航空矢量重力测量水平分量的带限直接地形影响     

周波阳  罗志才  宁津生  钟波 《测绘学报》2014,43(10):1019-1024

基于第二类Helmert凝聚法的级数展开式,独立推导了航空矢量重力测量水平分量带限直接地形影响的计算公式。在中国西部山区选取了两条沿纬圈方向4000m航线高度上的航线,采用 的数字高程模型基于解析核计算了水平分量的直接地形影响,经低通滤波后与基于带限公式计算的地形影响进行了比较。数值计算结果表明,二者吻合较好,本文给出的带限地形影响公式可用于航空矢量重力测量水平分量的地形归算。  相似文献   

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张西光  吕志平  赵冬青 《大地测量与地球动力学》2007,27(3):39-43

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Situating corporate framings of child labor: Toward grounded geographies of working children in globalized agriculture     

《Geoforum》2015

The expansion of multinational corporations into agricultural production around the world is resulting in new forms of engagement in specific places. In the context of neoliberal restructuring, these engagements are tied to shifting landscapes of societal, governmental and industry-based perceptions on the role of corporations in labor regimes. But how are these engagements developed and how do they connect to the everyday lives of workers? In India, when Monsanto expanded into hybrid cotton seed production in the early 2000s, the corporation came under pressure to address concerns over the widespread employment of children and young workers for seed pollination. In response, the corporation developed an approach to child labor that, I argue, works to reinforce generalized and problematic notions of childhood and work. Corporate engagements in global agriculture need to be situated in time and space, and alongside the experiences of workers. Children experience attempts to shape their patterns of work and mobility as a series of surmountable obstacles, disconnected from the process of deciding whether or not they will engage in this work. Drawing on qualitative fieldwork in Gujarat and Rajasthan, and documentary analysis of public documents, I outline the development of a corporate response to child labor and place it within the context of the rise of corporate social responsibility, global ideas of child labor, and in the specific case of cotton seed production in western India. I demonstrate that contextualized geographies of working children in globalized agriculture reveal the nature of multinational corporations’ engagements in specific places.  相似文献   

甘草和连翘对牙鲆CYP3A 活性影响的研究     

韩现芹  李健  李吉涛 《海洋科学》2010,34(12):19-25

研究甘草(Glycyrrhiza uralensis)和连翘(Forsythia suspensa)对牙鲆(Paralichthys olivaceus)肝细胞色素P4503A(CYP3A)活性的影响。将牙鲆随机分为3组,即对照组、甘草组和连翘组,对照组每日口灌0.9%的生理盐水,试验组每日1次口灌甘草30 mg/kg和连翘100 mg/kg,连续口灌6 d,第7天时,采用直接测定法和间接测定法(探针药物)进行CYP3A酶活性的测定。结果显示:在肝微粒体水平上,甘草和连翘均可明显提高红霉素-N-脱甲基酶活性,分别提高了1.79倍、4.87倍。与对照组相比,甘草组和连翘组氨苯砜的半衰期分别降低了4.51%(P0.05)和36.8%(P0.01);药时曲线下面积分别减小了8.28%(P0.05)和32.3%(P0.01);总清除率分别增加了5.63%(P0.05)和99.3%(P0.01)。说明连翘对牙鲆CYP3A的活性具有极显著诱导作用,甘草诱导作用不显著。提示其他药物与连翘合用时,其有效性和安全性可能会受到影响。  相似文献   

油企业抗震防灾规划信息管理系统的设计          下载免费PDF全文

《地震地质》1999,21(3):285

基于石油企业抗震防灾工作对网络与数据库的信息管理系统的需求，对数据库产品进行了简要分析，并根据石油企业抗震防灾规划的需求和信息管理的一般模式，提出了石油企业抗震防灾规划信息计算机管理系统的设想。认为，以 Ｍｉｃｒｏｓｏｆｔ Ａｃｃｅｓｓ 数据库软件为基础，利用 Ｖ Ｂ或 Ｖ Ｃ等可视化前端应用开发工具，是目前比较好的方案，它将使石油企业抗震防灾规划工作在办公自动化方面迈向新的台阶  相似文献   

Educating the compassionate water engineer–a remedy to avoid future water management failures? / Former des spécialistes de l’eau citoyens–une solution pour éviter de futurs échecs en gestion de l’eau?     

《水文科学杂志》2013,58(1)

Abstract

Abstract The number of local and regional-scale water management failures appears steadily to increase despite an apparently higher level of engineering solutions at hand. The objective of this paper is to examine the challenges the existing education system needs to meet in order to produce water engineers capable of responding to the complexity of contemporary and future water problems in relation to societal needs. The next generation of water engineers may stay in their professional functions until 2040 or 2050. It is likely that in this period more critical water management and environmental problems will be experienced than have been encountered so far. The question then arises whether the present water engineers have the proper background education to understand environmental, hydrological, ecological and socio-economic problems to resolve related water management problems. Future water engineers must, to a greater extent, include socio-economic consequences in planned and/or designed water management systems and convey greater transparency regarding risks and societal effects.  相似文献   

Observations of pulsating Ap stars in South Africa     

Peter Martinez  D. W. Kurtz 《Astrophysics and Space Science》1995,230(1-2):29-39

The rapidly oscillating Ap (roAp) stars currently represent the only main sequence stars other than the Sun which exhibit non-radial acoustic pulsations of high overtone. This makes them excellent subjects for asteroseismology, an approach which promises to yield accurate knowledge of the interior structures of stars. Of the 27 known roAp stars, 24 were discovered in Sutherland despite extensive searches conducted elsewhere. This paper reviews the discovery of the roAp phenomenon and describes the factors that contribute to the high discovery rate for these stars at Sutherland. Two long-term observational projects in progress at Sutherland are discussed,viz. the Cape roAp Star Survey and long-term monitoring of frequency variations in roAp stars.  相似文献   

Photopolarimetry of 3C 66A in 2003     

Yu. S. Efimov  N. V. Primak 《Astrophysics》2006,49(1):36-53

The BL Lac-type object 3C 66A was observed at the Crimean Astrophysical Observatory during the international project OJ-94. Observations were made over 10 nights from February through December 2003 at the Cassegrain focus of the 125-cm AZT-11 telescope with a photopolarimeter capable of simultaneous measurements in the UBVRI bands. In the course of our measurements the brightness of the object increased by more than 1 magnitude in all these bands. Its color indices varied and the degree of polarization decreased from ∼16% in February to ∼3% at the end of our observations. In December 2003 a rapid change in the position angle from 15° to 40° was noticed. The spectral energy distribution F_n is well described by a power law with a spectral index a (F_ν ∝ ν ^−α . The increase in brightness was accompanied by a reduction in the spectral index. The most probable mechanism for the observed changes in the brightness, degree of polarization, and spectral index may be a decrease in the magnetic field strength or a change in its configuration owing to a increase in the chaotic component of the field. __________ Translated from Astrofizika, Vol. 49, No. 1, pp. 41–59 (February 2006).  相似文献   

Merger Dynamics of the Pair of Galaxy Clusters——A399 and A401     

Qi-Rong Yuan  Peng-Fei Yan  Yan-Bin Yang  Xu Zhou Department of Physics  Nanjing Normal University  Nanjing yuanqirong@njnu. edu. cn National Astronomical Observatories  Chinese Academy of Sciences  Beijing Department of Mathematics  Physics  Qingdao University of Science  Technology  Qingdao 《中国天文和天体物理学报》2005,5(2):126-136

Convincing evidence for a past interaction between the two rich clusters A399 and A401 was recently found in the X-ray imaging observations. We examine the structure and dynamics of this pair of galaxy clusters. A mixture-modeling algorithm was applied to obtain a robust partition into two clusters, which allowed us to discuss the virial mass and velocity distribution of each cluster. Assuming that these two clusters follow a linear orbit and they have once experienced a close encounter, we model the binary cluster as a two-body system. As a result, four gravitationally bound solutions are obtained. The recent X-ray observations seem to favor a scenario in which the two clusters with a true separation of 5.4h-1 Mpc are currently expanding at 583 km s-1 along a direction with a projection angle of 67.5°, and they will reach a maximum extent of 5.65 h-1 Mpc in about 1.0 h-1 Gyr.  相似文献   

SN 1998A: explosion of a blue supergiant     

A. Pastorello  E. Baron  D. Branch  L. Zampieri  M. Turatto  M. Ramina  S. Benetti  E. Cappellaro  M. Salvo  F. Patat  A. Piemonte  J. Sollerman  B. Leibundgut  G. Altavilla 《Monthly notices of the Royal Astronomical Society》2005,360(3):950-962

We present spectroscopic and photometric observations of the peculiar Type II supernova (SN) 1998A. The light curves and spectra closely resemble those of SN 1987A, suggesting that the SN 1998A progenitor exploded when it was a compact blue supergiant. However, the comparison with SN 1987A also highlights some important differences: SN 1998A is more luminous and the spectra show bluer continua and larger expansion velocities at all epochs. These observational properties indicate that the explosion of SN 1998A is more energetic than SN 1987A and more typical of Type II supernovae. Comparing the observational data with simulations, we deduce that the progenitor of SN 1998A was a massive star  (∼25 M_⊙)  with a small pre-supernova radius  (≲6 × 10¹² cm)  . The Ba  ii lines, unusually strong in SN 1987A and some faint II-P events, are almost normal in the case of SN 1998A, indicating that the temperature plays a key role in determining their strength.  相似文献