从翡翠原石交易看翡翠市场的发展趋势     

包德清 《地质科学译丛》2014,(5):81-83

以翡翠原石投标为主体的缅甸珍宝玉石交易会（俗称“公盘”）一直是翡翠价格风向标,翡翠原石价格的上涨必然会推动成品价格的迅速跟进.通过对翡翠市场爆发式增长后的近几年原石交易特点的分析,发现所谓“原石价格上涨”完全是市场炒作的结果,一些玉商为了维护自身利益,聘请“枪手”投标,中标后又违约拒绝领标,造成原石投标交易现场火爆,价格屡创新高,但实际成交率却很低.从翡翠成品市场的反应来看,虽然价格有所上涨,但涨幅并不与媒体夸张的报道相适应.分析认为,玉商在翡翠原石交易中的行为需要进一步规范;在原石供应短缺和玉商极力维护自身利益的情况下,翡翠的价格不可能大幅度波动;高档翡翠因原料近于枯竭,价格还有进一步的上涨空间;在产能过剩的市场环境中,翡翠市场重归活跃尚待时日.  相似文献   

A Preliminary Study of Holocene Climate Change and Human Adaptation in the Horqin Region     

MU Yan  QIN Xiaoguang  ZHANG Lei  XU Bing 《《地质学报》英文版》2014,88(6):1784-1791

Abstract: Human activity during the Holocene in the Horqin region, northeastern China, has been widely documented. As an important proxy record of human activity, black carbon (BC) in sediments has been linked to climate change and human adaptation. A loess-paleosol section located in south Horqin was chosen for this study. Holocene climate change and human adaptation to the environment were discussed by analyzing BC, organic carbon (OC) and other proxies. The conclusions included: (1) before 3900 cal BP, human activity was closely related to the natural environment and cultural development was dominated by climate change. For example, the rapid decline of the agrarian Hongshan culture was caused by a slight decrease in temperature at ~5000 cal BP; (2) during 3900-3200 cal BP, the heavy dependence of human societies on nature gradually lessened and the ability of those human societies to adapt to the environment was enhanced. However, the farming-dominated Lower Xiajiadian culture was nonetheless replaced by the pastoralist Upper Xiajiadian culture due to an extremely cooling event at ~3200 cal BP; (3) during the late Holocene period, the marked influence of climate change on human activity might have lessened as a result of a clear improvement in human labor skills. After this, human living styles were influenced by cultural developments rather than climate change because humans had mastered more powerful means of productivity.  相似文献   

玉米秸秆还田和有机配施提高黑土酸中和容量     

姜勇  张勇勇  李天鹏  王汝振  王聪  张玉革  高洪军  朱平  李慧 《地理学报》2022,77(7):1701-1712

长期施用化肥导致农田黑土酸化、盐基离子耗竭、养分失衡及作物重金属污染等诸多问题。本文依托吉林公主岭国家黑土肥效监测基地25 a的施肥试验,研究了不施肥对照（C）、N、NP、NK、PK、NPK、厩肥—化肥配施（MNPK）、玉米秸秆还田（SNPK）等8个施肥处理对土壤酸中和容量（ANC）的影响,N、P、K施用量分别为165 kg hm^-2 a^-1、36 kg hm^-2 a^-1、68.5 kg hm^-2 a^-1,MNPK和SNPK处理与NPK处理为等N量。结果表明,施化肥导致表土pH下降0.37~1.39,MNPK和SNPK处理分别提高土壤pH值0.21和0.53。以pH 5.0为参比,N、NP、NK、PK、NPK各处理的酸中和容量ANC_{pH 5.0}分别为对照的42.85%、61.79%、54.05%、82.26%、63.68%;MNPK处理的ANC_{pH 5.0}是对照的1.86倍;加酸160 mmol kg^-1,SNPK处理的土壤pH值仅从7.65降至6.42,表现出极强的酸中和能力。SNPK和MNPK处理的土壤交换性盐基总量SEB分别是对照的1.37和1.14倍,土壤有机质SOM分别是对照的1.32和1.63倍,二者是提高土壤ANC主要原因。总之,有机物料添加显著提高了黑土抗酸化性能及土壤基础肥力水平,研究结果可为东北黑土区玉米秸秆还田保护性耕作及有机肥部分替代化肥实践提供长期试验的理论依据和数据支撑。  相似文献   

东北黑土区保护性耕作的发展现状与成效研究   总被引：1，自引：0，他引：1  

梁爱珍  张延  陈学文  张士秀  黄丹丹  杨学明  张晓平  李秀军  田春杰  McLaughlin Neil B  相洋 《地理科学》2022,42(8):1325-1335

东北黑土区承担着国家粮食安全“稳压器”的重要责任。然而,由于长期超负荷开发利用导致黑土日益退化,黑土资源的永续利用受到严重制约。理论与实践证明,保护性耕作是保护黑土地、推动黑土耕地质量和耕作效益绿色增长的发展模式。综述了保护性耕作的基本内涵及其在东北黑土区的发展现状与技术概况,从保护性耕作在土壤保持、保墒效益、结构改善、固碳培肥和土壤生物多样性增加、节本增效等方面系统评估了东北黑土区实施保护性耕作后的生态与经济效益,提出黑土区实施保护性耕作存在的问题与未来发展方向,以促进黑土地保护与利用协调发展、推动保护性耕作高质量跨越式发展。  相似文献   

Predicting the Impact of Climate Change on Vulnerable Species in Gandaki River Basin,Central Himalayas     

Raju RAI  ZHANG Yili  LIU Linshan  Paras Bikram SINGH  Basanta PAUDEL  Bipin Kumar ACHARYA  Narendra Raj KHANAL 《资源与生态学报(英文版)》2022,13(2):173-185

Gandaki River Basin (GRB) is an important part of the central Himalayan region, which provides habitat for numerous wild species. However, climatic changes are making the habitat in this basin more vulnerable. This paper aims to assess the potential impacts of climate change on the spatial distributions of habitat changes for two vulnerable species, Himalayan black bear (Ursus thibetanus laniger) and common leopard (Panthera pardus fusca), using the maximum entropy (MaxEnt) species distribution model. Species occurrence locations were used along with several bioclimatic and topographic variables (elevation, slope and aspect) to fit the model and predict the potential distributions (current and future) of the species. The results show that the highly suitable area of Himalayan black bear within the GRB currently encompasses around 1642 km² (5.01% area of the basin), which is predicted to increase by 51 km² in the future (2050). Similarly, the habitat of common leopard is estimated as 3999 km² (12.19% of the GRB area), which is likely to increase to 4806 km² in 2050. Spatially, the habitat of Himalayan black bear is predicted to increase in the eastern part (Baseri, Tatopani and north from Bhainse) and to decrease in the eastern (Somdang, Chhekampar), western (Burtibang and Bobang) and northern (Sangboche, Manang, Chhekampar) parts of the study area. Similarly, the habitat of common leopard is projected to decrease particularly in the eastern, western and southern parts of the basin, although it is estimated to be extended in the southeastern (Bhainse), western (Harichaur and northern Sandhikhark) and north-western (Sangboche) parts of the basin. To determine the habitat impact, the environmental variables such as elevation, Bio 15 (precipitation seasonality) and Bio 16 (precipitation of wettest quarter) highly contribute to habitat change of Himalayan black bear; while Bio 13 (precipitation of wettest month) and Bio 15 are the main contributors for common leopard. Overall, this study predicted that the suitable habitat areas of both species are likely to be impacted by climate change at different altitudes in the future, and these are the areas that need more attention in order to protect these species.  相似文献   

黑色页岩风化过程中元素的活动性及参照系的选取初探--以湖南省麻田、桃花江剖面为例   总被引：4，自引：0，他引：4  

宋照亮  彭渤  刘丛强 《地质科技情报》2004,23(3):25-29

系统考察了湖南省麻田和桃花江两个不同发育程度的下寒武统黑色页岩风化剖面,并提出了元素在理想剖面中的分布模式(概念模型);通过对比分析这两个剖面中元素的分布特征与理想分布模式的关系,并结合元素相关性研究、等质量图解的判别分析、微量元素的赋存状态及地球化学性质的探讨,认为在黑色页岩风化过程中,Ti为不活动元素,可作为参照系来计算其它元素的相对迁移性,Nb、Ta的活动性较小,Zr与Hf之间存在着共迁移现象;研究表明化学风化程度是影响元素活动性的重要因素.  相似文献   

The Newtonian forces in the Kerr geometry     

Sandip K. Chakrabarti  A. R. Prasanna 《Journal of Astrophysics and Astronomy》1990,11(1):29-35

We study the properties of the ’Newtonian forces’ acting on a test particle in the field of the Kerr black hole geometry. We show that the centrifugal force and the Coriolis force reverse signs at several different locations. We point out the possible relevance of such reversals particularly in the study of the stability properties of the compact rotating stars and the accretion discs in hydrostatic equilibria Received honourable mention in the 1989 Gravity Research Foundation essay competition.  相似文献   

Energy of a Stringy Charged Black Hole in the Teleparallel Gravity     

Mustafa Saltı 《Astrophysics and Space Science》2006,306(4):201-204

We use the teleparallel geometry analog of the Møller energy-momentum complex to calculate the energy distribution (due to matter plus field including gravity) of a charged black hole solution in heterotic string theory. We find the same energy distribution as obtained by Gad who investigated the same problem by using the Møller energy-momentum complex in general relativity. The total energy depends on the black hole mass M and charge Q. The energy obtained is also independent of the teleparallel dimensionless coupling constant, which means that it is valid not only in the teleparallel equivalent of general relativity, but also in any teleparallel model. Furthermore, our results also sustains (a) the importance of the energy-momentum definitions in the evaluation of the energy distribution of a given spacetime and (b) the viewpoint of Lessner that the Møller energy-momentum complex is a powerful concept of energy and momentum.  相似文献   

A Fundamental Plane of Black Hole Activity: Pushing Forward the Unification Scheme     

Andrea Merloni  Sebastian Heinz  Tiziana Di Matteo 《Astrophysics and Space Science》2005,300(1-3):45-53

We examine the disc-jet connection in stellar mass and supermassive black holes by investigating the properties of their compact emission in the hard X-ray and radio bands. We compile a sample of ∼100 active galactic nuclei with measured mass, 5 GHz core emission, and 2–10 keV luminosity, together with eight galactic black holes with a total of ∼50 simultaneous observations in the radio and X-ray bands. Using this sample, we study the correlations between the radio (L_R) and the X-ray (L_X) luminosity and the black hole mass (M). We find that the radio luminosity is correlated with both M and L_X, at a highly significant level. We show how this result can be used to extend the standard unification by orientation scheme to encompass unification by mass and accretion rate.  相似文献   

Self-consistent computation of γ-ray spectra due to proton–proton interactions in black hole systems     

S. Bhattacharyya  N. Bhatt  R. Misra 《Monthly notices of the Royal Astronomical Society》2006,371(1):245-251

In the inner regions of an accretion disc around a black hole, relativistic protons can interact with ambient matter to produce electrons, positrons and γ-rays. The resultant steady-state electron and positron particle distributions are self-consistently computed taking into account Coulomb and Compton cooling,  e⁻ e⁺  pair production (due to γ–γ annihilation) and pair annihilation. While earlier works used the diffusion approximation to obtain the particle distributions, here we solve a more general integro-differential equation that correctly takes into account the large change in particle energy that occurs when the leptons Compton scatter off hard X-rays. Thus this formalism can also be applied to the hard state of black hole systems, where the dominant ambient photons are hard X-rays. The corresponding photon energy spectrum is calculated and compared with broad-band data of black hole binaries in different spectral states. The results indicate that the γ-ray spectra  ( E > 0.8 MeV)  of both the soft and hard spectral states and the entire hard X-ray/γ-ray spectrum of the ultrasoft state could be due to p–p interactions. These results are consistent with the hypothesis that there always exists in these systems a γ-ray spectral component due to p–p interactions that can contribute between 0.5 and 10 per cent of the total bolometric luminosity. The model predicts that GLAST would be able to detect black hole binaries and provide evidence for the presence of non-thermal protons, which in turn would give insight into the energy dissipation process and jet formation in these systems.  相似文献