中国进出口贸易碳转移排放测算方法分析与评价

目前中国的碳转移排放测算方法有很多,虽然方法不尽相同,但总的结论和计算出的变化趋势类似。造成碳转移量测算结果产生较大差异的原因主要有两方面,一是碳排放强度的测算模型不同,二是对于中国加工贸易转移碳排放的认识不同。测算避免转移排放量时,如果不考虑加工贸易的影响,在某些年份（如2002年）甚至会得到＂中国是碳转移的净进口国...     

胶东大尹格庄金矿床热液蚀变作用

胶东是我国最重要的金矿集区。其中,破碎带蚀变岩型———"焦家式"金矿床是区内最重要的金矿床类型,占胶东已探明金矿资源量的90%以上。大尹格庄金矿床位于胶西北招平断裂带中段,是典型的破碎带蚀变岩型金矿床,区内发育有大规模的绢英岩化蚀变带(宽20~200m)和钾化/红化蚀变带(宽50~300m),蚀变岩型金矿体主要发育在招-平断裂带下盘的绢英岩化蚀变带中。本文在详细的野外地质观测基础上,查清了大尹格庄金矿床蚀变类型及矿物组合特征,针对大尹格庄金矿床Ⅱ号矿体系统采集了不同蚀变类型的岩石样品,进行了岩石元素地球化学分析,运用质量平衡方法讨论了热液蚀变过程中元素迁移规律,初步探讨了大尹格庄金矿床热液蚀变作用过程和金沉淀机制。通过本研究得出:大尹格庄金矿床内主要矿石类型为黄铁绢英岩,以浸染状、细脉状为主要矿化形式。大尹格庄金矿床热液蚀变期在时间上可以划分为:钾化/红化→绢英岩化→黄铁绢英岩化→碳酸盐化。钾化/红化蚀变为成矿前蚀变,在此过程中有少量热液钾长石的形成。在地球化学方面表现为Fe、Cu、Pb和Rb元素带入,Si、Al、Na、Ca、Ba、Sr、Cr等元素带出。同时流体-围岩通过交代反应使金从围岩中释放出来成为高价态离子活化进入成矿流体。绢英岩化和黄铁绢英岩化蚀变为成矿期蚀变,蚀变过程中与矿化有关的Fe、Cu、Pb元素表现为迁入状态,流体运移过程中,热液中的HS~-等组分损失,导致Au(HS)~(2-)络合物失稳分解,Fe~(2+)、Fe~(3+)被消耗形成黄铁矿,同时金大量聚集沉淀,此时完成了金由活化→迁移→沉淀富集成矿过程。     

Technology transfer by CDM projects

Abstract

Technology development and transfer is an important feature of both the United Nations Framework Convention on Climate Change (UNFCCC) and its Kyoto Protocol. Although the Clean Development Mechanism (CDM) does not have an explicit technology transfer mandate, it may contribute to technology transfer by financing emission reduction projects using technologies currently not available in the host countries. This article analyses the claims about technology transfer made by CDM project participants in their project design documents. Roughly one-third of all CDM projects, accounting for almost two-thirds of the annual emission reductions, involve technology transfer. Technology transfer varies widely across project types and is more common for larger projects and projects with foreign participants. Equipment transfer is more common for larger projects, while smaller projects involve transfers of both equipment and knowledge or of knowledge alone. Technology transfer does not appear to be closely related to country size or per-capita GDP, but a host country can influence the extent of technology transfer involved in its CDM projects.     

TOMRADE和MODTRAN 3.7模式研究紫外后向散射探测臭氧总量问题的比较

本文利用MODTRAN 3.7和TOMRADE模式分别计算了308.0 nm、312.5 nm、317.5 nm、322.3 nm、331.2 nm、360.0 nm六个紫外波段的后向散射强度并进行了比较,且利用两个模式计算得到的插值表,对EPTOMS实测资料分别进行反演,得到结论如下：1）两模式算得的后向散射强度随着太阳天顶角、卫星天顶角、地表反照率的变化特性基本一致,均能较好的反映紫外后向散射的辐射特性;2）总体而言,两模式计算的后向散射强度值相对偏差在－6％～18％之间;3）分别把MODTRAN 3.7和TOMRADE模式计算的插值表用于2003年7月30日中纬度地区EPTOMS实测资料的反演,得到的臭氧总量相对偏差在－3％～5％之间.本文对紫外波段大气辐射传输模式的研究和紫外后向散射探测臭氧总量的反演误差研究有着重要意义.     

The effects and characteristics of atmospheric dust during martian global dust storm 2001A

We present retrieved trends in dust optical depth, dust effective radius and surface temperature from our analysis of Mars Global Surveyor Thermal Emission Spectrometer daytime data from global dust storm 2001A, and describe their significance for the martian dust cycle. The dust optical depth becomes correlated with surface pressure during southern spring and summer in years both with and without a global dust storm, indicating that global dust mixing processes are important at those seasons. The correlation is low at other times of the year. We found that the observed decay of optical depths at the later stages of the dust storm match, to first-order, theoretical values of clearing from Stokes–Cunningham fallout of the dust. Zonally averaged effective radius is constant within standard deviation of results (between 1.2 and 2.0 μm, with a global mean for all seasons of 1.7 μm), at all latitudes and seasons except at southern latitudes of 35° and higher around equinoxes in both martian years, where it is larger than average (2–3 μm). The emergence and disappearance of these larger particles correlates with observations of polar cap edge storms at those latitudes. Northern latitude observations under similar conditions did not yield a similar trend of larger average effective radii during the equinoxes. We also report on a linear correlation between daytime surface temperature drop and rise in optical depth during the global dust storm. Global dust storm 2001A produced a significant optical depth and surface temperature change.     

基于MTFC的图像复原结果对比分析

地物在成像过程中,由于受到光学成像系统作用、地物周边环境等影响,会使得到的地物影像存在噪声、模糊等各种影像质量下降的问题,这种现象就是图像退化。根据影像退化机制,利用调制传递函数补偿(Modulation Transfer Function Compensation,MTFC)原理复原图像,提高航空面阵成像系统的成像质量,使航空面阵影像更便于判读解译。采用调制传递函数补偿(MTFC)原理进行图像复原。复原图像与原始影像相比在一定程度上边缘更加清晰,更利于判读解译,但在复原过程中也不可避免的添加了噪声。通过复原图像评价指标对比发现,利用航线方向MTF得到的复原图像效果较差,这与成像系统航线方向成像性能偏低有关。     

联合卷积神经网络与集成学习的遥感影像场景分类

针对人工设计的中、低层特征难以实现复杂场景影像的高精度分类以及卷积神经网络依赖大量训练数据等问题，结合迁移学习与集成学习，提出了一种联合卷积神经网络与集成学习的遥感影像场景分类算法。首先基于迁移学习的思想，利用在自然影像数据集上训练好的多个深层卷积神经网络模型作为特征提取器，提取图像多个高度抽象的语义特征；然后构建由Logistic回归和支持向量机组成的Stacking集成模型，对同一图像的多个特征分别训练Logistic模型，将预测概率结果融合构建概率特征；最后利用支持向量机对概率特征训练和预测，得到场景影像的分类结果。利用UCMerced_LandUse和NWPU-RESISC 45两种不同规模的遥感影像数据集进行试验，即使在只有10%的数据作为训练样本情况下，本文方法能够分别达到90.74%和87.21%的分类精度。     

Climate during the last glacial maximum in the Wasatch and southern Uinta Mountains inferred from glacier modeling

Recent improvements in understanding glacial extents and chronologies in the Wasatch and Uinta Mountains and other mountain ranges in the western U.S. call for a more detailed approach to using glacier reconstructions to infer paleoclimates than commonly applied AAR-ELA-ÄT methods. A coupled 2-D mass balance and ice-flow numerical modeling approach developed by [Plummer, M.A., Phillips, F.M., 2003. A 2-D numerical model of snow/ice energy balance and ice flow for paleoclimatic interpretation of glacial geomorphic features. Quaternary Science Reviews 22, 1389–1406] allows exploration of the combined effects of temperature, precipitation, shortwave radiation and many secondary parameters on past ice extents in alpine settings. We apply this approach to the Little Cottonwood Canyon in the Wasatch Mountains and the Lake Fork and Yellowstone Canyons in the south-central Uinta Mountains. Results of modeling experiments indicate that the Little Cottonwood glacier required more precipitation during the local Last Glacial Maximum (LGM) than glaciers in the Uinta Mountains, assuming lapse rates were similar to modern. Model results suggest that if temperatures in the Wasatch Mountains and Uinta Mountains were  6 °C to 7 °C colder than modern, corresponding precipitation changes were  3 to 2× modern in Little Cottonwood Canyon and  2 to 1× modern in Lake Fork and Yellowstone Canyons. Greater amounts of precipitation in the Little Cottonwood Canyon likely reflect moisture derived from the surface of Lake Bonneville, and the lake may have also affected the mass balance of glaciers in the Uinta Mountains.     

Origin and source regions of PM10 in the Eastern Mediterranean atmosphere

A set of daily PM₁₀ (n = 281) samples collected from April 2001 to April 2002 at a rural site (Erdemli), located on the coast of the Eastern Mediterranean, were analyzed applying Mass Closure (MC), absolute principal factor analysis (APFA) and Positive Matrix Factorization (PMF) to determine source contributions. The results from the three techniques were compared to identify the similarities and differences in the sources and source contributions. Source apportionment analysis indicated that PM₁₀ were mainly originated from natural sources (sea salt + crustal ≈ 60%) whilst secondary aerosols and residual oil burning accounted for approximately 20% and 10% of the total PM₁₀ mass, respectively. Calculations for sulfate showed that on average 8% and 12% of its total concentration were originated from sea salt and biogenic emissions, respectively. However, the contribution by biogenic emissions may reach up to a maximum of ~ 40% in the summer. Potential Source Contribution Function (PSCF) analysis for identification of source regions showed that the Saharan desert was the main source area for crustal components. For secondary aerosol components the analysis revealed one source region, (i.e. the south-Eastern Black Sea), whereas for residual oil, Western Europe and the western Balkans areas were found to be the main source regions.