表明,太阳辐照度增加导致青藏高原对流层臭氧增加的正效应.在太阳周期内,太阳辐射增加可使青藏高原对流层臭氧、平流层臭氧和臭氧总量分别增加1.31、4.97、6.628DU,或4.07%、2.04%、2.28%.该特征与赤道太平洋地区完全相反,分析产生差异的原因,至少应包括两方面因素：一是背景大气NOX和水汽含量的差异;二是青藏高原频繁发生的平流层-对流层大气物质交换和输送. 相似文献
12.
T. Tsuda Y. Masuda H. Inuki K. Takahashi T. Takami T. Sato S. Fukao S. Kato 《Pure and Applied Geophysics》1989,130(2-3):497-507
We have observed the time-height variation of the temperature field in the upper troposphere using a Radio Acoustic Sounding System (RASS) which consists of the MU radar and a high-power acoustic transmitter. The fast beam steerability of the MU radar has made it possible to measure temperature profiles in a fairly wide height range in the upper troposphere (5–11 km), even under intense wind conditions. Observations were continued for about 32 hr on 24–26 December, 1986 with a time-height resolution of 30 min and 150 m. During the observation period, the tropospheric jet was so intense that the acoustic wavefronts were severely distorted. Using wind velocity profiles observed by the MU radar we have numerically estimated the propagation of acoustic wavefronts, and further determined favorable pointing directions for the MU radar to receive significant backscattering from refractive index fluctuations produced by the acoustic waves. Conventional radiosonde soundings were carried out every 6 hr, which showed a temperature decrease of 4 K/day in the upper troposphere during the observation period. Temperature profiles taken by RASS agree well with the radiosonde results. 相似文献
13.
《Earth and Planetary Science Letters》2003,205(3-4):139-154
The Miyake-jima volcano abruptly erupted on July 8, 2000 after 17 years of quiet and gave birth to a crater, 1 km in diameter and 250 m deep. This expected unrest was monitored during the years 1995–2000 by electromagnetic methods including DC resistivity measurements and self-potential (SP) surveys. Beneath the 2500 yr old Hatcho-Taira summit caldera audio-magnetotelluric soundings made in 1997–98 identified a conductive medium, 200–500 m thick (within the 50 Ω m isoline) located at a few hundred metres depth. It was associated with the active steady-state hydrothermal system centred close to the 1940 cone and extending southward. A DC resistivity meter set in a Schlumberger array with 600, 1000 and 1400 m long injection lines evidenced strong resistivity changes between September 1999 and July 3, 2000 in the vicinity of the newly formed crater. The apparent resistivity has reached about three times its initial values on the 1400 m long line and has lowered to about 20% on the 600 m line. Just prior to the July 8, 2000 eruption SP mapping made inside the summit Hatcho-Taira caldera revealed negative anomalies where positive ones had occurred during the previous tens of years. The largest negative anomaly, −225 mV in amplitude, mainly took place above the 1940 cone which collapsed in the crater formation. A permanent 1 km long SP line across the caldera suggests accelerating changes during the 3 months preceding the eruption. On a larger scale, the comparison between 1995 and 2000 surveys has shown a global increase of the hydrothermal activity beneath the volcano. Its source could have been 250 m to the south of the crater. These observations suggest that the hydrothermal system was slowly disturbed in the months preceding the eruption while drastic changes have occurred during the 2 weeks before the summit collapse when tectonic and volcanic swarms have appeared. 相似文献
14.
H. K. Gupta B. K. Rastogi R. K. Chadha P. Mandal C. S. P. Sarma 《Journal of Seismology》1997,1(1):47-53
Reservoir induced earthquakes began to occur in the vicinity of Shivajisagar Lake formed by Koyna Dam in Maharashtra state, western India, soon after its filling started in 1962. Induced earthquakes have continued to occur for the past 34 years in the vicinity of this reservoir, and so far a total of 10 earthquakes of M 5.0, over 100 of M 4 and about 100,000 of M 0.0 have occurred. Every year, following the rainy season, the water level in the reservoir rises and induced earthquakes occur. Seismic activity during 1967–68 was most intense when globally, the largest reservoir induced earthquake occurred on 10 December, 1967. Other years of intense seismic activity are 1973 and 1980. During 1986 another reservoir, Warna, some 20 km south of Koyna, began to be filled. The recent burst of seismic activity in Koyna-Warna region began in August, 1993, and was monitored with a close network of digital and analog seismographs. During August, 1993–December, 1995, 1,272 shocks of magnitude 2 were located, including two earthquakes of M 5.0 and M 5.4 on 8 December, 1993 and 1 February, 1994, respectively. Two parallel epicentral trends in NNE-SSW direction, one passing through Koyna and the other through Warna reservoir are delineated. The 1993 increase in seismicity has followed a loading of 44.15 m in Warna reservoir during 11 June 11, 1993 through August 4, 1993, with a maximum rate of filling being 16 m/week. The larger shocks have been found to be preceded by a precursory nucleation process. 相似文献
15.
臭氧的时空分布特征对气候和环境变化具有显著影响,随着臭氧资料数量的增加和质量的提高,有必要对臭氧时空分布特征及其与气候变化的关系进行详细研究.本文利用欧洲中期天气预报中心提供的1979—2013年的全球月平均臭氧总量资料、平流层温度场资料,采用旋转经验正交函数分解(REOF)、Morlet小波分析、合成分析等方法研究了20°N以北的北半球冬季(12—2月)臭氧总量异常的主要空间分布结构与时间演变特征,并进一步分析了主要模态与平流层上层(2hPa)、中层(30hPa)以及下层(100hPa)温度异常的关系.结果表明:近30年北半球冬季臭氧总量异常变化最显著的区域主要有5个,分别位于极地地区(75°N—90°N,0°—360°)、北半球副热带地区(20°N—40°N,0°—360°)、阿拉斯加地区(60°N—75°N,180°—260°E)、北大西洋地区(45°N—60°N,310°E—360°E)及西伯利亚地区(50°N—65°N,80°E—130°E).5个区域的冬季臭氧总量异常具有明显的年际和年代际变化特征.1980年代后期是各个区域的臭氧总量异常由年代际偏多转为偏少的转换时段.此外,各区域存在显著的年际变化周期,而且各个区域的年际周期存在明显的差异.臭氧总量异常变化与平流层温度异常变化的关系表明,臭氧总量异常的增加(减少)能够导致平流层上层温度异常偏冷(暖)和平流层中、下层温度异常偏暖(冷),其中平流层中层温度异常的偏暖(冷)程度要比下层更加明显. 相似文献
16.
《Journal of Atmospheric and Solar》1999,61(7):539-543
The ozone concentration has been measured in the meteor zone using a method of radar echo duration distribution suggested by Jones and Šimek (1995). Data obtained by the forward-scatter system during the Lyrid meteor shower period in five consecutive years 1992–1996 agree with the Solar Mesosphere Explorer results for the same heights of 95 km. The mean value of the ozone concentration [O3]=(1.56±0.05)×1014 m−3 has been derived from a total of 6596 radar meteor echoes with duration ≥1 s. The results for individual years indicating a possible decrease in [O3] are discussed. 相似文献
17.
G. Dietze 《Pure and Applied Geophysics》1969,77(1):159-167
Summary It is proved by means of measuring series for skylight polarization during twilight carried out at different places that the zenith polarization is affected by the tropospheric turbidity still during the middle phase of twilight. This result is important for the inverse problem of the twilight theory. 3 approaches which explain this effect are examined. — Aerosol in the mesopause region is the cause for the well-known dip in the polarization curve during the middle phase of twilight. This interpretation can be supported by the distinct spectral differences.
This work has been presented at the IUGG/WMO Symposium on Radiation including Satellite Techniques (Bergen/Norway, August 22–28, 1968). 相似文献
Zusammenfassung An Meßreihen der Himmelslicht-Polarisation in der Dämmerung von verschiedenen Meßorten wird nachgewiesen, daß die Zenitpolarisation von der troposphärischen Trübung noch in der mittleren Dämmerungsphase beeinflußt wird. Dieses Ergebnis ist für die inverse Aufgabe der Dämmerungstheorie wichtig. 3 Möglichkeiten der Erklärung dieses Effekts werden untersucht. —Aerosol im Mesopausenbereich ist die Ursache für die bekannte Stufe in der Polarisationskurve während der mittleren Dämmerungsphase. Diese Deutung kann durch die deutlichen spektralen Unterschiede gestützt werden.
This work has been presented at the IUGG/WMO Symposium on Radiation including Satellite Techniques (Bergen/Norway, August 22–28, 1968). 相似文献
18.
This paper highlights the problem of step-length selection for the one-step-ahead prediction of ozone called the data time interval. This is done using a case study-based comparison of two approaches for predicting the maximum daily values of tropospheric ozone. The first approach is the 1-day-ahead prediction and the second is the prediction of the maximum values based on a multi-step-ahead iteration of 1-h predictions. Gaussian process modelling is utilised for this comparison. In particular, evolving Gaussian-process models are used that update on-line with the incoming measurement data. These sorts of models have been successfully used in the past for the prediction of ozone pollution. This paper contributes an assessment of the way that the maximum ozone values are predicted. A comparison of the daily maximum ozone values forecasted by a model based on 1-day-ahead predictions with those obtained by iterated 1-h-ahead predictions of the ozone with predictions at predetermined hours of the day is given. The forecast results are in favour of the on-line model based on hourly predictions when approaching closer to the real maximum values of ozone, and in favour of the daily predictions when they are made on a daily basis. 相似文献
19.
Janusz W. Krzy?cin Ma?gorzata Degórska Bonawentura Rajewska-Wich 《Journal of Atmospheric and Solar》1998,60(18):1755-1762
Total ozone data from some European stations have been analyzed to detect the ozone decrease in different seasons from 1979 to 1995. The differences between the winter–spring (December–March) and summer (May–August) total ozone means have decreased distinctly during the last three decades, by 10 Dobson Units per decade, showing that the winter–spring decrease is significantly stronger than the summer one. Applying a multiple regression model to the monthly means of tropopause height, positive trends in the summer and winter–spring seasons have been found, especially since 1979. This corresponds to the accelerating ozone decrease then. The possibility of using tropopause height variations as an indicator of dynamical variability in the total ozone trend model is discussed. The total ozone response to the changes of tropopause height seems to be independent of timescale over which the tropopause-total ozone relationship has been examined (month-to-month, interannual). The total ozone trends, as well as the accelerated rate of ozone decrease since 1979 in the winter–spring and summer seasons, respectively, are reduced by about 0.5–1% per decade after inclusion of the tropopause height effect on the ozone model. 相似文献
20.
Aboard commercial airliners twenty registrations of the ozone concentration of the upper troposphere were carried out within a period of 14 months between Europe and South Africa. Nearly each of these meridional ozone profiles shows an approximately constant ozone content between 25°S and 25°N with a pronounced seasonal variation. Most of these profiles show two marked peaks of the ozone concentration at about 30°N and between 40° and 45°N. Though the number of these registrations is not sufficient for statistical computations, the first results confirm the meridional ozone distribution, which was expected from studies with ozone-radiosonde soundings. Moreover a strong asymmetry of the northern and southern hemisphere is confirmed by these ozone measurements. 相似文献