昌马断裂带活动构造地貌之研究

本文根据野外地质调查资料和人工探槽的剖折,并结合¹⁴C年龄数据,讨论了昌马活动断裂带晚更新世晚期以来形成的构造地貌的类型、特征及分期问题.     

Morphological differentiation characteristics and classification criteria of lunar surface relief amplitude

Lunar landforms are the results of geological and geomorphic processes on the lunar surface. It is very important to identify the types of lunar landforms. Geomorphology is the scientific study of the origin and evolution of morphological landforms on planetary surfaces. Elevation and relief amplitude are the most commonly used geomorphic indices in geomorphological classification studies. Previous studies have determined the elevation classification criteria of the lunar surface. In this paper,...     

King of the plains: Lester King's contributions to geomorphology

Lester King was one of the most influential geomorphologists of the twentieth century. He based his interpretations of landforms and landscapes firmly in the concept of parallel scarp retreat, for although he acknowledged the possibility of slope decline in certain lithological and vegetational environments, he used the mechanism little, if at all, in understanding landscape. Rather, pediments and inselbergs, for instance, as well as entire landscapes, were construed in terms of scarp recession.King appreciated and emphasised the evidence provided by plains for the interpretation of landscape. He considered pediplanation (scarp retreat and pedimentation) to be active in all regions where running water is responsible for shaping the land surface. King's studies in denudation chronology are consistent with his commitment to scarp retreat, implicit in which is the possibility of the survival of very old surfaces; though whether old enough to match the realities of landscape is doubtful.King challenged the Davisian scheme of landscape evolution and offered an alternative model that has proved viable in many parts of the world. Whether pedimentation and scarp retreat are necessarily related is however questionable. King devised original explanations for several well known landforms, and though many of his ideas and interpretations have fallen by the wayside he stimulated many of his contemporaries critically to review their assumptions and explanations.     

Topography of a composite relict rock glacier, Ślęża Massif, SW Poland

A detailed geodetic survey and, additionally, a map of slope covers have been carried out for a composite relict rock glacier on the slopes of Mt ?l??a (718 m a.s.l.), Sudetic Foreland, SW Poland. The survey allows one to distinguish the mobilisation, transition and accumulation zones and to define geomorphic features diagnostic for relict rock glaciers such as lateral ridges standing above a central depression, steep margins of the landforms in the transition and accumulation zones, as well as absence of distinct head scarps above. Furthermore, it indicates that the present‐day hydrographic pattern on the surface of relict rock glaciers has been superimposed on the relief inherited from the active landforms. The topography indicates that tension prevailed rather than compression during the development of the rock glaciers. Some of the features, such as small lateral lobes, developed probably as a result of the compressive flow, however. The pattern of the slope cover shows that it developed during activity of the rock glaciers and been modified afterwards due to solifluction.     

The geomorphological features of Jordan

The main landform features of Jordan are considered: elevated plains with step-like topography, ramp (scarp) of the eastern wall of the graben of the Dead Sea and of the Jordan river valley, and the shore area of the Dead Sea with its salt morphostructure. Jordan's relief is compared with the western coast of the Red Sea and with the Western Ghats of the Indostanic Peninsula.     

Influence of structural framework on mountain slope deformation in the Maiella anticline (Central Apennines, Italy)

Relationships between tectonic framework and gravity-driven phenomena have been investigated in an area of the Central Apennines (Italy) characterised by high relief. The north–south, half-dome shaped Maiella anticline lies in the easternmost part of the Apennine fold-and-thrust belt. Its backlimb is bordered by the Caramanico Fault, a normal fault with a maximum downthrown of about 3.5 km that separates the western slope of the Maiella Massif from the Caramanico Valley. The southwestern Maiella area is affected by deep-seated gravitational slope deformation indicated by major double crest lines, down-hill and up-hill facing scarps, a pattern of crossing trenches, bulging at the base of slopes and the presence of different types of landslide and talus slope deposits.The onset and development of deep-seated gravitational slope deformations and the location of Quaternary, massive rockslope failures have been strongly influenced by the structural framework and tectonic pattern of the anticline. Deep-seated gravitational slope deformation at Mt. Macellaro–Mt. Amaro ridge has developed along the Maiella western, reverse slope in correspondence with the anticline axial culmination; it is bordered at the rear by a NNW–SSE oriented, dextral, strike-slip fault zone and has an E–W direction of rock mass deformation. Closer to the southern plunging area of the anticline, gravity-driven phenomena show instead a N–S and NW–SE direction, influenced by bedding attitude.3D topographic models illustrate the relationship between deep-seated gravitational slope deformation and massive rockslope failures. The Campo di Giove rock avalanche, a huge Quaternary failure event, was the result of an instantaneous collapse on a mountaine slope affected by a long-term gravity-driven deformation.     

西藏高原洞穴堆积物的粘土矿物组合特征及其古地理意义

本文通过对西藏高原洞穴堆积物的粘土矿物组合特征的分析,初步探讨了喀斯特地貌形成的古地理环境。喜马拉雅山北坡旧定日东山洞穴堆积物是较温湿的森林草原环境下的产物,新定日西侧遮普若山北坡洞穴堆积物则是在高寒草甸环境下形成的;拉萨西南曲水大佛后溶洞堆积物形成于湿热的亚热带气候环境,而拉萨西山洞穴堆积物却形成于较温湿的草原环境;唐古拉山南坡安多一带的洞穴堆积物则是在高寒的草甸环境下形成的。并以此研讨了西藏高原喀斯特的成因和时代。     

Degradation of unconsolidated Quaternary landforms in the western North America

One of the major goals of geomorphology is to understand the rate of landscape evolution and the constraints that erosion sets on the longevity of land surfaces. The latter has also turned out to be vital in modern applications of cosmogenic exposure dating and interpretation of lichenometric data from unconsolidated landforms. Because the effects of landform degradation have not been well documented, disagreements exist among researchers regarding the importance of degradation processes in the dating techniques applied to exposures. Here, we show that all existing qualitative data and quantitative markers of landform degradation collectively suggest considerable lowering of the surface of unconsolidated landforms over the typical life span of Quaternary moraines or fault scarps. Degradation is ubiquitous and considerable even on short time scales of hundreds of years on steeply sloping landforms. These conservative analyses are based entirely on field observations of decreasing slope angles of landforms over the typical range of ages in western North America and widely accepted modeling of landscape degradation. We found that the maximum depth of erosion on fault scarps and moraines is on average 34% of the initial height of the scarp and 25% of the final height of the moraine. Although our observations are limited to fault scarps and moraines, the results apply to any sloping unconsolidated landform in the western North America. These results invalidate the prevailing assumption of no or little surface lowering on sloping unconsolidated landforms over the Quaternary Period and affirm that accurate interpretations of lichen ages and cosmogenically dated boulder ages require keen understanding of the ever-present erosion. In our view, the most important results are twofold: 1) to show with a large data set that degradation affects universally all sloping unconsolidated landforms, and 2) to unambiguously show that even conservative estimates of the total lowering of the surface operate at time and depth scales that significantly interfere with cosmogenic exposure and lichen dating.     

雁荡山流纹岩地貌景观特征及其形成发育规律

流纹岩地貌有其独有的特色和发育规律。本文根据大量的实地调查数据, 对雁荡山流 纹岩地貌景观进行了类型、空间分布规律和时间发育规律的分析研究。研究结果表明: 区域 流纹岩地貌景观可分为2 个大类, 6 个亚类, 16 个类型单元; 受区域断裂构造的控制, 区内 沟谷和岩嶂在平面上的发育延伸主要沿NE、NW 和EW 三个方向; 在新构造运动和岩性差异 的控制下, 区内峰、嶂、瀑在垂向上的分布具有分带性; 区域现代地貌的发育肇始于晚第三 纪区域一级夷平面的分裂解体, 自此以后的区内地貌演化经历了四个不同发育阶段, 每个阶 段的地貌景观组合各具特色。     

Architecture,formation and implication of active structure-controlled intraslope channel system southeast offshore Sendai,Tohoku, Japan

Located off the Pacific coast of central Tohoku (NE Japan), the Ishinomaki slope channel (ISC) provides an excellent opportunity to study a structure-controlled intraslope channel and downslope sedimentation along the active margin. The seismic reflection data across ISC show an extensive basal surface and overlying channel complexes between the basement structures of the Abukuma ridge to the south and Kitakami massif to the north, indicating that the formation of the intraslope basin, channelization of ISC and sedimentation of the downstream channel-lobe transition zone (CLTZ) are very likely to be structure-controlled. The oblique channel stacking pattern, faulting of the seafloor and subsurface Abukuma ridge in the upper and lower domains of ISC, collectively suggest that ISC has migrated northward and is currently under the influence of active compression. Differences in styles of accommodation space between the upper and lower domains of ISC suggest that differential subsidence occurred along the strike-slip tectonic line. Based on the regional strike-slip tectonic line, we propose that a Kitakami-Abukuma ridge existed before the formation of ISC. The strike-slip faulting divided the Kitakami-Abukuma ridge into the Kitakami massif to the north and the Abukuma ridge to the south, and an intervening fault trough as the precursor of the intraslope basin and ISC. As the subduction of the Pacific Plate and associated compressional events continued, the Abukuma ridge was reactivated to narrow the intraslope basin into a confined channel. Located near the epicentre of the devastating 2011 Tohoku earthquake event, the ISC, downstream CLTZ and underlying intraslope basin provide information on active basement structure and the evolving sediment routing system on the tectonically active margin.     

广东深圳大鹏半岛海岸地貌特征

大鹏半岛位于广东省深圳市东部,海岸地貌类型多样,可分为基岩海岸、堆积海岸和生物海岸3大类型。文章根据野外调查和室内实验分析的结果论述了大鹏半岛海岸地貌类型、分布和成因,并在前人的研究基础上讨论了大鹏半岛海岸地貌演化过程：由于大鹏半岛处在构造隆升区,海岸类型以基岩海岸为主。多处基岩海岸保留了完好的海蚀崖、海蚀平台、海蚀槽穴、海蚀柱等各类典型的海蚀地貌。该半岛的堆积海岸主要发育于岩石岬角间的海湾内,在有河流流入的海湾处形成岬湾沙坝―澙湖海岸,在无河流的海岸处则形成湾顶海滩。半岛中段狭窄的呈哑铃状腰部的东岸,因深入内凹、波浪减弱,有淤泥质海岸发育;红树林发育于淤泥质海岸以及各澙湖内,而半岛周边浅海区有珊瑚群落生长。大鹏半岛以及邻近地区海岸地貌特征和海岸沉积物年代数据显示：1）地质构造与海平面升降是塑造该半岛海岸地貌的主要因素;2）该半岛的海岸地貌是在中全新世早期以后才开始发育的;3）该半岛全新世以来不存在强烈的地壳抬升;4）该半岛海岸中全新世出现过高于现代海平面的高海面。     

五台山冰缘地貌植物群落的数量分类与排序

在野外样方调查的基础上,采用双向指示种分析法(TWINSPAN)和除趋势对应分析法(DCA)对五台山冰缘地貌植被进行了数量分类和排序研究,将五台山冰缘地貌植被分为13个群丛,13个群丛是不同冰缘地貌生态景观的重要组成要素,各群丛的群落学特征与冰缘地貌生境有密切的生态关系。DCA样方排序结果和种排序结果表明,五台山冰缘地貌植物群落分布格局是土壤、水分、热量等综合环境因子决定的。而不同冰缘地貌上植物群丛优势种的分布格局在很大程度上决定着植物群丛类型的分布格局,反映出植物群落类型和物种分布随冰缘地貌类型及环境梯度变化的趋势。     

中国西南山区公路沿线乡村聚落景观格局演变

山区乡村聚落演化机制是聚落地理学研究的热点,为探究山区公路对乡村聚落变化的驱动机理,以贵州省麻江县为研究对象,基于1992,2012年乡村聚落数据,运用GIS技术和景观分析软件,对山区不同地貌的公路沿线乡村聚落景观格局变化进行研究。结果表明:(1)与整个研究区(行政单元)相比,公路影响范围内乡村聚落景观快速增加,景观趋于破碎化和形状复杂化。乡村聚落景观演变速度呈现岩溶槽谷区低山丘陵区中山峡谷区的特点。(2)距公路越近的缓冲区,景观格局变化更加剧烈。在3个公路距离缓冲区,乡村聚落景观演变速度都呈岩溶槽谷区低山丘陵区中山峡谷区的特点。(3)在0~1 500 m距离缓冲区,低坡度的乡村聚落景观格局变化速度明显快于中坡度与高坡度地区。低坡度的景观格局演变速度呈现出岩溶槽谷区低山丘陵区中山峡谷区的特点,而中坡度与高坡度的景观格局演变速度呈现出中山峡谷区低山丘陵区岩溶槽谷区的特点。这说明距公路远近和坡度的变化是影响山区公路影响范围内乡村聚落景观格局演变差异的重要因素。     

古海蚀与相似地形的区别：形态与成因——以广东黄圃海蚀遗迹为例

对比黄圃镇海蚀遗迹与其它非海蚀成因相似地形,得出其形态特征差异:海蚀槽穴同时切过软硬相间的岩石,仅出现在某一水平面;片流和风化作用形成的凹槽与结构面或岩层完全平行而且连续延伸,出现在整个山坡面上,凹槽前无平台;河流侧蚀作用在同一水平面上,不能同时形成凹槽和平台;河流溶蚀作用也是水平的,在石灰岩河岸侧壁形成凹槽,槽上有突出屋檐,无平台;波浪作用不强的石灰岩海岸也可形成凹槽和突出屋檐,但无海蚀平台;只有波浪作用才能同时形成(海蚀)平台和(海蚀)凹穴.     

Geomorphological research of large-scale slope instability at Machu Picchu, Peru

A multidisciplinary approach has been adopted to study the slope movements and landscape evolution at the archaeological site of Machu Picchu and its immediate surroundings. The basic event in the paleogeomorphological evolution of the area was the large-scale slope movement, which destroyed the originally higher ridge between Mt. Machupicchu and Mt. Huaynapicchu. Within remnants of that primary deformation, several younger generations of slope movements occurred. The laboratory analyses of granitoids revealed highly-strained zones on the slopes of Mt. Machupicchu, which strongly affect the largest slope deformation. The borders of the largest slope deformation are structurally predisposed by the existence of fault zones. The majority of various types of slope movements on the so-called Front Slope (E facing) and Back Slope (W facing) are influenced by the alignment between topography and joints. Along with slope movements, fluvial erosion and tectonic disturbance of the rocks have been affecting the evolution of the landscape. A monitoring network for dilatometric and extensometric measurements was used to detect the present-day activity of rock displacements within the archaeological site. In addition to standard mapping of surface hydrogeological phenomena, eleven express slug tests were conducted to verify the infiltration potential of precipitation. The results of these surveys indicate that recent large-scale slope movement as suggested by some previous studies is doubtful, and the detected movements can be explained by individual movements of rock blocks or several other mechanisms including sinking of archaeological structures, subsurface erosion and annual changes in the water content of the soils.     

Simulation of snow shielding corrections for cosmogenic nuclide surface exposure studies

Snow cover reduces cosmogenic nuclide production rates in bedrock. Corrections for snow cover can be more than 10% in mountainous, mid-latitude regions where many glacial chronologies have been constructed using cosmogenic nuclide surface dating of landforms. Most published snow corrections use historic climate data of limited duration that are not likely to reflect adequately the full range of snow conditions over the time of exposure. We present a model for describing the impact of snow burial on long-term exposure histories of landforms. The model applies an energy balance approach to snowpack evolution and incorporates both historic and long-term climate proxy data. Attenuation of cosmogenic fast neutrons is modeled alternatively as a simple exponential decrease with increased shielding or as a thin surface layer with constant production followed by an exponential decrease with increasing depth. The choice of attenuation model has little effect on the modeled results for the Cairngorms but will have a more significant effect in regions characterized by thinner, less dense snowpacks. Spatial variability in snow cover is modeled as a function of elevation only, ignoring local variability in snow accumulation as a result of slope aspect, wind redistribution and local topography. Thus, model results reveal general spatial and temporal trends in snow shielding effects, rather than site-specific corrections.Applications to data from the Cairngorm Mountains of Scotland show that the constant-plus-exponential (CPE) production rate-depth profile reduces but does not eliminate snow-shielding effects. Under present-day conditions, snow at 900 m in the Cairngorm Mountains reduces average production rates by 6% using the CPE profile and 9% with the exponential profile (EP). Long-term climate simulations from 15.5 ka through today produce larger snow shielding effects, mainly because they predict an increased proportion of precipitation as snowfall during the Younger Dryas. At 900 m, this long-term simulation reduces average cosmogenic isotope production rates by 12% (CPE) and 14% (EP). These results indicate that snow-shielding corrections based on historic climate records may be a potential source of systematic error in midlatitude mountainous regions.     

Planation, bauxites and epeirogeny: One or two paleosurfaces on the West African margin?

Mapping of lateritic bauxites over the West African rifted margin and analysis of the geomorphic properties of these bauxites, combined with available geological data lead to a discussion of the presence of either two Meso-Cenozoic planation surfaces or a single Eocene surface to account for the morphotectonic and paleoclimatic evolution of the Guinean landforms. At large scale, two stepped bauxitic levels are documented. Ongoing or episodic uplift following Gondwana breakup and Meso-Cenozoic climate change are proposed to have allowed the formation and abandonment of an Early mid-Cretaceous surface today preserved as the higher bauxitic level, and the setting of an Eocene planation surface bearing a second generation of bauxites, making the lower bauxitic level. The single Eocene surface hypothesis requires that Paleogene bauxitization preserved large pre-existing relief to explain two stepped bauxitic levels of the same age. The two-surface hypothesis is favored because it would explain rebauxitization of alluvial pebbles of bauxites under the lower lateritic level.     

DEM-based morphometry of range-front escarpments in Attica, central Greece, and its relation to fault slip rates

In this paper, we apply current geological knowledge on faulting processes to digital processing of Digital Elevation Models (DEM) in order to pinpoint locations of active faults. The analysis is based on semiautomatic interpretation of 20- and 60-m DEM and their products (slope, shaded relief). In Northern–Eastern Attica, five normal fault segments were recognized on the 20-m DEM. All faults strike WNW–ESE. The faults are from west to east: Thriassion (THFS), Fili (FIFS), Afidnai (AFFS), Avlon (AVFS), and Pendeli (PEFS) and range in length from 10 to 20 km. All of them show geomorphic evidence for recent activity such as prominent range-front escarpments, V-shaped valleys, triangular facets, and tilted footwall areas. However, escarpment morphometry and footwall geometry reveal systematic differences between the “external” segments (PEFS, THFS, and AVFS) and the “internal” segments (AFFS and FIFS), which may be due to mechanical interaction among segments and/or preexisting topography. In addition, transects across all five escarpments show mean scarp slope angles of 22.1°±0.7° for both carbonate and metamorphic bedrock. The slope angle equation for the external segments shows asymptotic behaviour with increasing height. We make an empirical suggestion that slope angle is a function of the long-term fault slip rate which ranges between 0.13 and 0.3 mm/yr. The identified faults may rupture up to magnitude 6.4–6.6 earthquakes. The analysis of the 60-m DEM shows a difference in fault patterns between Western and Northern Attica, which is related to crustal rheology variations.     

An earthquake swarm on the Chagos—Laccadive Ridge and its tectonic implications

Summary. An unusual, isolated swarm of earthquakes occurred on the Chagos-Laccadive Ridge in the Central Indian Ocean between 1965 and 1970. Sixteen earthquakes were "located at approximately 6.0° S, 71.3°E on the steep west facing scarp of the Chagos Bank. This swarm forms the only major seismic activity in the period 1963–76 on the otherwise aseismic ridge. The mechanisms of the three largest earthquakes were studied using body- and surface-wave data. All are extremely similar shallow normal fault events on an east—west fault plane. Such faulting is difficult to reconcile with that expected from either the trend of the Chagos-Laccadive Ridge or the spreading direction at the nearby Central Indian Ridge. The swarm may have occurred at depth on a cross fracture remaining from the breakup of the Chagos Bank and the Mascarene Plateau and the formation of the present Central Indian Ridge.     

月表地貌起伏形态分异特征及分级标准研究

月球地貌是月球表面发生的地质和地貌过程的结果,月球地貌单元的划分和等级分类体系的构建是月球地貌学研究的基础,也是月球地貌图制图的基础和关键科学问题。地貌学是研究形态和成因的科学,高程和起伏度是最基本的地貌指标。本文基于LOLA（Lunar Orbiter Laser Altimeter） DEM数据以及LOLA和SELENE TC（Terrain Camera）融合的DEM数据（SLDEM2015,文中简称SLDEM）,利用均值变点法确定月表起伏度计算的最佳窗口,并以起伏度100 m、200 m、300 m、700 m、1500 m及2500 m为阈值将月球表面分为微起伏平原（< 100 m）、微起伏台地[100 m, 200 m）、微小起伏丘陵[200 m, 300 m）、小起伏山地[300 m, 700 m）、中起伏山地[700 m, 1500 m）、大起伏山地[1500 m, 2500 m）及极大起伏山地（≥ 2500 m）地貌7个类型。划分结果显示：微起伏平原主要分布在月海平原区域、部分有玄武岩充填的撞击盆地的盆底区域以及撞击坑坑底区域;微起伏台地主要分布在月海和月陆区域的交界区域;微小起伏丘陵主要分布在月溪和皱脊等构造单元区域;小起伏山地主要分布在撞击坑中央峰及坑底断裂区域;中起伏山地主要分布在撞击坑坑底和坑壁过渡区域、撞击坑坑壁和坑缘过渡区域、撞击盆地盆底与盆壁过渡区域以及盆壁与盆缘过渡区域;大起伏和极大起伏山地主要分布在撞击坑坑壁区域及撞击盆地盆壁区域。本文确定的月表起伏度分级标准可以对月表数字地貌分类体系的构建和月球地貌图集的编研提供定量标准和重要参考。