西北五省(区)生态环境综合分区及其建设对策

本文以图像遥感解译为主 ,结合野外实际考察 ,并通过抽样验证完成。在对生态环境界定和赋予内涵的基础上 ,根据区划目的、原则和所选取的指标体系 ,从生态环境分类入手 ,经过从上向下续分和由下向上合并的反复磨合过程、专家集成模拟 ,对西北五省(区 )生态环境做了全面的综合分区研究 ,并针对所存在的生态环境问题 ,提出生态环境保护和建设的对策 ,为西北五省 (区 )实施西部大开发生态环境监测、治理、建设和规划提供科学依据。     

滇池农村固体废物和化肥流失治理试验研究

怎样合理处置农村固体废物和减少农田化肥流失一直是农村面源污染控制的难题之一。该研究将农村固体废物的处理与减少化肥施用措施有机结合，利用微生物复合发酵剂和农村固体废物生产活性肥料，开展了一系列农业种植试验和数据监测，在此基础上，提出了一套实用性强、效果好的控制农业固体废物和化肥流失污染的对策措施。     

Constraining the cosmological baryon density with X-ray clusters

We study the properties of X-ray galaxy clusters in four cold dark matter models with different baryon fractions Ω_BM, ranging from 5 to 20 per cent. By using an original three-dimensional hydrodynamic code based on the piecewise parabolic method, we run simulations on a box with a size of 64  h ⁻¹ Mpc and we identify the clusters by selecting the peaks in the X-ray luminosity field. We analyse these mock catalogues by computing the mass function, the luminosity function, the temperature distribution and the luminosity–temperature relation. By comparing the predictions of the different models to a series of recent observational results, we find that only the models with low baryonic content agree with the data, while models with larger baryon fraction are well outside the 1σ error bars. In particular, the analysis of the luminosity functions, both bolometric and in the energy band [0.5–2] keV, requires Ω_BM ≲ 0.05 when we fix the values h  = 0.5 and n  = 0.8 for the Hubble parameter and the primordial spectral index, respectively. Moreover we find that, independently of the cosmological scenario, all the considered quantities have very little redshift evolution, particularly between z  = 0.5 and 0.     

阿尔泰高山区金矿带的确定和意义

根据地质、地球化学和资源总量预测等方法的综合研究表明,在阿尔泰高山区红山咀断裂以北宽20～30km,东西长约150km地带为一重要金成矿带。金矿赋存于晚古生代陆相酸—中酸性火山岩地层中,空间上受冰长石-黄铁绢英岩化蚀变带严格控制,是以毒砂、辉锑矿等金属硫化物为主要载体的层控浅成低温热液溶滤型金矿,也是一种新的重要的金矿工业类型。     

双核型空间结构模式及其在世界地理研究中的应用

作者在我国沿海和沿江地区的空间结构进行深入研究的基础上,发现了一种新的空间结构模式,即双核型空间结构模式。本文在对这一模式进行理论分析的基础上,初步探讨也该模式在世界地理研究中的应用：①指出全球最大的双核结构由全球最大的港口城市鹿特丹和全球最大的内河港口城市杜伊斯堡所组成;②作为推动美国区域经济发展的最重要的一个轴线－“美国经济地理横轴”,是一由芝加哥和纽约组成的双核结构;③新旧首都构成一特殊的双     

雄安新区生态系统服务簇权衡与协同

河北雄安新区建设是千年大计、国家大事。在生态优先、绿色发展理念引领下,深入理解生态系统服务间关系对于优化国土空间开发保护、实现自然资源可持续管理具有重要意义。本文基于多源数据评估了雄安新区四种生态系统服务,分析了生态系统服务间关系,并利用自组织映射特征网络划分了生态系统服务簇,以期为新区统筹权衡规划建设提供科学依据。研究结果表明：雄安新区生物多样性维持服务供给总体呈从东北向西南递增;食物供给服务在安新县与容城县供给较高,在雄县供给较低;产水服务供给以西南部地区较高,东北部地区较低;娱乐服务供给则以中北部地区较高,西南部地区较低。不同类型生态系统服务间多为协同关系,少为权衡关系。识别出四种生态系统服务簇,不同服务簇的主要土地利用类型及服务供给特点均存在差异,食物供给簇以旱地为主,主要提供食物供给服务;文化娱乐簇也以旱地为主,主要提供娱乐服务;生态保育簇以水域、旱地和林地为主,主要提供生物多样性维持服务;城镇生活簇则以建设用地为主,也包括少部分水田,主要以产水服务较高。根据不同生态系统服务供给间关系特征,为新区合理确定土地利用变更时序与位置以及促进多重生态系统服务可持续供给提出了建议。     

Modelling the runoff-sediment yield relationship using a proportional function in hilly areas of the Loess Plateau, North China

Based on data observed at the 12 small watersheds in hilly areas of the Loess Plateau, North China, the relationship between event runoff volume and sediment yield is examined. The results reveal that the runoff-sediment yield relationship at the inter-event timescale is mainly determined by the runoff-sediment concentration relationship at the intra-event timescale. In the study area, the sediment concentration tends to be stable when the flow discharge exceeds a certain critical value. Many factors that are important for determining the characteristics of low-magnitude events, such as flow discharge, particle size of fluvial sediment, and accumulation of loose material on land surfaces prior to a rainstorm, appear to have little importance for high-magnitude events. Consequently, mean sediment concentration tends to be stable for large flood events, suggesting a strong similarity between the two flow-sediment relationships at inter-and intra-event temporal scales. Furthermore, a proportional function is proposed to predict event sediment yield, and the correspondence between the predicted and observed sediment yields is examined. The performance of the model is good for high-magnitude events, especially extreme events. The applicability of the proposed model at the annual timescale is also discussed.     

Redshifted 21-cm observations of high-redshift quasar proximity zones

The introduction of low-frequency radio arrays is expected to revolutionize the study of the reionization epoch. Observation of the contrast in redshifted 21-cm emission between a large H  ii region and the surrounding neutral intergalactic medium (IGM) will be the simplest and most easily interpreted signature. However, the highest redshift quasars known are thought to reside in an ionized IGM. Using a semi-analytic model we describe the redshifted 21-cm signal from the IGM surrounding quasars discovered using the i -drop-out technique (i.e. quasars at   z ∼ 6  ). We argue that while quasars at   z < 6.5  seem to reside in the post-overlap IGM, they will still provide valuable probes of the late stages of the overlap era because the light-travel time across a quasar proximity zone should be comparable to the duration of overlap. For redshifted 21-cm observations within a 32-MHz bandpass, we find that the subtraction of a spectrally smooth foreground will not remove spectral features due to the proximity zone. These features could be used to measure the neutral hydrogen content of the IGM during the late stages of reionization. The density of quasars at   z ∼ 6  is now well constrained. We use the measured quasar luminosity function to estimate the prospects for discovery of high-redshift quasars in fields that will be observed by the Murchison Widefield Array.     

Limits on the changes in the gravitational constant from nucleosynthesis

Due to the recent all-sky, high-precision measurement of microwave background anisotropies by WMAP, a value for baryon-to-photon ratio η was obtained. At the WMAP value for η, the ⁴HE abundance was predicted. In this article we use a simple semi-analytical method with ⁴He predicted and measured values to place a limit on the variation of the gravitational constant G. We find using a conservative range for the measured values for Y _p , that ΔG/G is constrained between −0.26 and 0.15. If we assume a monotonic power law time dependence G∼t ^−β then β values is constrained between −0.008 and 0.0038, which translate into . This compares well with results obtained by others using full numerical analysis.      

Electron surfing acceleration in oblique magnetic fields

Initially, inhomogeneous plasma jets, ejected by active galactic nuclei and associated with gamma-ray bursts, are thermalized by the formation of internal shocks. Jet subpopulations can hereby collide at Lorentz factors of a few. As the resulting relativistic shock expands into the upstream plasma, a significant fraction of the upstream ions is reflected. These ions, together with downstream ions that leak through the shock, form relativistic beams of ions that outrun the shock. The thermalization of these beams via the two-stream instability is thought to contribute significantly to plasma heating and particle acceleration by the shock. Here, the capability of a two-stream instability to generate relativistic field-aligned and cross-field electron flow, is examined for a magnetized plasma by means of a particle-in-cell (PIC) simulation. The electrons interact with the developing quasi-electrostatic waves and oblique magnetic fields. The simulation results bring forward evidence that such waves, by their non-linear interactions with the plasma, produce a highly relativistic field-aligned electron flow and electron energies, which could contribute to the radio synchrotron emissions from astrophysical jets, to ultrarelativistic leptonic subpopulations propagating with the jet and to the halo particles surrounding the accretion disc of the black hole.