共查询到20条相似文献，搜索用时 515 毫秒
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M. Van Roozendael P. Peeters H. K. Roscoe H. De Backer A. E. Jones L. Bartlett G. Vaughan F. Goutail J.-P. Pommereau E. Kyro C. Wahlstrom G. Braathen P. C. Simon 《Journal of Atmospheric Chemistry》1998,29(1):55-83
Comparisons of total column ozone measurements from Dobson, Brewer and SAOZ instruments are presented for the period 1990 to 1995 at seven stations covering the mid- and the high northern latitudes, as well as the Antarctic region. The main purpose of these comparisons is to assess, by reference to the well established Dobson network, the accuracy of the zenith-sky visible spectroscopy for the measurement of total ozone. The strengths and present limitations of this latter technique are investigated. As a general result, the different instruments are found to agree within a few percent at all stations, the best agreement being obtained at mid-latitudes. On average, for the mid-latitudes, SAOZ O3 measurements are approximately 2% higher than Dobson ones, with a scatter of about 5%. At higher latitudes, both scatter and systematic deviation tend to increase. In all cases, the relative differences between SAOZ and Dobson or Brewer column ozone are characterised by a significant seasonal signal, the amplitude of which increases from about 2.5% at mid-latitude to a maximum of 7.5% at Faraday, Antarctica. Although it introduces a significant contribution to the seasonality at high latitude, the temperature sensitivity of the O3 absorption coefficients of the Dobson and Brewer instruments is shown to be too small to account for the observed SAOZ/Dobson differences. Except for Faraday, these differences can however be largely reduced if SAOZ AMFs are calculated with realistic climatological profiles of ozone, pressure and temperature. Other sources of uncertainties that might affect the comparison are investigated. Evidence is found that the differences in the air masses sampled by the SAOZ and the other instruments contribute significantly to the scatter, and the impact of the tropospheric clouds on SAOZ measurements is displayed. 相似文献
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J. Brion A. Chakir J. Charbonnier D. Daumont C. Parisse J. Malicet 《Journal of Atmospheric Chemistry》1998,30(2):291-299
Absolute absorption cross-sections of ozone have been measured at ambient (295 K) and low temperature (218 K) in the visible region corresponding to the Chappuis bands. The temperature effect has been studied and found to be very small. The minimum of the absorption between the Hartley and the Chappuis bands is observed for the first time at 377,5 nm. 相似文献
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Data of stratospheric ozone measurements with the AK-3 lidar over Obninsk in 2012–2015 are compared with Aura/MLS and Aura/OMI satellite data and parallel surface observations of total ozone (TO) with the Brewer spectrophotometer. The maximum difference in mean ozone concentration between the lidar and Aura/MLS data in the altitude range of 13 to 32 km does not exceed 0.2 x 1012 mol./cm3 (or the maximum of 9% at the altitude of 13 km). At the same time, Aura/OMI data have a positive bias of about 20% relative to lidar data in the range of 13 to 20 km that is associated with OMI measurement errors according to literature data. Total ozone values calculated from lidar measurements jointly with the known climatology data are compared with those measured with the Brewer spectrophotometer. It is demonstrated that the correlation between the results of measurements obtained by two methods is close to linear, and the mean relative difference in the overall measurement range does not exceed 5%. 相似文献
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Abstract This work presents the climatology of the sulphur dioxide column over Thessaloniki derived from three years of observation with the Brewer spectrophotometer. The SO2 column averages 2.5 m atm‐cm and the shielding of UV‐B by SO2 is investigated and compared with the changes in shielding resulting from an anticipated ozone reduction. Columnar and surface SO2 concentrations over Thessaloniki appear to be typical of those in major industrial‐urban regions of the world. It is concluded that, for urban regions, predictions of changes in UV‐B as a result of man's activities must consider projections of changes in the SO2 column as well as ozone. 相似文献
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Om P. Tripathi S. G. Jennings C. D. O’Dowd K. P. Lambkin E. Moran 《Journal of Atmospheric Chemistry》2013,70(4):297-316
Sixteen years (1994 – 2009) of ozone profiling by ozonesondes at Valentia Meteorological and Geophysical Observatory, Ireland (51.94° N, 10.23° W) along with a co-located MkIV Brewer spectrophotometer for the period 1993–2009 are analyzed. Simple and multiple linear regression methods are used to infer the recent trend, if any, in stratospheric column ozone over the station. The decadal trend from 1994 to 2010 is also calculated from the monthly mean data of Brewer and column ozone data derived from satellite observations. Both of these show a 1.5 % increase per decade during this period with an uncertainty of about ±0.25 %. Monthly mean data for March show a much stronger trend of?~?4.8 % increase per decade for both ozonesonde and Brewer data. The ozone profile is divided between three vertical slots of 0–15 km, 15–26 km, and 26 km to the top of the atmosphere and a 11-year running average is calculated. Ozone values for the month of March only are observed to increase at each level with a maximum change of +9.2?±?3.2 % per decade (between years 1994 and 2009) being observed in the vertical region from 15 to 26 km. In the tropospheric region from 0 to 15 km, the trend is positive but with a poor statistical significance. However, for the top level of above 26 km the trend is significantly positive at about 4 % per decade. The March integrated ozonesonde column ozone during this period is found to increase at a rate of ~6.6 % per decade compared with the Brewer and satellite positive trends of ~5 % per decade. 相似文献
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Ultraviolet absorption cross-sections of trifluoro-bromo-methane (CF3Br-Halon 1301), difluoro-dibromo-methane (CF2Br2-Halon 1202) and of difluoro-bromo-chloro-methane (CF2BrCl-Halon 1211) are measured in the wavelength interval 172–304 nm for temperatures ranging from 210 to 295 K with uncertainties of between 2 and 4%. They are compared with previous measurements available at room temperature. Temperature effects are discussed and parametrical formulae are proposed to compute the absorption cross-sections for wavelengths and temperatures useful in atmospheric modelling calculations. Photodissociation coefficients are presented and their temperature dependence is discussed. 相似文献
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The temperature-dependent ultraviolet absorption cross-sections of CF3-CHFCI (HCFC-124) have been measured between 170 and 230 nm for temperatures ranging from 295 to 210 K, with uncertainties between 2 and 4%. These results are compared with other available sets of determinations. Temperature effects are discussed and the photodissociation coefficients, presented with their temperature dependence, are calculated. Implication of the temperature dependences on the stratospheric chemistry is also discussed. Parametrical formulae are proposed to compute absorption crosssection values for wavelengths and temperatures useful in modelling calculations. 相似文献
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大气臭氧变化在全球气候和环境中具有重要作用,是当今大气科学领域的重要研究对象之一。对比分析了中国科学院大气物理研究所河北香河大气综合观测试验站2014～2016年Dobson和Brewer两种臭氧总量观测仪器探测结果的一致性,并使用1979～2016年Dobson观测数据分析了香河地区臭氧总量的长期变化趋势。结果表明:进行有效温度修正后,两种臭氧总量仪器观测结果一致性较好,平均偏差仅为-0.14DU(多布森单位),平均绝对偏差为8.00 DU,标准差为36.09 DU,相关系数达0.964。整体来说,两类仪器观测臭氧总量吻合较好。SO2浓度对Dobson仪器数据精度有一定影响,两组仪器数据在SO2浓度为0～0.2DU、0.2～0.4DU和0.4DU大气条件情况下的平均偏差分别为4.8 DU、7.0 DU和8.0 DU,平均偏差随SO2浓度升高而增大。过去38年香河地区的臭氧总量季节差异性强,春、冬两季臭氧总量高,夏、秋两季臭氧总量相对低,季节变化趋势差异明显。从长期变化上看,臭氧总量变化波动有不同的周期,在4个大的时间段变化趋势不同,2000～2010年臭氧层有显著恢复,但最近几年又有变薄的趋势。 相似文献
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Stray light in single-monochromator Brewer instruments increases the uncertainty of solar ultraviolet spectral irradiance measurements and ozone retrievals. To study how spectral irradiance within and outside the measurement ranges of the instruments affects stray light, two Brewer MKII instruments were characterized for the level of in- and out-of-range stray light at multiple laser wavelengths. In addition, several solar-blind filters utilized in single-monochromator Brewers to limit out-of-range stray light were characterized for spectral and spatial transmittances. Finally, the measurement results were used to simulate the effect of stray light and stray light correction on spectral irradiance and ozone measurements at different wavelength regions. The effect of stray light from wavelengths above 340?nm was found to be negligible compared with other sources of uncertainty. On the other hand, contributions from wavelengths between 325 and 340?nm can form a significant portion of the overall stray light of the instrument, with 325?nm being the upper limit of the nominal measurement range of the instrument. 相似文献
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漠河地区臭氧的观测和计算 总被引：2，自引：0，他引：2
1997年3月上旬,在黑龙江漠河地区对地面和整层臭氧、太阳辐射等进行了短期观测,以初步了解该地区臭氧和辐射的变化规律以及它们之间的相互关系.研究发现,漠河地区近地面臭氧日变化明显,其峰值出现在每日10:00(北京时间)左右,并早于紫外辐射(UV)峰值出现时间.整层大气臭氧总量的日变化特征不明显.基于UV能量守恒,建立了臭氧与其影响因子-光化学、散射、UV等因子之间较好的定量关系和经验模式,并将其用于计算地面、整层大气臭氧小时值和日平均值.结果表明,计算值与观测值吻合的都比较好,它们相对偏差的平均值分别为:地面臭氧小时值(11.9%)和日平均值(9.0%);整层大气臭氧小时值和日平均值-7.4%、1.8%.因此,地面和整层臭氧的经验算法是合理和可行的.利用散射辐射/直接辐射(D/S)和散射辐射/总辐射(D/Q)可以描述大气中的物质如气溶胶、云等的散射作用.采用D/Q表示散射作用可以提高地面臭氧和整层大气臭氧计算的准确度,特别是对云量较大的情况.
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Sensitivity Studies for Monitoring Tropospheric Ozone from Space Using the Ultraviolet,Visible,and Polarization Bands 
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下载免费PDF全文 The authors analyzed the retrieval sensitivity of tropospheric ozone using simulated the Global Ozone Monitoring Experiment-2 （GOME-2） measurements. The retrieval sensitivity was evaluated by the degree of free- dom for signal （DFS）. The combination of the ultraviolet （UV）, UV polarization （UVPOL）, and visible （VIS） bands enhances DFS of tropospheric ozone and improves the vertical resolution of the retrieved ozone profile. UVPOL reduces the dependence on solar zenith angle, mainly in- creases the sensitivity in upper troposphere. Polarization increased the DFS by 20% on the eastern side of the GOME-2 orbit, with little improvement on the western side because the increase in DFS due to polarization is depend- ent on the relative azimuth angle. The inclusion of the visi- ble band reduces significantly the dependence on viewing geometry, and mainly increases the DFS in the lower tro- posphere （0-6 kin） by a factor of two. It was possible to retrieve several independent pieces of tropospheric ozone information from GOME-2 UV/UVPOL/VIS measure- ments, especially in the lower troposphere. 相似文献
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The effect of temperature (296–238 K) on the reaction of combustion soot (n-hexane) with ozone at low concentration (6–8 ppm) has been measured. Long optical path FTIR spectroscopy has revealed the rate law for ozone loss beyond initial stages, second order in O3, to be the same over this range of conditions. The reaction rate is 3.5 times lower at 238 K than at 296 K, and reveals an activation energy of 12.9 ± 0.5 kJ mol–1. The effect of humidity on the reaction has been estimated using its recently determined rate law dependence (p0.2). These data, differing from O3 reaction kinetics obtained from other types of carbonaceous particles used as surrogates for atmospheric soot, have implications for the role of combustion soot in atmospheric chemistry. Any involvement of aircraft soot in ozone depletion near the tropopause, for example, should be estimated using these temperature and humidity dependences. 相似文献
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Om Prakash Tripathi Sophie Godin-Beekmann Franck Lefèvre Marion Marchand Andrea Pazmiño Alain Hauchecorne Florence Goutail Hans Schlager C. Michael Volk B. Johnson G. König-Langlo Stefano Balestri Fred Stroh T. P. Bui H. J. Jost T. Deshler Peter von der Gathen 《Journal of Atmospheric Chemistry》2006,55(3):205-226
Simulations of polar ozone losses were performed using the three-dimensional high-resolution (1∘ × 1∘) chemical transport model MIMOSA-CHIM. Three Arctic winters 1999–2000, 2001–2002, 2002–2003 and three Antarctic winters 2001, 2002, and 2003 were considered for the study. The cumulative ozone loss in the Arctic winter 2002–2003 reached around 35% at 475 K inside the vortex, as compared to more than 60% in 1999–2000. During 1999–2000, denitrification induces a maximum of about 23% extra ozone loss at 475 K as compared to 17% in 2002–2003. Unlike these two colder Arctic winters, the 2001–2002 Arctic was warmer and did not experience much ozone loss. Sensitivity tests showed that the chosen resolution of 1∘ × 1∘ provides a better evaluation of ozone loss at the edge of the polar vortex in high solar zenith angle conditions. The simulation results for ozone, ClO, HNO3, N2O, and NO
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for winters 1999–2000 and 2002–2003 were compared with measurements on board ER-2 and Geophysica aircraft respectively. Sensitivity tests showed that increasing heating rates calculated by the model by 50% and doubling the PSC (Polar Stratospheric Clouds) particle density (from 5 × 10−3 to 10−2 cm−3) refines the agreement with in situ ozone, N2O and NO
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levels. In this configuration, simulated ClO levels are increased and are in better agreement with observations in January but are overestimated by about 20% in March. The use of the Burkholder et al. (1990) Cl2O2 absorption cross-sections slightly increases further ClO levels especially in high solar zenith angle conditions. Comparisons of the modelled ozone values with ozonesonde measurement in the Antarctic winter 2003 and with Polar Ozone and Aerosol Measurement III (POAM III) measurements in the Antarctic winters 2001 and 2002, shows that the simulations underestimate the ozone loss rate at the end of the ozone destruction period. A slightly better agreement is obtained with the use of Burkholder et al. (1990) Cl2O2 absorption cross-sections. 相似文献
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利用1979—2018年太阳后向散射紫外辐射计SBUV(/2)星下点臭氧遥感资料,结合ERA-Interim和MERRA-2大气温度再分析资料,考察青藏高原区域内拉萨和共和两地春季臭氧和大气温度变化趋势的差异性。结果表明拉萨和共和两个地区的臭氧和大气温度逆转趋势均发生于1999年。对比2008年以来青藏高原整体臭氧总量变化速率（4.5 DU/(10 a)),拉萨臭氧总量变化更快,为5.9 DU/(10 a),共和相对较慢,仅为3.7 DU/(10 a);同时,1999年以来拉萨和共和春季下平流层（100~30 hPa）大气温度分别以0.5~1.4℃/(10 a)和0.01~0.9℃/(10 a)速率增加,上对流层(250~175 hPa)大气温度分别以0.2~1.5℃/(10 a)和0.2~1.2℃/(10 a)速率降低。与2008年以来高原整体大气温度变化相比较,均慢于高原下平流层（125~70 hPa) 1~2℃/(10 a)的增温速率,快于高原上对流层（225~175 hPa）0.4~1.1℃/(10 a)的降温速率。两地臭氧与大气温度的相关系数和回归系数计算结果表明,拉萨和共和两个地区1999年以来春季臭氧恢复速率的不同是导致两地同期下平流层-上对流层温度逆转速率差异的重要因子之一。 相似文献
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本文选取多个臭氧总量观测站点,采用"三重制约法"分别对下列3组仪器观测臭氧总量数据进行统计分析,解算出不同观测资料的误差标准差,进而对比研究各种仪器的精度特征:1)1996~2003年期间地基WOUDC(World Ozone and Ultraviolet Radiation Data Centre)观测网络仪器(包括Brewer、Dobson和Filter臭氧测量仪)与星载TOMS(Total Ozone Mapping Spectrometer)和GOME(The Global Ozone Monitoring Experiment)仪器;2)2004~2013年期间WOUDC与星载OMI(ozone monitoring instrument)和SCIAMACHY(scanning imaging absorption spectrometer for atmospheric chartography)仪器;3)2004~2013年期间地基SAOZ(Système D’Analyse par Observations Zénithales)与星载OMI和SCIAMACHY仪器。结果表明,1996~2003年期间TOMS V8和GOME观测精度相当,分别为7.6±2.8 DU/46(其中,7.6±2.8 DU为所分析站点观测资料的平均精度及其标准差,46为站点数目)和7.6±1.5 DU/46。TOMS V8观测精度优于TOMS V7(8.5±3.0 DU/46),验证了前者对后者有所改进。2004~2013年期间OMI和SCIAMACHY在WOUDC地基站点观测精度接近,分别为6.6±1.4 DU/21和6.0±1.6 DU/21。SAOZ地基仪器精度为8.4±3.6 DU/8。对于3类WOUDC地基仪器,Brewer站点观测资料的平均精度最优(7.9±3.3 DU/12),Dobson次之(8.7±2.3 DU/19),Filter最差(14.7±4.0 DU/15)。相比于卫星,3种地面仪器观测平均精度较差(10.5±4.3 DU/46),这主要是由于Filter精度较差引起。中国境内的瓦里关(Brewer)、香河(Dobson)和昆明(Dobson)3个地基站点仪器观测精度均较优,分别为7.8 DU、6.7 DU和6.6 DU。尽管不同站点之间存在一定差异,但整体来说,地基与卫星仪器在中国境内3个站点观测臭氧总量吻合较好。 相似文献
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J. Malicet D. Daumont J. Charbonnier C. Parisse A. Chakir J. Brion 《Journal of Atmospheric Chemistry》1995,21(3):263-273
Absolute absorption cross-sections of ozone have been measured at five temperatures (218–295 K) in the UV wavelength region corresponding to the Hartley and Huggins bands (195–345 nm). The aim is to give to the users, a coherent set of data determined under high resolution. A comparison with previous work has been made. 相似文献