降水中甲酸和乙酸研究综述   总被引：1，自引：0，他引：1  

何晓欢  徐晓斌 《气象科技》2009,37(6):646-650

对大气降水中甲酸和乙酸的相关研究进行了综述。介绍了过去曾采用的研究降水样品中两种有机酸的处理和分析方法,以及目前最常用的实验室分析方法。对降水中两种有机酸的浓度范围、全球时空分布以及受影响因素等相关研究工作进行了系统归纳,并且结合理论计算说明了有机酸对降水酸度的影响是不可忽视的。介绍了历史研究工作中得出的降水中两种有机酸的来源,包括天然源、人为源和有机物的二次化学转化等,以及有机酸源研究对于开展其它降水有机酸工作的研究意义。  相似文献   

夏季亚洲季风区对流层向平流层输送的源区、路径及其时间尺度的模拟研究   总被引：9，自引：4，他引：5  

陈斌  徐祥德  卞建春 《大气科学》2010,34(3):495-505

基于NCEP/NCAR分析资料和拉格朗日轨迹输送模式FLEXPART, 通过气块轨迹计算, 对2005年夏季亚洲季风区对流层向平流层输送 (Troposphere to Stratosphere Transport, 简称TST) 的近地层源区、 输送路径及其时间尺度问题进行了一些初步探讨。结果表明: (1) 夏季亚洲季风区TST两个主要的边界层源区, 一个是热带西太平洋地区; 另一个是青藏高原南部、 孟加拉湾以及印度半岛中北部等地区, 上述两个区域与夏季强对流的分布相一致。在对流层顶高度附近 (约16 km高度), 两个近地层源区的垂直输送贡献相当。但进一步分析发现, 穿越对流层顶高度的质量输送只有约10％能够进入20～22 km高度的平流层中, 且主要源于以青藏高原南侧为代表的南亚季风区 (约贡献75%), 这进一步强调了青藏高原及其周边区域在全球TST过程中的重要地位。 (2) 轨迹分析显示, 夏季亚洲季风区对流层进入平流层的 “入口区” 主要在 (25°N～35°N, 90°E～110°E) 区域的青藏高原及其周边区域。TST路径受对流层上层南亚高压闭合环流、 北半球副热带西风急流和赤道东风急流的共同控制。 (3) 亚洲季风区TST两个主要的过程, 一个是和夏季湿对流抬升直接联系的快速输送过程, 它可以使近地层大气在1～2天内输送到平流层中, 贡献了整个TST的10%～30%; 另一个是大气辐射加热所致的大尺度垂直输送, 该输送是一个相对的慢过程, 时间尺度一般为5～30天。此结果意味着, 源于地表的短生命周期的大气污染物可通过光化学反应过程对该区域平流层臭氧及其他大气痕量成分平衡产生重要影响。  相似文献   

New data of typomorphic features of diamonds from placers in North Timan     

G. K. Khachatryan  M. B. Kopchikov  V. K. Garanin  M. V. Chukichev  N. N. Golovin 《Moscow University Geology Bulletin》2009,64(2):102-110

The morphological and spectral-optical properties of diamond crystals from placers in North Timan rivers have been studied with IR-spectroscopy and cathode luminescence methods. As a result, correlation between external characteristics of diamonds (size and degree of mechanical damage) and number of optically active centers has been revealed. The habit and the type of distribution of structural defects in diamond crystals studied are comparable with those in diamonds from the Archangelsk Region and North Timan’s placers. Based on the obtained data, origin issues and possible primary sources of diamonds from North Timan’s placers are discussed.  相似文献   

河南桐柏围山城金银成矿带成矿物质来源: 铅同位素证据   总被引：1，自引：0，他引：1  

李红梅 《地质与勘探》2009,45(4):374-384

围山城金银成矿带出露有破山银矿床、银洞坡金矿床和银洞岭银矿床等三个大型金银矿床,均受地层和构造的双重控制,赋矿地层为新元古界歪头山岩组,河前庄背斜是成矿带的主要控矿构造.围岩地层歪头山岩组的铅同位素组成具有整体富Th亏U、低μ高ω的特征,与围山城金银成矿带的矿石铅整体富Th亏U、低μ高ω的特征一致.经过年龄校正后,把成矿带内的围岩地层和岩体的全岩铅同位素样品与矿石铅同位素对比分析发现,围岩歪头山岩组与矿石关系最为接近,其次为燕山期梁湾花岗岩体.成矿带的矿石铅具有混源特征.可以认为围岩歪头山岩组和梁湾花岗岩体共同为成矿带提供了铅源及成矿物质.  相似文献   

Gamma-ray bursts and their links with supernovae and cosmology     

Peter Meszairos  Neil Gehrels 《天体物理学报》2012,(8):1139-1161

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中国冰川积累与水汽来源补给分析   总被引：9，自引：4，他引：5  

张忠林  何元庆  庞洪喜  卢爱刚  顾娟 《冰川冻土》2004,26(6):729-735

利用冰川编目数据和NCEP/NCAR再分析资料, 对中国及周边地区水汽通量、中国冰川地理分布情况、大气环流途径和降水分布进行分析, 发现中国冰川水汽来源复杂, 不同地区各季节存在不同的大气环流控制. 这说明不同地理位置的冰川所指示的气候信息是不同的, 大约以30° N和100° E为界, 中国西北部主要受西风环流影响, 冰川发育的水汽主要源于西风环流. 以横断山脉为界, 横断山脉以西, 即30° N以南和100° E以西的区域, 主要受印度季风控制, 冰川发育水汽主要源于印度洋、阿拉伯海和孟加拉湾; 横断山脉以东区域, 受东亚季风控制, 冰川发育水汽主要来源于太平洋和南海; 横断山脉、念青唐古拉和青藏高原东部地区受印度季风和东亚季风共同控制, 冰川发育水汽主要来源于孟加拉湾和南海. 不同地区冰芯积累量的变化与该地区夏季季风环流指数的变化具有较好的一致性.  相似文献   

Ion and neutral sources and sinks within Saturn's inner magnetosphere: Cassini results     

E.C. Sittler Jr.  N. Andre  M. Burger  A. Coates  D. Reisenfeld  A. Persoon  H.T. Smith  R.E. Hartle  M.D. Shappirio  D.J. McComas 《Planetary and Space Science》2008,56(1):3-18

Using ion-electron fluid parameters derived from Cassini Plasma Spectrometer (CAPS) observations within Saturn's inner magnetosphere as presented in Sittler et al. [2006a. Cassini observations of Saturn's inner plasmasphere: Saturn orbit insertion results. Planet. Space Sci., 54, 1197-1210], one can estimate the ion total flux tube content, N_IONL², for protons, H⁺, and water group ions, W⁺, as a function of radial distance or dipole L shell. In Sittler et al. [2005. Preliminary results on Saturn's inner plasmasphere as observed by Cassini: comparison with Voyager. Geophys. Res. Lett. 32(14), L14S04), it was shown that protons and water group ions dominated the plasmasphere composition. Using the ion-electron fluid parameters as boundary condition for each L shell traversed by the Cassini spacecraft, we self-consistently solve for the ambipolar electric field and the ion distribution along each of those field lines. Temperature anisotropies from Voyager plasma observations are used with (T_⊥/T_∥)_W⁺∼5 and (T_⊥/T_∥)_H⁺∼2. The radio and plasma wave science (RPWS) electron density observations from previous publications are used to indirectly confirm usage of the above temperature anisotropies for water group ions and protons. In the case of electrons we assume they are isotropic due to their short scattering time scales. When the above is done, our calculation show N_IONL² for H⁺ and W⁺ peaking near Dione's L shell with values similar to that found from Voyager plasma observations. We are able to show that water molecules are the dominant source of ions within Saturn's inner magnetosphere. We estimate the ion production rate S_ION∼10²⁷ ions/s as function of dipole L using N_H⁺, N_W⁺ and the time scale for ion loss due to radial transport τ_D and ion-electron recombination τ_REC. The ion production shows localized peaks near the L shells of Tethys, Dione and Rhea, but not Enceladus. We then estimate the neutral production rate, S_W, from our ion production rate, S_ION, and the time scale for loss of neutrals by ionization, τ_ION, and charge exchange, τ_CH. The estimated source rate for water molecules shows a pronounced peak near Enceladus’ L shell L∼4, with a value S_W∼2×10²⁸ mol/s.  相似文献   

New active galactic nuclei among the INTEGRAL and SWIFT X-ray sources     

R. A. Burenin  A. V. Mescheryakov  M. G. Revnivtsev  S. Yu. Sazonov  I. F. Bikmaev  M. N. Pavlinsky  R. A. Sunyaev 《Astronomy Letters》2008,34(6):367-374

We present the results of our optical identifications of a set of X-ray sources from the INTEGRAL and SWIFT all-sky surveys. The optical data have been obtained with the 1.5-m Russian-Turkish Telescope (RTT-150). Nine X-ray sources have been identified with active galactic nuclei (AGNs). Two of them are located in the nearby spiral galaxies MCG-01-05-047 and NGC 973 seen almost edge-on. One source, IGR J16562-3301, is probably a BL Lac object (blazar). The remaining AGNs are observed as the starlike nuclei of spiral galaxies whose spectra exhibit broad emission lines. The relation between the hard X-ray (17–60 keV) luminosity and the [O III] 5007 line luminosity, log L _x/L _{[O III]} ≈ 2.1, holds good for most of the AGNs detected in hard X rays. However, the luminosities of some AGNs deviate from this relation. The fraction of such objects can reach ～20%. In particular, the [O III] line flux is lower for two nearby edge-on spiral galaxies. This can be explained by the effect of absorption in the galactic disks.  相似文献   

Optical identifications of five INTEGRAL hard X-ray sources in the Galactic plane     

I. F. Bikmaev  R. A. Burenin  M. G. Revnivtsev  S. Yu. Sazonov  R. A. Sunyaev  M. N. Pavlinsky  N. A. Sakhibullin 《Astronomy Letters》2008,34(10):653-663

The results of optical identifications of five hard X-ray sources in the Galactic plane from the INTEGRAL all-sky survey are presented. The X-ray data on one source (IGR J20216+4359) are published for the first time. The optical observations were performed with the 1.5-m RTT-150 telescope (Turkish National Observatory, Antalya, Turkey) and the 6-m BTA telescope (Special Astrophysical Observatory, Nizhny Arkhyz, Russia). A blazar, three Seyfert galaxies, and a high-mass X-ray binary are among the identified sources.  相似文献   

Analyses of the Compositional Characteristics and Sources of the Organochlorine Pesticides in the Surface Sediments of Guanghai Bay,Taishan City,Guangdong Province     

FAN Xiaoping  HE Yicheng  ZHANG Peng  Huo Zhuqing  ZHEN Leiming 《《地质学报》英文版》2019,93(Z2):65-66

Organochlorine pesticides (OCPs) are a class of toxic and harmful persistent organic pollutants widely found in environment. Hexachlorocyclohexane (HCHs) and DDTs are two of the most widely used OCPs (Qiu et al., 2004), so it is important to find out their compositional characteristics and sources in surface sediments. Guanghai Bay is located in the south of Guanghai Bay Industrial Park in Taishan City, Guangdong Province. It borders Huangmaohai to the east and Zhenhai Bay to the west, covering an area of about 236 square kilometers. In this study, surface sediments were collected at 16 sites in Guanghai Bay (Fig. 1). After the surface sediments were pretreated, GC‐MS was used to analyze OCPs. A total of 14 OCPs were detected and their content was shown in Table 1. The concentration of ΣOCPs ranged between 0.507～0.860ng·g‐1, with an average of 0.680 ng?g‐1. In general, the content of ΣOCPs was the highest at No. A12 site. The concentrations of these 14 detected OCPs ordered as dieldrin > epoxy heptachlor > P, P'‐DDD > γ‐HCH >endrin >aldrin > P, P'‐DDE >mirex >hexachlorobenzene >P, P'‐DDT > α‐HCH > δ‐HCH >β‐HCH > heptachlor.  相似文献