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101.
《Geoforum》2014
Concerns with the politics and practices of resource rights and access are integral to contemporary debates over environmental justice. Struggles over identity politics, especially the strategic articulation and deployment of particular identities at diverse geographical scales, have recently emerged as important mediators of justice claims in respect of resources rights, but also of recognition and procedural justice. To date, critical, multi-scalar analyses of identity-based claims for environmental justice have focused largely on the indigenous peoples’ movement. In doing so, they have failed to embrace an emergent dimension of identity-based, trans-scalar justice, namely the fledgling global pastoralists’ movement, the empirical focus for this paper. In the early years of the 21st century mobile pastoralists have begun to carve out new global spaces, through which diverse groups have attempted to negotiate common ground and forge common identities in their struggles for justice. In particular, mobile pastoralists have become increasingly visible in conservation politics and contests over land rights as they lay claim to both discursive and material ground as ‘custodians of the commons’ in an era of global climatic change. This paper draws on empirical work amongst pastoralists, NGOs and activists from Kenya, Mongolia and Spain to explore these identities, their implications for resource rights and access and the multi-scalar chains of accountability and legitimacy between global activists and their local constituents. 相似文献
102.
This work integrates stress data from Global Positioning System measurements and earthquake focal mechanism solutions, with new borehole breakout and natural fracture system data to better understand the complex interactions between the major tectonic plates in northwestern South America and to examine how the stress regime in the Eastern Cordillera and the Llanos foothills in Colombia has evolved through time. The dataset was used to generate an integrated stress map of the northern Andes and to propose a model for stress evolution in the Eastern Cordillera. In the Cordillera, the primary present-day maximum principal stress direction is WNW–ESE to NW–SE, and is in the direction of maximum shortening in the mountain range. There is also a secondary maximum principal stress direction that is E–W to ENE–WSW, which is associated with the northeastward “escape” of the North Andean block, relative to stable South America. In the Cupiagua hydrocarbon field, located in the Llanos foothills, the dominant NNE–SSW fractures are produced by the Panama arc–North Andes collision and range-normal compression. However, less well developed asymmetrical fractures oriented E–W to WSW–ENE and NNW–SSE are also present, and may be related to pre-folding stresses in the foreland basin of the Central Cordillera or to present-day shear associated with the northeastward “escape” of the north Andean block. Our study results suggest that an important driver for orogenic deformation and changes in the stress field at obliquely convergent subduction zone boundaries is the arrival of thickened crust, such as island arcs and aseismic ridges, at the trench. 相似文献
103.
104.
GPS无线电掩星技术能提供高精度、高分辨率、全球覆盖的地球电离层和中性层大气剖面。它具有全天候、低费用、无系统长期漂移等优点。从1995年4月至1997年3月,首次GPS/MET试验的成功显示了GPS掩星技术对监测全球大气能够发挥重要的作用,从而成为当前空间探测技术的研究热点之一。该文主要叙述了无线电掩星技术的数据处理系统的有关情况,并介绍了美国UCAR的掩星数据处理系统CDAAC的概况,可作为我国开展无线电掩星计划有关工作的借鉴。 相似文献
105.
Connecting atmospheric science and atmospheric models for aerocapture at Titan and the outer planets
Many atmospheric measurement systems, such as the sounding instruments on Voyager, gather atmospheric information in the form of temperature versus pressure level. In these terms, there is considerable consistency among the mean atmospheric profiles of the outer planets Jupiter through Neptune, including Titan. On a given planet or on Titan, the range of variability of temperature versus pressure level due to seasonal, latitudinal, and diurnal variations is also not large. However, many engineering needs for atmospheric models relate not to temperature versus pressure level but atmospheric density versus geometric altitude. This need is especially true for design and analysis of aerocapture systems. Drag force available for aerocapture is directly proportional to atmospheric density. Available aerocapture “corridor width” (allowable range of atmospheric entry angle) also depends on height rate of change of atmospheric density, as characterized by density scale height. Characteristics of hydrostatics and the gas law equation mean that relatively small systematic differences in temperature versus pressure profiles can integrate at high altitudes to very large differences in density versus altitude profiles. Thus, a given periapsis density required to accomplish successful aerocapture can occur at substantially different altitudes (∼150-300 km) on the various outer planets, and significantly different density scale heights (∼20-50 km) can occur at these periapsis altitudes. This paper will illustrate these effects and discuss implications for improvements in atmospheric measurements to yield significant impact on design of aerocapture systems for future missions to Titan and the outer planets. Relatively small-scale atmospheric perturbations, such as gravity waves, tides, and other atmospheric variations can also have significant effect on design details for aerocapture guidance and control systems. This paper will discuss benefits that would result from improved understanding of Titan and outer planetary atmospheric perturbation characteristics. Details of recent engineering-level atmospheric models for Titan and Neptune will be presented, and effects of present and future levels of atmospheric uncertainty and variability characteristics will be examined. 相似文献
106.
Claude Froeschlé Massimiliano Guzzo Elena Lega 《Celestial Mechanics and Dynamical Astronomy》2005,92(1-3):243-255
We detect and measure diffusion along resonances in a quasi-integrable symplectic map for different values of the perturbation parameter. As in a previously studied Hamiltonian case (Lega et al., 2003) results agree with the prediction of the Nekhoroshev theorem. Moreover, for values of the perturbation parameter slightly below the critical value of the transition between Nekhoroshev and Chirikov regime we have also found a diffusion of some orbits along macroscopic portions of the phase space. Such a diffusion follows in a spectacular way the peculiar structure of resonant lines. 相似文献
107.
全球变化与浙江洪水大势 总被引:4,自引:1,他引:3
根据历史和实测资料分析,对于全球变化下浙江近期洪水的运作大势,可得如下几点认识:(1)在未来的十几年之内,浙江省将处在枯水年占优势的阶段,但全球变化将使浙江洪水的时空变化更为剧烈,使沿海地区的洪水灾害更为严重。(2)由于浙江省的大中洪水一般都集中在太阳黑子活动的峰谷年前后,而近期的2004年和2009年分别是黑子活动第23周期的峰年和谷年,因此这两年前后必须予以足够的重视。(3)浙江洪水对厄尔尼诺现象具有较好的响应,因此厄尔尼诺同年或次年也必须引起足够的重视。(4)根据浙江历史上的台风重灾年资料,利用灰色灾变预测分析,可得浙江未来第一、第二和第三个台风重灾年分别为2001、2004和2008年,其中后两个台风重灾年与太阳黑子活动第23周期的峰年和谷年是大致吻合的。(5)植被破坏、河道设障等人类活动会产生一定的增灾效应,从而使浙江未来的洪水灾害更为严重。 相似文献
108.
The impact of two boundary-layer parameterisation schemes on the prediction of Indian monsoon systems by a global spectral model has been investigated. The turbulent kinetic energy closure scheme shows a positive impact on the prediction of some important synoptic features, including the genesis of monsoon lows, the tracking of monsoon depressions, and precipitation. 相似文献
109.
本项研究是PMIP(PalaeoclimateModelingIntercomparisonProject)国际合作项目中有关模型模拟与观测资料对比的一部分。模型试验对象是6000yr.BP的全球湿润状况。模拟试验以检测太阳辐射变化对全球大尺度气候系统的影响为主要目的。观测资料是利用地质证据恢复的古湖泊水位变化,实际上是某一地区的有效降水(降水减蒸发)的变化。通过两者的比较发现,所有模拟试验均能重现6000yr.BP在亚洲南部与非洲北部的湿润环境,从而证实了因太阳辐射变化导致的亚洲与非洲季风的增强。但模拟的季风增强无论是强度还是范围均小于地质记录。原因很可能是模拟试验中下垫面特征用“现代”的来处理。模拟试验对北半球夏季辐射增加造成的西风带北移及由此引起的中纬度地区的气候变化不够成功。绝大多数模拟对受洋流与海温影响较大的地区是失败的。主要原因可能是所有PMIP中的模拟试验都未考虑海洋的作用。 相似文献
110.
对全球变化背景下构建生态地理区域系统的若干认识 总被引:3,自引:1,他引:2
研究复杂的人地系统,研究区域的可持续发展需要有一个比较适当的区域划分。全球变化问题研究的水平也取决于对地域差异认识的深度。因此,建立中国生态地理区域系统,探讨其在全球变化中的应用,可为区域发展与陆地生态系统关系的研究提供科学的区域框架。本文从理论基础、必要性、目的、意义、界线、指标和方法论等方面探讨了有关生态地理区划的若干问题。 相似文献