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1.
The Heilaigou basin, located in the Inner Mongolia of China, is predominantly influenced by the aeolian-fluvial actions, with complicated sediment transport conditions on the mainstream riverbed. In order to identify the relationship between sedimentary particles and geomorphic processes, mechanisms for the formation of characteristics of grain size composition were investigated by analyzing grain size parameters and external dynamic geomorphologic features. Firstly, the grain size parameters of the riverbed, stream power, maximum grain size of the wind-blown particles and HI values of the mainstream channel were calculated and analyzed, and they were used to establish multiple regression functions of grain size parameters in order to determine the effects of wind and river actions on particles. The results show that sediments in different reaches are formed in different environments: the upper stream is controlled by fluvial and aeolian processes; the sorting properties of riverbed sediments in the middle stream are worse than those in the upper stream since they are affected mainly by fluvial processes as indicated by the larger stream power there; and the particles on the downstream riverbed are likely contributed by the Kubuqi Desert. The size of particles on the riverbed depends on the hydrodynamic conditions, but is not significantly associated with the evolution of landform. Sorting is significantly related to both the hydrodynamic conditions and wind actions. Riverbed deposits brought in by winds likely become finer from the lower to the upper reaches, which are not coarser than 0.88f. Generally speaking, the stream power has a major effect on sedimentation characteristics of the riverbed, followed by wind power.  相似文献   
2.
基于30 m分辨率DEM数据,利用Arc GIS10.0对内蒙古狼山东南坡河流流域地貌参数进行提取,精确计算了其中15条规模较大的北西—南东向河流的面积-高程积分值(HI),并据此对河流发育阶段以及构造运动进行分析。研究结果显示有8条河流的HI值处于0.3~0.6之间,属于河流发展的壮年阶段;7条河流的HI值大于0.6,为幼年期,未出现老年期河流。狼山西南部河流河谷V1—V14的HI值变化平缓,波动幅度不大,构造运动呈现出先增强后减弱的态势;中北部河流V14—V22的HI值变化较剧烈,尤其是V14—V19,呈明显上升趋势,河流受侵蚀后残存体积增多,构造运动活跃性下降;V19以北HI值持续下降,其构造运动的活跃性增加。由此认为狼山从西南到东北总体呈现增强—减弱—增强的差异性运动状态,该结论与前人所做山前构造地貌研究结果较为一致。  相似文献   
3.
We present new results of our kinematic study of the supernova remnant S8 in the galaxy IC 1613. Based on our observations at the 6-m Special Astrophysical Observatory telescope with the two-dimensional MPFS spectrograph and the SCORPIO focal reducer in the mode of a scanning Fabry-Perot interferometer, we have determined the expansion velocity of the bright optical nebula. Analysis of the 21-cm VLA radio observations for the galaxy confirms our previously suggested model for a supernova explosion in a cavity surrounded by a dense HI shell and a collision of S8 with the shell wall.  相似文献   
4.
Observations have been conducted using the Ooty Radio Telescope in order to place constraints on the evolutionary scenario leading to the formation of the present day superclusters. The experiment attempted to detect 21 cm emission from massive neutral hydrogen condensates at a redshift ofz = 3.3. In an Einstein de-Sitter universe with baryon density Ω = 0.05, about ten condensates were expected in the volume surveyed if superclusters, having H I masses ≃5 × 1015 M , were the first objects to separate out of the Hubble expansion. The sensitivity of our experiment rules out the existence of these condensates atz = 3.3 unless their lifetimes are less than one-tenth the dispersion in their epoch of formation or the proto-superclusters subtend angles greater than 6 arcmin. The result indicates that superclusters form at z > 3.3 if indeed they were the first objects to condense out of the Hubble flow. An erratum to this article is available at .  相似文献   
5.
The morphological and velocity structures in the gaseous (HI and CO) and stellar components of two interacting systems are examined. Both Arp 140 and Arp 104 reveal extended tidal tails in the HI. The Hα and FIR fluxes of Arp 140 yield similar SFR of ∼ 0.8 M yr-1. In contrast the Hα flux of Arp 104 yields a SFR of ∼ 0.05 M yr-1, ∼ 20 times smaller than that obtained from the FIR flux. Spectra were used to examine the changing velocity of atomic and molecular gas in NGC 5218 (Arp 104). The atomic and molecular gas were found to be dynamically similar with comparable velocities and velocity widths across the galaxy; consistent with the two phases responding similarly to the interaction, or enhanced HI to CO conversion in the centre of the galaxy. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   
6.
The compact source 0125 + 628 in the centre of the galactic supernova remnant G 127.1 + 0.5 has been re-observed in HI absorption using the Westerbork Synthesis Radio Telescope (WSRT). The outer arm HI absorption atV = -95km s-1 has been confirmed. The absorption spectrum is similar to that of the nearby extragalactic source 0123 + 633. We discuss the arguments concerning an extragalactic origin of 0125 + 628 and conclude that it is most likely extragalactic and not an SS 433 type object. The National Radio Astronomy Observatory is operated by Associated Universities Inc. under contract with the National Science Foundation.  相似文献   
7.
丽江-小金河断裂位于青藏高原东南缘,是川滇菱形块体内重要的次级边界断裂。构造活动对区域河流水系的发育有重要影响,因此,定量研究水系地貌特征可在一定程度上反映区域内构造活动信息。本文采用地形坡度、地形起伏度、面积-高程积分值(HI)等地貌参数研究沿该断裂区域地貌对构造活动的响应。研究发现,断裂北侧坡度和地形起伏度较断裂南侧高,跨断裂4级流域盆地内亚流域盆地面积-高程积分值变化也指示断裂北侧流域成熟度低于断裂南侧,这反映了丽江-小金河断裂存在一定逆冲分量。  相似文献   
8.
海相成熟干酪根生气潜力评价方法研究   总被引:2,自引:0,他引:2       下载免费PDF全文
高成熟阶段干酪根热解氢指数(HI)非常低,在热成熟度指标镜质组反射率Ro为2.0%以上的Ⅰ或Ⅱ型有机质,一般都在20 mg/gTOC以下,甚至接近0 mg/gTOC,因此,一般认为这种干酪根生烃能力极低。本文通过对不同成熟阶段的干酪根采用元素分析和热解模拟实验相结合的方法,发现HI指数很低的高过成熟阶段干酪根仍然具有一定的生气能力,生气潜力是HI指数的数倍,如HI指数为12 mg/gTOC的样品,H/C原子比为046,生气能力仍然为65 mg/gTOC,占总生烃能力的15%左右,说明成熟—过成熟有机质HI指数不适合衡量生气潜力。同时发现,干酪根生气能力与H/C原子比具有极好相关性,相关系数达到096,通过回归公式所获得有效生气干酪根H/C原子比下限为026。  相似文献   
9.
Multi-proxies of lacustrine sediments, such as total carbon (TC), total organic carbon (TOC), total inorganic carbon (TIC), total nitrogen (TN), total sulfur (TS), hydrogen index (HI), oxygen index (OI) and stable carbon isotopic composition of organic matter (δ 13Corg), were analyzed using a 7.3 m core from Zigê Tangco. The source of the organic matter in the sediment was mainly from autochthonous phytoplankton, therefore the significances of proxies can be interpreted as that high TOC, TOC/TS, HI and δ13Corg values, low TC, TIC values corresponded to warm and wet climatic condition, and vice versa. The process of climatic development in the Zigê Tangco region was hence recovered. During the early and Mid-Holocene, the climate was warm and wet and intensive cold events occurred during the periods of 8600 to 8400 cal a BP and 7400 to 7000 cal a BP. In the second half of Holocene, the climate became cold and dry gradually. The palaeoclimatic process during Holocene in Zigê Tangco region matched well with that in Co Ngoin region which is ca 40 km to the south-east. Therefore this palaeoclimatic process represents the Holocene climatic feature in the Central Tibetan Plateau which has the same pattern in the Northern Tibetan Plateau, but the time and duration of some climatic events might be different. We can conclude that in Holocene solar insolation controlled the climatic pattern on the central Tibetan Plateau.  相似文献   
10.
一次冰雹风暴的CINRAD/SA产品分析   总被引:26,自引:8,他引:26       下载免费PDF全文
分析了2002年9月27日发生在山东东阿附近一次冰雹风暴发生、发展各阶段新一代天气雷达CINRAD/SA反射率、平均径向速度等产品的演变过程。在风暴中, 观测到了低层前侧入流缺口、有界弱回波区 (BWER)、中气旋 (M) 等超级单体风暴的特征。中气旋在风暴中维持了约90 min, 通过连续时次各仰角高度风暴相对速度产品的分析, 揭示了中气旋发生、发展和消亡的过程。分析表明风暴跟踪信息 (STI)、冰雹指数 (HI)、垂直积分液态含水量 (VIL)、中气旋 (M) 等产品对冰雹有较好的识别和预报能力。  相似文献   
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