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生物气溶胶对全球气候、空气质量、大气过程和人体健康均具有重要影响。每年爆发的沙尘事件,使得生物气溶胶可借助沙尘进行长距离输运,从而影响到下风向地区生物气溶胶的浓度和性质。综述了沙尘天气下生物气溶胶中微生物的浓度、特性和分布特征的研究现状。已有研究显示,沙尘发生时,生物气溶胶中不同类别微生物的组成比例会有显著变化,细菌和真菌相对贡献随之改变。可培养细菌、真菌和总微生物浓度,均在沙尘天气下显著增加,但不同地区不同种类微生物在沙尘天气下的增加幅度相差很大。生物气溶胶中微生物主要分布于粗粒子中,其粒径分布受到沙尘天气的较大影响,而且不同种类微生物粒径分布的变化并不相同。沙尘发生时,生物气溶胶中的微生物群落结构与优势微生物也会发生明显改变。沙尘天气对生物气溶胶浓度、粒径分布、群落结构和活性的影响程度和影响机制,还需要进一步深入研究。 相似文献
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气溶胶吸收及气候效应研究的新进展 总被引：14，自引：1，他引：13
最新研究结果表明仅关注气溶胶大气顶辐射强迫是不够的,特别是对于在短波辐射区域存在较强吸收的气溶胶类型,如烟尘、沙尘气溶胶。INDOEX实验表明来自印度次大陆的吸收性气溶胶产生的地表辐射强迫在量值上是大气顶辐射强迫的3倍左右,二者的差额以大气辐射加热的形式出现。气溶胶吸收通过加热气溶胶层所在大气,减少地表太阳辐射,影响地面蒸发,改变大气稳定度,从而影响水分循环。另外气溶胶的吸收对云产生“燃烧效应”,从而可能导致云量下降。鉴于气溶胶吸收的重要性,气溶胶吸收问题是当前气溶胶气候效应研究的一个热点问题。尽管关于气溶胶的吸收问题以及与之有关的气候效应还存在很大不确定性,根据观测事实或模拟结果得出的结论差别明显,但勿庸置疑的是气溶胶吸收是一个急需深入探讨的课题。由于我国北方地区春季沙尘活动十分频繁,而东部地区由于能源结构以及能源利用效率等问题致使气溶胶中吸收性成分（碳黑）含量偏高,一些资料分析以及模式研究结果均表明我国发生了一些有别于全球或其他地区的独特气候变化现象,初步分析表明气溶胶吸收在其中可能发挥了一定作用,因此加强我国气溶胶吸收特性的观测和理论研究,结合全球或区域气候模式,深入认识我国气溶胶辐射强迫、气候效应具有重要的科学意义,另外对于评估我国近年来采取的一些卓有成效的污染控制措施的环境和气候效应也是必不可少的。 相似文献
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天山乌鲁木齐河源1号冰川大气气溶胶的微观形貌及元素组成分析 总被引：4，自引：1，他引：3
为研究冰川区大气气溶胶单颗粒物的物理化学特征,使用带能谱的扫描电镜(SEM-EDX)对2007年在天山乌鲁木齐河源1号冰川东支积累区海拔4 130m(86°49′E,43°06′N)处采集的38个气溶胶样品中的38 861个单颗粒物进行了微观形貌和元素组成的分析.结果表明:天山乌鲁木齐河源1号冰川区大气气溶胶主要以粒径在0.6～2.5μm之间的不规则的非圆形矿物颗粒为主,其中以富含Si、Ca的粘土矿物颗粒为主,与人类活动密切相关的含S颗粒物及烟尘飞灰等含量较少.这与其它沙尘源区的气溶胶特征相似,其中含Ca颗粒多于其它沙尘源区,主要受西风带的影响.气团轨迹显示,来自于西面中亚地区的高空气流影响了1号冰川区的大气环境,表明天山乌鲁木齐河源1号冰川区的气溶胶主要代表了中亚沙尘源区对流层中上部大气的本底状况. 相似文献
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大气沉降对海洋初级生产过程与氮循环的影响研究进展 总被引：4，自引：1，他引：3
大气沉降通过为海洋提供外源性氮、磷和铁等微量元素,可显著影响海洋氮、碳循环过程,并产生气候效应。一方面促进海洋初级生产和生物固氮,增强海洋吸收二氧化碳的能力;另一方面影响海洋氮、碳循环路径,增加海洋生物源气溶胶排放量,间接影响气候变化。由于大气沉降对海洋生态系统及气候变化的重要影响,相关科学问题已成为海洋科学与大气科学交叉研究的热点,被多个国际研究计划列为核心研究内容。在大气污染物排放持续增加与沙尘事件频发的背景下,大气沉降对我国东部陆架海(黄海、东海)及其邻近西北太平洋碳、氮循环过程的影响日趋增强,因此该海区已成为大气沉降及其气候影响研究的代表性海域。结合分子生物学和实验生态学手段理解大气沉降影响下的海洋初级生产过程,利用同位素示踪技术研究大气沉降对海洋氮循环的影响,以及获得大气沉降影响下海洋生物源气溶胶排放的观测证据将是未来研究的重点方向。 相似文献
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SO2排放,硫酸盐气溶胶和气候变化 总被引：3，自引：0，他引：3
工业ＳＯ２排放的增加使对流层大气中硫酸盐气溶胶浓度增大，硫酸盐气溶胶通过其直接和间接辐射强迫作用影响气候变化。有关的研究结果显示：硫到盐气溶胶的冷却效应在一定程度上抵消了温室效应，北半球增暖趋势的减缓和日较差的减小可能与大气中人为硫酸盐气溶胶浓度的增加有关。 相似文献
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文章依据冰芯、树木年轮等自然记录和历史文献记录,分析了中国北方不同地区近2000年的沙尘事件及其与气候变化的关系。结果表明,在干旱区西部,历史时期的沙尘变化主要受温度变化的制约,无论在10年尺度,还是百年尺度上,沙尘事件与温度变化均表现为显著的反相关,即气候寒冷期与沙尘频发事件相对应,气候温暖期与沙尘发生变弱期一致;在半干旱区,在10年尺度上温度和降水序列与沙尘发生频率均显著负相关,但在百年尺度上沙尘与降水变化的关系更为密切;在干旱区东部,沙尘与气候变化的关系具有明显的过渡性特征,气候变化对沙尘事件的作用主要在百年尺度上体现出来,沙尘与温度记录的负相关比降水更好,在10年尺度上气候与沙尘序列尽管也是负相关,但不显著。通过对现代气象记录的气温、降水变化和沙尘事件频数分析,其结果与历史时期情况基本一致。 相似文献
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2006年春季我国东部海域气溶胶光学厚度与沙尘天气 总被引：1，自引：0，他引：1
结合船基的太阳光度计观测资料和空基卫星遥感的MODIS气溶胶光学厚度资料,研究了我国东部海域气溶胶光学厚度与沙尘天气的关系。通过对不同天气条件下500 nm气溶胶光学厚度的分析,得出晴天(背景天气)、有云和浮尘以及只有浮尘时的平均值分别约为0.2、0.6和1.3以上;将MODIS的气溶胶光学厚度与船基观测资料进行对比之后发现,两者随时间的变化趋势非常一致,但前者在数值上明显偏高;利用订正后的MODIS资料,分析了2006年春季我国东部海域气溶胶光学厚度的时空分布特征,并与我国北方发生的沙尘天气进行了对比,发现两者之间关系密切。 相似文献
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The planet's radiation budget includes practically all energy exchange between the Sun, the Earth, and space, and so is a fundamental factor of climate. The terms of this budget, observable only from space, are determined from sampled direct measurements of the solar and terrestrial radiation fields. On the contrary, however, it should be remembered that energy exchange between the Earth's surface and its atmosphere involves not only radiative but also non-radiative energy fluxes. Nevertheless, only observations from space can provide satisfactory global coverage of the different energy fluxes that determine climate at the Earth's surface, by way of indirect retrievals of radiative fluxes at the surface and at different heights in the atmosphere. We describe the methods, applied to measurements made with a variety of instruments on board different artificial satellites, that have led to our present knowledge of the Earth's radiation budget (ERB) at the “top of the atmosphere”: global annual mean values of the ERB terms, its annual cycle, its geographical structure, and its variations. We know that solar irradiance, averaged over the globe and the year, varies by only 0.1% with the solar activity cycle; we also know that planetary (Bond) albedo is close to 0.3, that the global annual mean emission of thermal infrared radiation to space is close to 240 Wm?2, and that these terms exhibit a weak but well determined annual cycle. We also know that cloud cover plays a major role in the radiation budget, both in the “shortwave” domain (global SW “cloud radiative forcing” –50 Wm?2) and in the “longwave” domain (+20 Wm?2), thus a net forcing of –30 Wm?2. Successive satellite missions give consistent results for the shape, the phase, and the amplitude of the annual cycle of the planetary radiation balance. However, the different estimates of its annual mean absolute value remain uncertain, not differing significantly from zero, although generally excessively positive. We also rapidly review the methods used to determine the surface radiation budget as well as that of the atmosphere. For the planetary (TOA) radiation budget, we examine to what extent interannual variations and interdecadal trends have been or could be detected. We conclude with a review of projects under way. We also discuss priorities for future efforts, considering in particular, on the one hand (Ringer, 1997), the need to better quantify the factors that govern climate sensitivity to modifications of the atmosphere's radiative properties, on the other hand, the importance of monitoring the evolution of the present disequilibrium situation. 相似文献
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Britta Bielefeld 《GeoJournal》1997,42(2-3):329-336
In recent years, attention has increasingly been paid to the question of the stability of the earth's climate. It has been observed that changes in climate are usually related to changes in the earth's surface. On this question, Liedtke writes ‘A change in climate can lead to considerable landscape changes’ (Liedtke 1990, p. 38). There seems to be some form of interaction between climate and the condition of the earth's surface. If solar radiation is taken to be the primary energy source for the earth's climate, the question arises as to how insolation affects the character of the earth's surface, and vice versa, how does the character of the earth's surface affect the insolation which occurs? Reconstructions of the last great Pleistocene glaciation 18,000 years ago show that the form of the earth's surface at that time was considerably different to its present form. In view of the interaction mentioned above between climate and earth surface, does this suggest a difference between the earth's radiation budget 18,000 years ago and that of today? If, as is widely believed, the area of the earth's surface covered by ice 18,000 years ago was approximately three times the current area (Liedtke 1990, p. 42), this presumably would have had at least some influence on the earth's radiation budget. The ice-covered areas may have modified the radiation budget by means of their high reflexivity. In other words, an albedo-related loss of radiation may have occurred. The results of this investigations show, that the global radiation budget at 18,000 B.P was about 7- -10% less than that of today. 相似文献
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黑河流域陆地—大气相互作用研究的几点思考 总被引：4，自引：2，他引：2
陆地和大气之间是相互作用、相互影响的,不仅陆面分布与地表过程对大气变化有着响应过程,而且陆面物理过程、地表特征分布对大气过程也有着重要影响。我国西北地区地形分布极不均匀,是水资源变化和气候变化的敏感区与脆弱地区。这里,由于海拔高度起伏造就了以水为主线的上游山区冰雪、冻土—中游森林、绿洲—下游戈壁荒漠的多个自然景观带共存的内陆河流域,是开展陆—气相互作用研究的理想场所。文章集中黑河流域水循环过程、冰雪/冻土与大气相互作用、降水异质性、人类活动影响以及尺度等问题,阐述了流域研究现状以及研究热点,指出发挥各学科优势,将大尺度的大气过程与中间尺度和小尺度的陆面水文/生态过程结合,建立流域尺度大气—水文—生态过程真正的双向耦合模式,不仅研究气候变化对陆面水文、生态的影响,同时探讨陆面小尺度过程对大气的反馈机理,探索流域尺度的水循环过程和驱动机理,为水资源合理利用提供理论基础。 相似文献
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In this paper satellite-derived radiative energy budget such as shortwave radiative heating, longwave radiative heating and net radiation balance have been studied for the post-onset phase of summer monsoon 1979. Since clouds play an important role in determining diabatic heating field as well as being a reflection of status of the monsoon itself, the day to day evolution of clouds from TIROS-N satellite has been made. Satellite-derived radiative heating rates from surface to 100 hPa were computed for each 100 hPa thickness layer. These heating rates were then compared with the observed latitudinal distribution of total radiative heating rates over the domain of the study. From the results of our study it was found that the characteristic features such as net radiative heating rates of the order of 0.2°C/day at upper tropospheric layer (100–200 hPa) and cooling throughout the lower tropospheric layers with relatively less cooling between 500–700 hPa layer observed in a case of satellite-derived radiative energy budget agree well with the characteristic features of observational radiative energy budget over the domain of the study. Therefore, it is suggested that radiative energy budget derived from satellite observations can be used with great potential and confidence for the evolution of the complete life cycle of the monsoon over the Indian region for different years. 相似文献
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Andrew P. Roberts Eelco J. Rohling Katharine M. Grant Juan C. Larrasoaña Qingsong Liu 《Quaternary Science Reviews》2011,30(25-26):3537-3541
Atmospheric mineral dust aerosols affect Earth’s radiative balance and are an important climate forcing and feedback mechanism. Dust is argued to have played an important role in past natural climate changes through glacial cycles, yet temporal and spatial dust variability remain poorly constrained, with scientific understanding of uncertainties associated with radiative perturbations due to mineral dust classified as “very low”. To advance understanding of the dust cycle, we present a high-resolution dust record from the Red Sea, sourced principally from Arabia, with a precise chronology relative to global sea level/ice volume variability. Our record correlates well with a high-resolution Asian dust record from the Chinese Loess Plateau. Importing our age model from the Red Sea to the Chinese Loess Plateau provides a first detailed millennial-scale age model for the Chinese loess, which has been notoriously difficult to date at this resolution and provides a basis for inter-regional correlation of Chinese dust records. We observe a high baseline of dust emissions from Arabia and China, even through interglacials, with strong superimposed millennial-scale variability. Conversely, the distal EPICA Dome C Antarctic ice core record, which is widely used to calculate the radiative impact of dust variations, appears biased to sharply delineated glacial/interglacial contrasts. Calculations based on this Antarctic dust record will therefore overestimate the radiative contrast of atmospheric dust loadings on glacial/interglacial timescales. Additional differences between Arabian/Asian and circum-Saharan records reveal that climate models could be improved by avoiding ‘global mean’ dust considerations and instead including large-scale regions with different dust source variability. 相似文献