天山乌鲁木齐河源1号冰川物质平衡对气候变化的敏感性研究   总被引：42，自引：23，他引：19  

刘时银 《冰川冻土》1998,20(1):9-13

应用度日物质平衡模式对天山乌鲁木齐河源１号冰川物质平衡及平衡线高度对气候变化的敏感性进行了研究．结果表明,位于大陆性气候区且具有暖季补给特征的乌鲁木齐河源１号冰川物质平衡对气候变化的敏感性要小于海洋性冰川,升温１℃或增加２０％的降水可引起平衡线上升８１ｍ或下降３１ｍ．此外,气温与降水在物质平衡形成过程中的作用是不同的,气温引起物质平衡剖面以旋转方式变化,而降水可导致其平移方式的响应．若未来升温２℃时,即使降水增加３０％,１号冰川向负平衡变化仍然不能得到遏制．  相似文献   

基于栅格数字高程模型自动提取黄土地貌沟沿线技术研究   总被引：36，自引：2，他引：34  

闾国年  钱亚东 《地理科学》1998,18(6):567-573

从数字高程模型中提取具有精确定位特征的连续的沟沿线是构建黄土沟壑丘陵地区土壤侵蚀,泥沙搬运和径流过程的空间分布式机理－过程模型的关键技术。本文提出了基于地貌形态学特征的地貌提取技术,在提取具有代表性的黄土丘陵沟壑区山西离石王家沟流域汇流网络的基础上,自动提取了该流域完整的沟沿线,得到了满意的结果。  相似文献   

二滩水电站地震遥测台网持续时间震级的研制   总被引：2，自引：0，他引：2  

赵珠  谢蓉华 《地震地磁观测与研究》1998,19(2):21-29

利用二滩水电站地震遥测台网的速度量和位移量观测记录,收集了震级ＭＬ为０．４￣５．４的４６０次地震（Δ〈２１０ｋｍ）的振动持续时间３５００多条,制作了该台网的持续时间震级公式和便查表。在方法上,不同于通常的按一次或两次曲线拟合,而采取计算机自动分段按折线拟合的方法,以阻尼最小二乘法完成其计算;在资料上,先分台制作８个子台的持续时间震级公式,在此基础上选择仪器、台基及公式中参数相近的子台,制作了适用于  相似文献   

利用WIN—SURFER软件绘制物化探图件   总被引：10，自引：4，他引：6  

田黔宁 《物探化探计算技术》1998,20(4):366-369

本文主要介绍了如何在ＷＩＮ－ＳＵＲＦＥＲ环境下实现物化探图件中的经纬网绘制、标准图框绘制、曲线类型图绘制方法。  相似文献   

Mineral Potential of Myanmar     

SOE WIN  MARLAR MYO MYINT 《Resource Geology》1998,48(3):209-218

Abstract: Myanmar is rich in mineral resources, and of potential importance are the deposits of antimony, chromium, nickel, PGM, copper, gold, lead, zinc, silver, tin and tungsten, which form district metallogenic provinces within the six geomor–phic–tectonic units. In terms of past production and potential mineral wealth Myanmar ranks high among Asian countries. The last few decades witnessed a dramatic fall in mineral production, but undoubtedly, the high level of mineral potential remains unrealized. This paper reveals mineral belts with a high level of economic potential which form attractive targets for mineral exploration and some individual mineral deposits of significant magnitude and grade, creating opportunities for development and mining investment.  相似文献   

Radiative acceleration of coronal gas in Seyfert nuclei     

L. Binette 《Monthly notices of the Royal Astronomical Society》1998,294(3):L49-L51

The line ratios from coronal gas in Seyferts can be successfully fitted with photoionized clouds of high densities and low volume filling factor. The ionization parameter implied is sufficiently high that models must consider the effect of radiation pressure from the active nucleus. In spite of the gravitational force of the nucleus, radiation pressure is sufficiently strong to compress and radially accelerate the internally stratified gas clouds provided that these contain small amounts of dust (≃ 10 per cent of the solar neighbourhood value). This radial acceleration could explain the blueshift of the coronal lines relative to the systemic velocity without the need to invoke an ambient 'pushing' wind. Embedded dust has the interesting effect of making the photoionized clouds marginally ionization-bounded instead of matter-bounded.  相似文献   

Lattice dynamical system modelling of molecular clouds     

G. Rousseau  H. Chaté  & J. Le Bourlot 《Monthly notices of the Royal Astronomical Society》1998,294(3):373-390

Because a comprehensive microscopic treatment of interstellar molecular clouds is out of reach, an alternative approach is proposed in which most of the crucial ingredients of the problem are considered, but at some 'minimal' level of modelling. This leads to the elaboration of a lattice dynamical system , i.e. a time-dependent, spatially extended, deterministic system of macroscopic cells coupled through radiative transfer. Each cell is characterized by a small set of variables and supports a caricatural chemistry possessing the essential dynamical features of more realistic reaction schemes.   This approach naturally precludes quantitative results, but allows heretofore unavailable insights into some of the basic mechanisms at play. We focus on the response of the transfer process and the chemistry to a frozen 'turbulent' velocity field. It is shown that the system settles generically into a state where the effective coupling between cells is neither local nor global, and for which no single length-scale exists.   The spectral lines reconstructed from the spatiotemporal evolution of our model may, depending on the velocity field, exhibit profiles ranging from Gaussian to bimodal with strong realization effects. In the bimodal case, the model intrinsically displays an energy cascade transport mechanism to the cells that cool most efficiently: the feedback of chemistry on radiative transfer cannot be neglected.   Finally, extensions of this work are discussed and future developments are outlined.  相似文献   

Solar EUV line identifications from delayed beam-foil spectra     

Elmar Träbert 《Monthly notices of the Royal Astronomical Society》1998,297(2):399-404

A number of electric dipole transitions from low-lying long-lived levels in Si-, P- and S-like ions of Fe and neighbouring elements have been identified by their longevity in delayed EUV spectra after foil excitation of fast ion beams. Some of these new identifications pertain to previously unidentified lines in solar flare spectra.  相似文献   

C-type shocks in the interstellar medium: profiles of CH⁺ and CH absorption lines     

D. R. Flower  & G. Pineau des Forêts 《Monthly notices of the Royal Astronomical Society》1998,297(4):1182-1188

We have computed optical absorption-line profiles of CH⁺ and CH, as predicted by a model of a C-type shock propagating in a diffuse interstellar cloud. Both these species are produced in the shock wave in the reaction sequence that is initiated by C⁺(H₂, H)CH⁺. Whilst CH⁺ flows at the ion speed, CH, which forms in the dissociative recombination reaction CH⁺₃(e⁻, H₂)CH, flows at a speed which is intermediate between those of the ions and the neutrals. The predicted velocity shift between the CH⁺ and CH line profiles is found to be no more than approximately 2 km s⁻¹, which is smaller than has previously been assumed. We also investigate OH and HCO⁺, finding that the correlation between their column densities, recently observed in the diffuse interstellar medium, can be reproduced by the model.  相似文献   

Equivalent width, shape and proper motion of the iron fluorescent line emission from molecular clouds as an indicator of the illuminating source X-ray flux history     

R. Sunyaev  & E. Churazov 《Monthly notices of the Royal Astronomical Society》1998,297(4):1279-1291

Observations of the diffuse emission in the 8–22 keV energy range, elongated parallel to the Galactic plane, and detection of the strong 6.4-keV fluorescent line with ∼ 1 keV equivalent width from some giant molecular clouds (e.g. Sgr B2) in the Galactic Centre region suggest that the neutral matter of these clouds is (or was) illuminated by powerful X-ray radiation, which gave rise to the reprocessed radiation. The source of this radiation remains unknown. A transient source close to the Sgr B2 cloud, or a short outburst of the X-ray emission from a supermassive black hole at the Galactic Centre are the two prime candidates under consideration. We argue that a new generation of X-ray telescopes combining very high sensitivity and excellent energy and angular resolutions would be able to discriminate between these two possibilities when studying time-dependent changes of the morphology of the surface brightness distribution, the equivalent width and the shape of the fluorescent line in Sgr B2 and other molecular clouds in the region. We note also that detection of broad and complex structures near the 6.4-keV line in the spectra of distant AGNs, which are X-ray weak now, may prove the presence of violent activity in the central engines of these objects in the past. Accurate measurements of the line shape may provide information on the time elapsed since the outburst. Proper motion (super- or subluminal) of the fluorescent radiation wave front can give additional information on the location of the source. Observations of the described effects can provide unique information on the matter distribution inside Sgr B2 and other giant molecular clouds.  相似文献