InSAR复数影像配准方法探讨

复数影像配准是卫星合成孔径雷达干涉数据处理中的重要步骤之一,本文对目前影像配准最常用的方法进行了研究分析,提出了基于幅度影像的配准方案,并证明该方案配准精度高,适应能力强,运算效率高.     

大别山黄石-六安反射地震剖面新的地质解释

在大别山黄石至六安反射地震剖面上有很多近水平的反射体,表明大别山中心部位的中、下地壳内也有近水平的分层性。反映有流变性和动力学方面的差异,与大型薄皮构造理论对岩石圈性质的认识一致,因而在其运动过程中应服从薄皮构造的运动规律。结合以往对大别山区划分的岩石一构造组合,在前人对此反射地震剖面所作的地质解释的基础上,对反射地震剖面作了较为详细的地质解释,并建立了大别山造山带在此剖面上的两维几何结构。剖面南部为造山过程中形成的背斜构造。地表15km深度内为由碰撞混杂岩组成的扬子与中一朝大陆之间的主滑脱带。剖面中部为造山期后的侵入体。剖面北部为主滑脱带的根带（通常认为的缝合带）,根带被中生代形成的晓天磨子潭断裂带切割。剖面最北端为变质复理石中略晚于主滑脱带的反向冲断带。推溺l下地壳的断开距离在扬子大陆俯冲时（三叠纪前）规模较大,然后逐渐缩小,直至保留到今天的规模。     

应用探地雷达探测活动断层

在浅覆盖区采用探地雷达探测地震活动断层。通过实验确定出最佳的采集参数和数据处理流程,在雷达剖面上,能够清晰地显示出断层上部的形态特征、上断点埋深和岩土分层。结合钻孔资料,利用雷达剖面上对第四系覆盖的分层结果和上断点所在的层位可以分析和评价断层的活动性。     

青藏高原锡铁山—格尔木—亚东剖面地温分布特征

以青藏高原锡铁山—格尔木—亚东剖面作为研究对象,测定不同深度土层的温度。结果表明,除北部柴达木地块地温高出其它地块外,该剖面总体上呈现出青藏高原各地块地温状况南高北低的现象:以拉萨—冈底斯地块的地温为最高,其次为喜马拉雅地块,北部的羌塘地块、可可西里-巴颜喀拉地块、昆仑地块的地温依次降低。测量结果较好地对应于各地块及断裂带的划分,断裂带温度明显高出相邻低温地块温度,并且以狮泉河—雅鲁藏布江断裂带为最高。该试验方法较好地反映了青藏高原热活动状况,为青藏高原热动力学研究提供了依据。     

The origin of accretionary lapilli

Experimental investigations in a recirculating wind tunnel of the mechanisms of formation of accretionary lapilli have demonstrated that growth is controlled by collision of liquid-coated particles, due to differences in fall velocities, and binding as a result of surface tension forces and secondary mineral growth. The liquids present on particle surfaces in eruption plumes are acid solutions stable at 100% relative humidity, from which secondary minerals, e.g. calcium sulphate and sodium chloride, precipitate prior to impact of accretionary lapilli with the ground. Concentric grain-size zones within accretionary lapilli build up due to differences in the supply of particular particle sizes during aggregate growth. Accretionary lapilli do not evolve by scavenging of particles by liquid drops followed by evaporation — a process which, in wind tunnel experiments, generates horizontally layered hemispherical aggregates. Size analysis of particles in the wind tunnel air stream and particles adhering to growing aggregates demonstrate that the aggregation coefficient is highly grain-size dependent. Theoretical simulation of accretionary lapilli growth in eruption plumes predicts maximum sizes in the range 0.7–20 mm for ash cloud thicknesses of 0.5–10 km respectively.     

Structure and energy transfer of unstable hot star winds

Due to the instability of the radiation line force, the winds of hot, luminous stars should show a pronounced time-dependence resulting from the nonlinear growth of initially small perturbations. Following the method of Owocki, Castor & Rybicki (1988), we describe the time-dependent wind structure obtained with an independently developed code. Under the central assumption ofisothermality, our results are in very good agreement with the ones by Owocki et al. We find that the response of the wind to periodic base perturbations remains largely periodic, at least up tor 2...3R _* , with no clear evidence of stochastic behaviour.In order to test the foregoing assumption of isothermality and to compute the X-ray emission from models of structured winds, we have also incorporated theenergy equation into our simulations. We encountered the numerical problem that all radiative cooling zones collapse because of the oscillatory thermal instability (cf. Langer et al. 1981). We present a method to hinder this collapse by changing the cooling function at low temperatures. The resulting wind showsresolved cooling zones; but, for a supergiant wind relatively close to the star (r 10R _* ), the macroscopic wind structure is very similar to isothermal calculations. Most of the hot material is caused by shell-shell collisions.     

新疆地区夏季平流层低层风场特征分析及数值模拟

利用2017年6—8月的FNL再分析资料分析了新疆地区夏季平流层低层风场的时空演变特征，开展了平流层低层风场的高分辨率数值模拟和检验。结果表明：新疆地区夏季平流层纬向风随时间的变化存在经向差异，同时准零风层开始和结束的时间也存在经向差异，准零风层开始时间南部地区早于北部地区，而准零风层结束时间则相反。整个夏季新疆地区上空的准零风层处于70～40 hPa之间，其高度随时间呈先降低而后升高的变化趋势。准零风层数值模拟结果表明，模拟的准零风层参数与探空资料分析结果相比二者存在一致的变化趋势，准零风层起始高度的平均绝对误差为467 m，该高度对应的风速均方根误差为1.75 m/s。     

鄂北一次超级对流单体的双偏振雷达特征分析

利用湖北省随州市S波段双偏振雷达资料及常规观测资料，对2020年5月4日鄂北随州出现的超级单体风暴进行分析。结果发现：①在有利天气背景作用下，形成了上干冷下暖湿的垂直层结、0~6 km中等强度垂直风切变以及地面辐合线，为强风暴的发生发展提供环境条件和触发条件。②超级单体发展过程中，观测到前侧“V”形入流缺口、中气旋、弱回波穹隆、悬垂回波、钩状回波等特征，且风暴顶高度、风暴质心高度、最大水平反射率因子高度以及垂直累积液态含水量等风暴参数均呈先升后降趋势。③超级单体的发展和成熟阶段，在0 ℃层以下的低层，于前侧下沉气流西侧的水平反射率因子大梯度区观测到浅薄的差分反射率因子Zdr大值区，即Zdr弧；④超级单体的初始阶段、发展阶段以及成熟阶段，在0 ℃层之上的中层，观测到强上升气流的正温度扰动使冰相粒子在附近融化而形成的Zdr环形大值区和相关系数环形小值区。⑤垂直方向上，在超级单体的初始阶段、发展阶段以及成熟阶段均观测到Zdr柱和差分相位常数Kdp柱。Zdr柱与弱回波穹隆区位置对应较好，其不同时期特征反映了上升气流强的变化；Kdp柱的变化反映了超级单体中含有大量液态水滴区域的变化。     

Airborne gamma-ray spectrometry to quantify chemical erosion processes

Airborne gamma-ray spectrometry data (uranium, potassium and thorium contents) reveal geochemical heterogeneities within the monolithological Hyrôme watershed (ca. 150 km²) in the Armorican massif (western France). Our observations and computations provide important constraints on the spatial distribution and the associated magnitudes of chemical erosion processes at the scale of a small watershed. Two distinct, partially preserved, weathering profiles exhibit a strong correlation between regolith evolution and airborne-derived K/Th ratios, suggesting that the variability is linked to supergene processes. Using both airborne data and laboratory measurements on rock samples, the total net export of potassium has been estimated at 422 ± 50 kg/m² and the chemical weathering rate of potassium at 17 ± 2 kg/km²/a.     

Threshold velocity for wind erosion: the effects of porous fences

Porous fence is a kind of artificial windbreak that has many practical applications. The threshold wind velocities at different distances downwind from porous fences were measured and the corresponding characteristics of particle movement observed to assess their shelter effect. It is found that the fence’s porosity is the key factor that determines the resulting shelter effect. The area near a fence can be typically classified into five regions, each with a different mode of particle movement. Dense fences, and especially solid fences, favor the accumulation of sand upwind of the fences. Fences with porosities of 0.3–0.4 produce the maximum threshold wind velocity; those with porosities of 0.3–0.6 (depending on the fence height) provide the maximum effective shelter distance. It is confirmed that the fence porosities of 0.3–0.4 that have been proposed for practical application in previous research are the most effective for abating wind erosion.