西部山区总辐射气候学计算及分布

根据西部山区太阳总辐射的实测资料分析，指出，西部山区总辐射的气候学计算必须考虑日照，水汽分布及海拔高度的影响。为此研制了适宜于西部山区的总辐射气候学计算公式Ｑ＝Ｑ０（ａ＋ｂｓ１＋ｃｓ１＾２），进而讨论了西部山区总辐射的时，空分布。     

中国大气有效辐射的气候计算及其分布

应用１９７９年５－８月季风试验期间印度８个陆地辐射探空站资料，通过多种方案试验，得出适用于各种云量条件下各等压面大气有效辐射的气候计算式，并计算和讨论了全国１０４站５００ｈＰａ大气有效辐射的时空分布特征。     

烟雾层的长波辐射效应以及对边界层温度层结的影响

本文利用一个简化的长波辐射方案，计算了兰州城市烟雾层大气的辐射效应．计算表明:烟雾层气溶胶增加了到达地面的大气逆辐射和气层的冷却率，平均污染状况时，增加量分别为15．2％和0．073℃／h．与烟雾层对太阳辐射吸收加热率相比，冷却率量值较小，但对全天边界层能量平衡所起作用不可忽略．对比分析了兰州和郊区夜晚的平均温度廓线演变情况，可以看出烟雾层长波辐射效应增加了低层大气中上部的冷却．     

Secular evolution of the vertical column abundances of CHCIF2 (HCFC-22) in the Earth's atmosphere inferred from ground-based IR solar observations at the Jungfraujoch and at Kitt Peak,and comparison with model calculations

Series of high-resolution infrared solar spectra recorded at the International Scientific Station of the Jungfraujoch, Switzerland, between 06/1986 and 11/1992, and at Kitt Peak National Observatory, Tucson, Arizona (U.S.A.), from 12/1980 to 04/1992, have been analyzed to provide a comprehensive ensemble of vertical column abundances of CHCIF₂ (HCFC-22; Freon-22) above the European and the North American continents. The columns were derived from nonlinear least-squares curve fittings between synthetic spectra and the observations containing the unresolved 2v ₆ Q-branch absorption of CHCIF₂ at 829.05 cm^–1. The changes versus time observed in these columns were modeled assuming both an exponential and a linear increase with time. The exponential rates of increase at one-sigma uncertainties were found equal to (7.0±0.35)%/yr for the Junfraujoch data and (7.0±0.23)%/yr for the Kitt Peak data. The exponential trend of 7.0%/yr found at both stations widely separated in location can be considered as representative of the global increase of the CHCIF₂ burden in the Earth's atmosphere during the period 1980 to 1992. When assuming two realistic vertical volume mixing ratio profiles for CHCIF₂ in the troposphere, one quasi constant and the other decreasing by about 13% from the ground to the tropopause, the concentrations for mid-1990 were found to lie between 97 and 111 pptv (parts per trillion by volume) at the 3.58 km altitude of the Jungfraujoch and between 97 and 103 pptv at Kitt Peak, 2.09 km above sea level. Corresponding values derived from calculations using a high vertical resolution-2D model and recently compiled HCFC-22 releases to the atmosphere, were equal to 107 and 105 pptv, respectively, in excellent agreement with the measurements. The model calculated lifetime of CHCIF₂ was found equal to 15.6 years. The present results are compared critically with similar data found in the literature. On average, the concentrations found here are lower by 15–20% than those derived from in situ investigations; this difference cannot be explained by the absolute uncertainty of ±11% assigned presently to the infrared remote measurements.     

广州地区太阳分光辐射的某些变化特征

利用广州地区1985—1990年的太阳分光辐射的连续观测资料（观测角度为23°11′），研究了广州地区紫外辐射、可见光辐射（光合有效辐射）、近红外辐射的某些特征。结果指出，每年7—10月份各分光辐射及总辐射总量较大。月总辐射中可见光辐射占总辐射的百分比年平均为47.3%，相应的紫外辐射和近红外辐射分别占7.1%和45.6%。文中还分析了晴天条件下分光辐射的变化和1990年紫外辐射变化的某些特征，并分析和讨论了分光辐射与云量、日照时间等因子的相关。     

与地震预报有关的电磁现象国际讨论会概况

与地震预报有关的电磁现象国际学术讨论会已于１９９３年９月６－８日在东京召开。这次学术讨论会的宗旨是，为世界各国学者提供一个公开讲坛以讨论与地震有关的电磁现象，并通过交叉学科与多科学相关领域相结合的方式探讨地震预报等问题。本文较详细地介绍了各国学者在这一领域中的最新成果。     

A CLIMATOLOGICAL STUDY ON SOLAR ULTRAVIOLET RADIATION

I.observedResultsandtheEmpiricalEstimatedFormulasforDirect'UltraviolctRadiationl.observedresultsofdirectultravioletradiationDuetostrongabsorptionofo2,N2,O,N,andO3inthehighlayeroftheatmosphere,solarradiationatwavelengthlessthan29onmcannotarriveateartl1suthee.Betweenthewavelength29Onmand4Oonm,thedirectultravioletirradia11ceSuvcanbewrittenas:Where,S.xissolarsPectralirradiancearrivedattopofatmosphere,Tlxisoptlcalthicknessofatmosphericmolecularabovesea1evel,Whicl1isaknownfunctiollofwavelengt…     

Characterization of the halophilic archaeal community in saltern crystallizer ponds by means of polar lipid analysis

Saltern crystallizer ponds are coloured red due to the presence of dense communities of red halophilic archaea (family Halobacteriaceae). Little quantitative information exists on the species distribution within the archaeal community in such ponds. As the different genera of the Halobacteriaceae differ in polar lipid content, and especially in the types of glycolipids, lipid analysis can be used to obtain information on the nature of the organisms present. Analysis of the polar lipids extracted from the biomass collected from the saltern crystallizer ponds in Eilat, Israel, showed one major glycolipid to be present, co-chromatographing with the sulfated diglycosyl diether lipid characteristic of the genusHaloferax. No indications were found for the presence of significant amounts of those glycolipids that would indicate the presence of large numbers of other archaea such asHalobacterium species (H. cutirubrum andH. salinarium, characterized by sulfated triglycosyl and tetraglycosyl diethers), orHaloarcula species (possessing a triglycosyl diether). Phosphatidyl glycerosulfate, a polar lipid absent inHaloferax species, was present in the lipid extract from the crystallizer ponds, suggesting that the dominant microorganism present may be related to strains which are presently classified in the genusHalobacterium but are awaiting a taxonomic reappraisal (H. sodomense, H. saccharovorum, andH. trapanicum). Organisms of the latter group are characterized by sulfated diglycosyl diethers, and the presence of phosphatidyl glycerosulfate. Attempts to isolate the dominant type of bacterium on agar plates yielded relatively low counts (1–2 orders of magnitude lower than the numbers observed microscopically) of bacteria, and most of the isolates had a polar lipid composition characteristic of theH. salinarium group or theH. sodomense-H. saccharovorum-H. trapanicum group.     

Some measurements of the extinction coefficients of solar radiation in Lagos

Solar radiance measurements covering over seventeen months are analysed for a location beside the Lagos Lagoon. The aerosol extinction coefficient was generally higher in the dusty months than in the wet months. Clean air estimates of the coefficient are made. Data on its wavelength dependence are also presented.     

Approximation of the infra-red radiation flux in an atmosphere with cloud

Summary A three-stream infra-red radiation scheme for use particularly in boundary layer models is described. Local uniformity of the atmosphere (i.e. a generalization of the cooling to space approximation in clear air) is assumed, and the radiation equation is solved by simple collocation rather than by the full discrete ordinate method. In clear air the scheme corresponds to the usual approximation, which incorporates the Elsasser factor in the transmission function to account for diffuse radiation. The band models of Goody for water vapour and Elsasser for carbon dioxide are used for the band averaging of the transmission functions. Consistent with this, the band averaging of the radiation flux in cloud is undertaken by replacing the rapidly varying absorption coefficients for the gases by the actual band-averaged values of those coefficients. The band averaging is precise in the limits of strong and weak gaseous absorption.