基于水准剖面的山西断陷带现今活动性研究     

陈阜超  塔拉  陈聚忠 《大地测量与地球动力学》2015,35(4):576-580

根据跨山西断陷带的水准剖面观测资料,计算其垂直形变量和垂直形变速率,研究其现今垂直活动性。2006年以来的垂直形变揭示,山西断陷带东北段延怀盆地和蔚县盆地呈掀斜上升活动,北段阳原盆地和大同盆地以下降活动为主,晋中盆地为上下波动,临汾盆地呈现上升活动。2013年山西断陷带活动出现转折性变化,蔚县盆地大幅度下降,大同盆地、代县-定襄盆地、晋中盆地和临汾盆地均呈现不同程度的上升。  相似文献   

北京地区主要活断层活动参数的重力反演     

董运洪  刘峡  韩月萍  杜雪松  塔拉 《地震研究》2014,37(3)

采用1991~1999年首都圈重力测网的重力测量资料,根据地质调查结果确定断层初始运动模型,利用稳健—贝叶斯最小二乘方法反演北京地区4条活断层的活动参数(走滑、倾滑、引张)。反演结果表明:在1991~1999年间,北京地区活断层的运动性质均以走滑和垂直升降为主,兼有伸展特征,但运动速率都不大,约为2 mm/a。北京地区北西走向断层反演的运动特征为左旋走滑正断层,北东走向断层反演的运动特征为右旋走滑正断层。  相似文献   

Strike-slip fault patterns on Europa: Obliquity or polar wander?     

Alyssa Rose Rhoden  Terry A. Hurford 《Icarus》2011,211(1):636-647

Variations in diurnal tidal stress due to Europa’s eccentric orbit have been considered as the driver of strike-slip motion along pre-existing faults, but obliquity and physical libration have not been taken into account. The first objective of this work is to examine the effects of obliquity on the predicted global pattern of fault slip directions based on a tidal-tectonic formation model. Our second objective is to test the hypothesis that incorporating obliquity can reconcile theory and observations without requiring polar wander, which was previously invoked to explain the mismatch found between the slip directions of 192 faults on Europa and the global pattern predicted using the eccentricity-only model. We compute predictions for individual, observed faults at their current latitude, longitude, and azimuth with four different tidal models: eccentricity only, eccentricity plus obliquity, eccentricity plus physical libration, and a combination of all three effects. We then determine whether longitude migration, presumably due to non-synchronous rotation, is indicated in observed faults by repeating the comparisons with and without obliquity, this time also allowing longitude translation. We find that a tidal model including an obliquity of 1.2°, along with longitude migration, can predict the slip directions of all observed features in the survey. However, all but four faults can be fit with only 1° of obliquity so the value we find may represent the maximum departure from a lower time-averaged obliquity value. Adding physical libration to the obliquity model improves the accuracy of predictions at the current locations of the faults, but fails to predict the slip directions of six faults and requires additional degrees of freedom. The obliquity model with longitude migration is therefore our preferred model. Although the polar wander interpretation cannot be ruled out from these results alone, the obliquity model accounts for all observations with a value consistent with theoretical expectations and cycloid modeling.  相似文献   

A high-amplitude thermal inertia anomaly of probable magnetospheric origin on Saturn’s moon Mimas     

C.J.A. Howett  J.R. Spencer  R.E. Johnson  T.A. Hurford  M. Segura 《Icarus》2011,216(1):221-226

Spectral maps of Mimas’ daytime thermal emission show a previously unobserved thermal anomaly on Mimas’ surface. A sharp V-shaped boundary, centered at 0°N and 180°W, separates relatively warm daytime temperatures from a cooler anomalous region occupying low- to mid-latitudes on the leading hemisphere. Subsequent observations show the anomalous region is also warmer than its surroundings at night, indicating high thermal inertia. Thermal inertia in the anomalous region is , compared to < outside the anomaly. Bolometric Bond albedos are similar between the two regions, in the range 0.49-0.70. The mapped portion of the thermally anomalous region coincides in shape and location to a region of high-energy electron deposition from Saturn’s magnetosphere, which also has unusually high near-UV reflectance. It is therefore likely that high-energy electrons, which penetrate Mimas’ surface to the centimeter depths probed by diurnal temperature variations, also alter the surface texture, dramatically increasing its thermal inertia.  相似文献   

太阳黑子活动与新疆强震活动的关系     

杨马陵  塔青 《内陆地震》2012,26(1):10-16

使用1900年以来的太阳黑子数据,统计分析了其与新疆地区MS≥6.6强震的关系。结果显示：新疆地区69%的MS≥6.6和86%的MS≥7的地震,发生在黑子数月均值≤35的时段内。以黑子数月均值≤20和≤35的时段作为MS≥6.6强震的预测指标,报准率分别为71%和64%;以黑子数月均值≤35的时段作为MS≥6.6强震的预测指标,报准率为69%。R值评分检验表明,上述预测指标是有效的。最后使用这些统计关系和指标对新疆未来几年发生强震的可能性作了估计。  相似文献   

中国时空间行为研究进展   总被引：11，自引：4，他引：7  

柴彦威  塔娜 《地理科学进展》2013,32(9):1362-1373

自时间地理学和活动分析法引入中国以来的近20年间,时空间行为研究已经成为中国城市地理学的重要领域。中国时空间行为研究关注城市空间重构的描述与解释,试图从行为角度解释中国城市社会转型,强调转型期中国城市空间与居民个体行为之间的互动关系,重视日常生活、生活质量、社会公正、低碳社会、智慧城市等热点问题,探索在城市交通、旅游和城市规划等领域中的实践应用。中国时空间行为研究已经形成了以解读城市转型为目标、以规划应用为导向的鲜明特点,为理解中国城市制度与空间转型背景下人类行为模式的复杂性和多样性提供了一个全新的视角。但是,中国时空间行为研究依然面临着理论发展滞后、实践应用需要突破等挑战。本文是对时空行为研究近年来发展的综述性文章,从数据采集与分析方法演进、实证研究与规划应用进展等方面回顾了近20年来中国城市时空间行为研究的最新进展,致力于推动不同学科领域之间的交流和时空间行为研究自身的发展。  相似文献   

地磁数据处理与地震关系之探   总被引：1，自引：0，他引：1  

马钦忠  塔青  王炜  林命周  吴耿锋  吴绍春 《华南地震》2008,28(3):21-30

研究了上海崇明、佘山和杭州这3个地磁台的观测资料在2004年4月21日南黄海ML4．0级、5月26日浙江省舟山群岛ML4．3级和11月15日南黄海％4．6级地震前的异常变化特征,结果表明：杭州台和崇明台数字化地磁观测资料分钟值空间差值于4月14日～17日、4月30日、5月8日出现的异常信息很可能是震磁异常信息;杭州台和余山台数字化地磁观测资料分钟值、模拟观测21时值Z分量地磁场相关系数R值分别在震前2天、24天和震前5天、15天出现了超出2σ值的震磁异常变化：崇明和余山地磁台数字化地磁Z分量分钟值的空间差值异常信息在4月21日南黄海尬4．0级地震前后有所显示。但在5月26日舟山群岛ML4．3级地震前不太明显,可能与谈两个地磁台站相距较近日震中距较近有美．  相似文献   

首都圈地区现今地壳垂直形变特征   总被引：1，自引：1，他引：0  

韩月萍  杨国华  董运宏  塔拉 《华北地震科学》2009,27(1):13-16

利用首都圈地区1998、2001、2005、2007年151期精密水准复测资料,分析该区近十年来地壳垂直形变状态与动态特征。结果表明,形变场以继承性运动为主,即山区上升、盆地及平原下降。值得注意的是首都圈西部地区等值线分布密集有序,有些象限图形特征,东西升,南北降,其最大差值为10mm／a,可能预示该区应力场处于逐步积累及有所加强的势态,虽然异常形变数值及所涉面积均较小,但仍需跟踪关注。  相似文献   

Gamma-ray and hard X-ray imaging of solar flares     

T. A. Prince  G. J. Hurford  H. S. Hudson  C. J. Crannell 《Solar physics》1988,118(1-2):269-290

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Cycloidal cracks on Europa: Improved modeling and non-synchronous rotation implications     

T.A. Hurford  R. Greenberg 《Icarus》2007,186(1):218-233

Cycloidal crack patterns on Europa are influenced by tides induced by orbital eccentricity, which in turn is driven by the Laplace orbital resonance. Their shapes potentially record the location of their formation (relative to the direction of Jupiter), as well as the parameters of crack formation. Hoppa et al. [Hoppa, G., Tufts, B.R., Greenberg, R., Geissler, P., 1999a. Icarus 141, 287-298] modeled several cycloid chains using a fixed set of material parameters, but some details did not fit. We now allow material parameters to vary for each arc of an observed cycloid. In general, with minimal variation of model parameters between the arcs, fits are greatly improved. Furthermore, accounting for tidal stress accumulated during non-synchronous rotation, in addition to diurnal stress, allows even better fits. Even with the added freedom in the model our fits allow us to better constrain the location where each cycloid may have formed. Our results support Hoppa et al.'s finding that only a few cracks form ridges per cycle of non-synchronous rotation in the region examined, probably because cracking relieves built up stress until further substantial rotation occurs.  相似文献