基于高分辨率遥感影像的林地变化检测方法研究

本文采用2013年QuickBird和2017年GF-1卫星遥感影像,以黑龙江省五常市为研究区,利用遥感影像的光谱特征提取纯净森林像元,构建整合森林指数(Integrated Forest Z-Score,IFZ)对影像的森林和非森林区域进行区分,叠加对比分析两期影像提取结果,得到研究区内林地的变化区域.再将自动提取结果与人工判读图斑进行精度验证,面积误差为4.2％,图斑重叠率为85％.从精度结果可知,高分辨遥感影像可以准确地监测林地变化,对研究环境变化和森林经营管理具有决策性作用.     

Noble Gases in the Lunar Regolith

The most fundamental character of lunar soil is its high concentrations of solar-wind-implanted elements, and the concentrations and behavior of the noble gases He, Ne, Ar, and Xe, which provide unique and extensive information about a broad range of fundamental problems. In this paper, the authors studied the forming mechanism of lunar regolith, and proposed that most of the noble gases in lunar regolith come from the solar wind. Meteoroid bombardment controls the maturity of lunar soil, with the degree of maturation decreasing with grain size; the concentrations of the noble gases would be of slight variation with the depth of lunar soil but tend to decrease with grain size. In addition, the concentrations of noble gases in lunar soil also show a close relationship with its mineral and chemical compositions. The utilization prospects of the noble gas ^3He in lunar regolith will be further discussed.     

柴达木盆地三湖地区第四系生物气的形成途径与运聚方式

柴达木盆地三湖(台吉乃尔湖、涩聂湖、达布逊湖)地区第四系生物气区是我国最大的生物气区。笔者系统采集了该气区21个天然气样品,测量了其组分和碳同位素组成,重点探讨了生物气形成途径和运聚方式。生物气δ~(13)C_1和δ~(13)C_(CO_2)均随深度增大而变重,显示了CO_2还原途径成气的特征。生物气δ~(13)C_1、δ~(13)C_(CO_2)和δD分布与CO_2还原方式形成的生物气的相应同位素值分布范围接近。在有关成因图解中这些数据主要位于CO_2还原途径成气范围内。生物气CO_2和CH_4之间的碳同位素分馏系数α_c>1.055,具有CO_2还原途径成气的特征。柴达木盆地第四纪干旱的古气候、较低的古温度、较高的沉积速率和水体中较高的硫酸盐含量使得甲烷菌的大量繁殖只能在较大的深度范围内才能实现,从而,有利于CO_2还原途径成气作用进行。涩北一号、涩北二号气田生物气δ~(13)C_1组成分布可能表明,生物气形成以后沿疏导层水平运移进入气藏,基本不存在垂向运移。该项研究对于进一步深入探讨生物气成因、形成条件,确定生物气模拟实验方式与条件,计算生物气资源量,建立成藏模式和选择天然气有利勘探区块均具有重要价值。     

Identifying urban–rural differences in social vulnerability to natural hazards: a case study of China

Identifying and analyzing the urban–rural differences of social vulnerability to natural hazards is imperative to ensure that urbanization develops in a way that lessens the impacts of disasters and generate building resilient livelihoods in China. Using data from the 2000 and 2010 population censuses, this study conducted an assessment of the social vulnerability index (SVI) by applying the projection pursuit cluster model. The temporal and spatial changes of social vulnerability in urban and rural areas were then examined during China’s rapid urbanization period. An index of urban–rural differences in social vulnerability (SVI_D) was derived, and the global and local Moran’s I of the SVI_D were calculated to assess the spatial variation and association between the urban and rural SVI. In order to fully determine the impacts of urbanization in relation to social vulnerability, a spatial autoregressive model and Bivariate Moran’s I between urbanization and SVI were both calculated. The urban and rural SVI both displayed a steadily decreasing trend from 2000 to 2010, although the urban SVI was always larger than the rural SVI in the same year. In 17.5% of the prefectures, the rural SVI was larger than the urban SVI in 2000, but was smaller than the urban SVI in 2010. About 12.6% of the urban areas in the prefectures became less vulnerable than rural areas over the study period, while in more than 51.73% of the prefectures the urban–rural SVI gap decreased over the same period. The SVI_D values in all prefectures had a significantly positive spatial autocorrelation and spatial clusters were apparent. Over time, social vulnerability to natural hazards at the prefecture-level displayed a gathering–scattering pattern across China. Though a regional variation of social vulnerability developed during China’s rapid urbanization, the overall trend was for a steady reduction in social vulnerability in both urban and rural areas.

     

A Preliminary Study on Dust Grains in the Stratosphere

Collected by means of a high-altitude scientific balloon and a self-made automatic sample collector,a total of 276 dust grains were selected for the study of shape,grain size and optical property.Some of the grains were examined by X-ray diffraction and electrom microprobe techniques,The stratospheric dust grains can be classified as 6 types:cosmic dusts,cosmic dusts(?),microtektite,natural pollutants,artificial pollutants and the unknown substances.The different types of dust grains have different characters and distinguishing symbols.Widespread in the space of the solar system,cosmic dusts are the initial substances of the solar system and ,to some degree,have recorded a great wealth of information on the early history of the solar system.So they have become one of the important objects in the field of cosmochemistry at present time,Since the 1960‘s,scholars of many countries have collected cosmic dusts both in the space near the earth(using rock ets,space probes and space shuttles)and in the stratosphere (using high-altitude balloons or U-2air planes).According to the shape(the scanning electron microimage),element composition(the energy-dispersive X-ray spectrum)and optical properties of dust grains,the substances in the stratosphere can be classified as 5 types:cosmic dusts,alumina spheroids,terrestrial artificial pollutants,terrestrial natural pollutants and unknown substances(CDPET,1982).     

核爆炸玻璃、撞击玻璃和玻璃陨石源岩

本文根据核爆炸岩石熔融玻璃的地球化学研究结果,与超速陨石撞击坑的熔岩进行比较,获得在远离热力学平衡条件下,各种玻璃和熔岩在化学成分上分布十分均匀的重要结论。岩石玻璃和熔岩是由基岩各组成岩石按一定比例混合熔融形成的。它们的主量元素和痕量元素丰度受基岩元素背景值制约。文中根据熔体和靶岩的化学成分,计算了熔岩各组成岩石的百分比。玻璃陨石是地壳岩石受撞击熔融形成的。同一撒布区的玻璃陨石化学成分相近,说明起源于同一源坑;而玻璃陨石化学成分的不同,则说明母岩组成分量的差异。因此,文中通过模拟计算,得出各玻璃陨石的组成源岩。澳大利亚撒布区的玻璃陨石,Al₂O₃,K₂O 和Na₂O 与 SiO₂及 K₂O/Na₂O 比值不完全相同,说明澳大利亚撒布区存在着几个不同的源岩和源坑,至少有印支、爪哇、菲律宾和澳大利亚四个相应撞击坑。     

关于太古宙—元古宙界线的新认识

２５００Ｍａ作为太古宙－元古宙界线的提议被２８届国际地质大会通过，但并不意味着２５００Ｍａ作为太古宙－元古宙界线是永恒的最佳选择。事实上，太古宙－元古宙界线划在何处还存在很多争论，现行的界线划分依据也期分期标准相悖。大量资料表明），２３００Ｍａ时曾发生全球地质环境的灾变，灾变前后的地质作用（尤其是表生地质作用），有明显变化，导致了太古宙与元古宙的一系列差别。该灾变与元古宙－显生宙，古生代－中生代，     

A preliminary study on mineralogical and chemical compositions of some chondrites falling in China

Samples are available from 37 stony meteorites falling in China. Twenty-two chondrites are examined in terms of chemical and mineral compositions, cosmogenic nuclides, formation and exposure ages, impact effect and chondrule textures. On the basis of chemical-petrologic features these chondrites are classified asE ₄ (Qingzhen),H ₅ (Jilin, Changde, Shuangyang, Anlong, Xinyi and Yangjang),L ₆ (Renqiu, Junan, Heze, Rugao and Nei Monggol) andLL ₆ (Dongtai). E ₄ is characterized by high iron and sulfur, with the former occurring mainly as Fe^o and FeS. FromH ₅ throughH ₆ toLL ₆, iron and nickel decrease gradually while FeO and the ratio of Fe silicate to total iron increase gradually. indicating a general increase in the orderE-H-L-LL in the degree of oxidation at the time of formation. E ₄ consists mainly of enstatite and, to much less extent, free SiO₂ but olivine is hardly to be found. The olivine proportions amount to 29.07, 41.98 and 51.36 percent inH ₅,L ₆ andLL ₆ respectively, with Fa increasing from 17 to 27 percent. Recrystallization has been noticed to different degrees inH ₄,H ₅,L ₆ andLL ₆ chondrites. The extent to which the original structure disappears and the boundaries of chondrules become indistinct decreases from type 6 through type 5 to type 4, reflecting different degrees of thermal metamorphism. Major minerals in the meteorites all exhibit signs of low to medium shock metamorphism. Specific activity, depth effect and orbit effect are also measured on some chondrites that have fallen in recent years and some new information has been obtained with respect to the orbit and source region for meteorite parent bodies in space. This results show that the environment of formation ofE group may be nearer to Mars than that ofO group. Each chemical group of chondrites has its own evolutionary history, and chondritets of different chemical groups may have originated from parent bodies of different compositions. Or owing to the differentiation caused by thermal melamorphism, various kinds of meteorites may be derived from a common parent body. From this argument it is suggested that five stages may be recognized during the formation process of chondrites.     

Refinement of a lunar FeO mapping method

Clementine UVVIS and NIR data from the lunar sampling sites (totaling 46 sampling sites) were processed and used to refine the iron determination method of Le Mouéic et al. (2000, 2002). We found that about 21 sampling sites are unsuitable to Le Mouéic et al's spectral parameters ("slope" and "depth l") because their 1500 nm filter could not be used as spectral parameters' right shoulders and to evaluate the depth of the 1-μm absorption feature accurately. We used the rest 25 sampling sites to refine the method developed by Le Mouéic et al. (2000, 2002 ) and obtained our own equation of FeO content determination. We tested our own equation, and the results are satifactory. In our work we also acquired some useful experiences in scientific applications of our own dataset of the Chang'E-1 mission.     

太阳系生命信息探测

寻找地外生命是人类开展太阳系探测的根本出发点。火星是太阳系中最可能存在生命的天体之一。尽管海盗号开展的生物科学实验没有获得存在生命的确凿证据,但是近二十年的探测利用高分辨成像、光谱、质谱、雷达、中子分析等多方面的探测手段,获得了河流侵蚀地貌、古湖泊河流沉积物、水成矿物、极地冰盖、大气中水蒸气组分等一系列反映火星上有水的证据。这些发现暗示了火星过去或现在存在适宜生命繁衍的环境特征。大气甲烷、火星样品中有机物是下一步火星生命探测的重点。木星和土星的天然卫星,包括木卫二、土卫二和土卫六等在地外生命的研究中引起极大关注。木卫二上的盐水海洋环境被认为可能孕育生命,海洋中可能存在类似地球上的水热地质作用。土卫二南极存在细粒冰晶的喷射,且喷射物含有对于生命非常关键的液态水、氨气和其他碳氢化合物等。碳质球粒陨石存在大量可溶性有机物,其中包括多种构成蛋白质的氨基酸。星尘号和深度撞击任务的探测结果证实彗星所代表原始物质中含有大量的有机化合物,部分类型的氨基酸在碳质陨石和星际尘埃IDP颗粒相同,进一步支持了彗星与地球生命的起源之间存在联系。文中分析了太阳系生命探测中亟须解决的关键问题,包括系统建立地外生物标志化合物、发展适合太阳系探测的有机物分析技术、开展地球极端生命研究。最后呼吁我国在未来火星等天体探测任务中能增加有机物探测的相关载荷,及时介入太阳系生命探测,开拓深空领域。