1993—2004年华东部分地区酸雨的时空分布特征及其与气象条件的关系     

张明明  杨军  黄志勇  徐静馨 《南京气象学院学报》2013,5(2):120-126

分析华东地区15个酸雨观测站的1993—2004年数据资料,结果显示华东地区的酸雨灾害在全国范围内较为严重,其中以长江以南的浙江、福建地区尤为突出.1993—2004年华东地区降水的酸度呈现出先减轻后加重的趋势.降水量是影响华东酸雨的电导率和pH值的重要因素.pH值季节变化由高到低为夏、秋、冬、春,酸雨频率随季节的变化不显著.对同期15个观测站的电导率变化的分析显示,12年间华东地区降水的电导率呈现先稳定后变幅增大的趋势,降水酸度和电导率的年际变化存在显著的正相关关系.应当对影响降水酸度和电导率的相关大气成分加强监测与研究.  相似文献   

伽师近场观测地震资料的三维Q值成像     

赖晓玲  孙译 《大地测量与地球动力学》2006,26(3):28-32

为了研究震源区介质的物性特征,利用振幅谱拟合和有限差分三维Q值成像方法处理了伽师地震区临时台网的地震波形资料,获得了该地震区上地壳的S波三维Q值图像。结果表明:不同深度的Q值图像都存在低Q值带,主要展布方向为EW向、NNE向和NNW向,与研究区的柯坪断裂、羊达曼断裂和麦盖提断裂有一定的对应关系,并且NNE向的低Q值带与强震群分布和余震分布的条带位置接近,推测低Q值带可能是震源区的几条深部断裂。  相似文献   

Hybrid estimation of cosmic microwave background polarization power spectra     

G. Efstathiou 《Monthly notices of the Royal Astronomical Society》2006,370(1):343-362

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The Atacama Cosmology Telescope project: A progress report     

Arthur Kosowsky   《New Astronomy Reviews》2006,50(11-12):969

The Atacama Cosmology Telescope is a project to map the microwave background radiation at arcminute angular resolution and high sensitivity in three frequency bands over substantial sky areas. Cosmological signals driving such an experiment are reviewed, and current progress in hardware construction is summarized. Complementary astronomical observations in other wavebands are also discussed.  相似文献   

PERMAFROST　CHANGES　AND　ENVIRONMENTAL　PROBLEMS　ALONG　THE　QINGHAI－XIZANG　HIGHWAY     

王绍令 《中国地理科学(英文版)》1995,5(2):149-156

ＰＥＲＭＡＦＲＯＳＴＣＨＡＮＧＥＳＡＮＤＥＮＶＩＲＯＮＭＥＮＴＡＬＰＲＯＢＬＥＭＳＡＬＯＮＧＴＨＥＱＩＮＧＨＡＩ－ＸＩＺＡＮＧＨＩＧＨＷＡＹ￥ＷａｎｇＳｈａｏｌｉｎｇ（王绍令）（ＬａｎｚｈｏｕＩｎｓｔｉｔｕｔｅｏｆＧｌａｃｉｏｌｏｇｙａｎｄＧｅｏｃｒ...  相似文献   

InFOCμS Hard X-ray Imaging Telescope     

J. Tueller  H. A. Krimm  T. Okajima  S. D. Barthelmy  S. M. Owens  P. J. Serlemitsos  Y. Soong  K.-W. Chan  Y. Ogasaka  R. Shibata  K. Tamura  A. Furuzawa  Y. Tawara  H. Kunieda  K. Yamashita 《Experimental Astronomy》2005,20(1-3):121-129

InFOCμS is a new generation balloon-borne hard X-ray telescope with focusing optics and spectroscopy. We had a successful 22.5-hour flight from Fort Sumner, NM on September 16,17, 2004. In this paper, we present the performance of the hard X-ray telescope, which consists of a depth-graded platinum/carbon multilayer mirror and a CdZnTe detector. The telescope has an effective area of 49 cm² at 30 keV, an angular resolution of 2.4 arcmin (HPD), and a field of view of 11 arcmin (FWHM) depending on energies. The CdZnTe detector is configured with a 12 × 12 segmented array of detector pixels. The pixels are 2 mm square, and are placed on 2.1 mm centers. An averaged energy resolution is 4.4 keV at 60 keV and its standard deviation is 0.36 keV over 128 pixels. The detector is surrounded by a 3-cm thick CsI anti coincidence shield to reduce background from particles and photons not incident along the mirror focal direction. The inflight background is 2.9 × 10⁻⁴ cts cm⁻² sec⁻¹ keV⁻¹ in the 20–50 keV band.  相似文献   

The imprints of local superclusters on the Sunyaev–Zel'dovich signals and their detectability with Planck     

K. Dolag  F. K. Hansen  M. Roncarelli  L. Moscardini 《Monthly notices of the Royal Astronomical Society》2005,363(1):29-39

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Powerful, obscured active galactic nuclei among X-ray hard, optically dim serendipitous Chandra sources     

P. Gandhi  C. S. Crawford  A. C. Fabian  R. M. Johnstone 《Monthly notices of the Royal Astronomical Society》2004,348(2):529-550

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国家资源环境安全要素的综合评价   总被引：5，自引：0，他引：5  

张雷 《地球信息科学学报》2002,4(4):86-92

资源环境安全问题始终是世界各国持续发展的核心任务和基本需求。考虑到单要素和整体两大分析方法的不足 ,作者提出了一种具有针对性的要素综合分析方法。根据世界 10个人口 1亿以上国家的抽样分析表明 ,土地、水资源、矿产及生态环境的整体状态是决定国家资源环境安全的基本要素群体。与此同时 ,为了改善国家 ,特别是发展中国家的资源环境脆弱状态和提高其稳定程度 ,第一是严格控制人口增长 ;第二是努力推进本国资源环境开发的国际化进程 ;第三是增大智力投入以提高资源深化加工程度 ;第四是加大本国生态环境保护力度。  相似文献   

No Higher Criticism of the Bianchi-corrected Wilkinson Microwave Anisotropy Probe data     

L. Cayón  A. J. Banday  T. Jaffe  H. K. Eriksen  F. K. Hansen  K. M. Gorski  J. Jin 《Monthly notices of the Royal Astronomical Society》2006,369(2):598-602

Higher Criticism (HC) has been proposed by Donoho & Jin as an effective statistic to detect deviations from Gaussianity. Motivated by the success of the Bianchi VII_h model in addressing many of the anomalies observed in the Wilkinson Microwave Anisotropy Probe ( WMAP ) data (Jaffe et al.), we present calculations in real and in wavelet space of the HC statistic of the Bianchi-corrected WMAP first-year data. At the wavelet scale of 5°, the HC of the WMAP map drops from a value above the 99 per cent confidence level (c.l.) to a value below the 68 per cent CL when corrected by the Bianchi template. An important property of the HC statistic is its ability to locate the pixels that account for the deviation from Gaussianity. The analysis of the uncorrected WMAP data pointed to a cold spot in the Southern hemisphere, centred at   l ∼ 209°, b ∼−57°  . The HC of the Bianchi-corrected map indicates that this spot remains prominent, albeit at a level completely consistent with Gaussian statistics. Consequently, it is debatable how much emphasis should be placed on this residual feature, but we consider the effect of modestly increasing the scaling of the template. A factor of only 1.2 renders the spot indistinguishable from the background level, with no noticeable impact on the results published in Jaffe et al. for the low- l anomalies, large-scale power asymmetry or wavelet kurtosis. A trivial interpretation would be that the Bianchi template may require a small enhancement of power on scales corresponding to the wavelet scale of 5°.  相似文献