Monitoring Muztagh Kuksai glacier surface velocity with L-band SAR data in southwestern Xinjiang, China   总被引：1，自引：1，他引：0  

Shiyong Yan  Huadong Guo  Guang Liu  Wenxue Fu 《Environmental Earth Sciences》2013,70(7):3175-3184

This study presents the results of measuring surface velocity fields of alpine glaciers with multi-temporal ALOS/PALSAR synthetic aperture radar (SAR) data using the normalized cross-correlation technique. The main limitations of spaceborne optical data and interferometric SAR for retrieving reliable interferometric product are firstly discussed. Next, an efficient method of deriving surface velocity with spaceborne SAR system using the intensity-tracking method based on the cross-correlation optimization is expounded. This method is an invaluable alternative way of estimating the glacier surface field when the differential SAR interferometry is limited by the loss of coherence and can also overcome the drawback of the lack of available optical data in alpine glacier areas. The method was successfully applied in the region of the Muztagh Kuksai Glacier using ALOS/PALSAR L-band data with 44 days temporal separation. The glacier surface velocity fields were obtained for two different time intervals (14 January to 11 March 2009 and 1 September to 17 October 2009). The accuracy of the method was estimated from the residual value in the non-glacier area, which is often used to evaluate the performance of the approach for monitoring the glacier surface velocity. Finally the distribution maps of the surface velocity fields on the Muztagh Kuksai Glacier were retrieved with an accuracy of 0.3 m (SD 0.2 m) using L-band spaceborne SAR data. The results show that overall average velocity for 1 September to 17 October in 2009 is about 11 % faster than that for 14 January to 11 March in 2009. It is concluded that the potential of monitoring the long-term evolution of glaciers with SAR data should be emphasized.  相似文献   

新疆阿尔泰塔拉特铁铅锌矿床流体包裹体研究及矿床成因   总被引：4，自引：1，他引：3  

李登峰  张莉  郑义 《岩石学报》2013,29(1):178-190

塔拉特铁铅锌矿位于新疆阿尔泰造山带南缘的阿巴宫多金属成矿带,矿体赋存于克兰盆地下泥盆统康布铁堡组中,为一套海相中酸性火山岩-火山碎屑岩、陆源碎屑沉积岩-碳酸盐岩建造,脉状矿体受阿巴宫大断裂次级断裂控制.根据矿物组合和脉体穿插关系,塔拉特铁铅锌矿可分为4个成矿阶段:矽卡岩,氧化物,硫化物和碳酸盐阶段,后3个阶段均有石英共生.其中,硫化物(方铅矿-闪锌矿±磁黄铁矿±黄铜矿)阶段是铅锌成矿的主要阶段.不同阶段石英中广泛发育流体包裹体,可分为水溶液包裹体(W型)、纯CO2包裹体(PC型)、CO2-NaCl-H2O包裹体(C型)及含子矿物多相包裹体(S型)4类.冷热台显微测温和激光拉曼分析表明,氧化物阶段石英含有4种类型的包裹体,以W型为主,C型和S型包裹体次之,包裹体均一温度介于271～ 426℃,W型和C型盐度范围0.5％～22.4％ NaCleqv,S型包裹体盐度30.5％ ～40.6％ NaCleqv;硫化物阶段的石英流体包裹体为W型、C型和PC型,均一温度为204 ～ 269℃,盐度介于0.2％～15.6％ NaCleqv之间;碳酸盐阶段的矿物只含W型包裹体,均一温度集中在175～211℃之间,盐度为1.1％ ～9.9％ NaCleqv.利用C型包裹体对硫化物阶段成矿压力估算,得到107 ～ 171MPa,对应深度为4～6km.塔拉特铁铅锌矿初始成矿流体具有高温、高盐度、富CO2的特征,但碳酸盐阶段低盐度、贫CO2,流体不混溶和混合作用导致了成矿物质的沉淀.塔拉特铁铅锌矿的地质和成矿流体特征显示其为碰撞造山体制形成的矽卡岩型成矿系统.  相似文献   

西昆仑塔什库尔干布伦阔勒群的岩石地球化学特征及变质P-T轨迹   总被引：1，自引：1，他引：0  

刘文平  王核  仝来喜  吴玉峰  黄朝阳  胡军 《岩石学报》2013,29(3):923-937

西昆仑布伦阔勒群变质岩是西昆仑造山带的重要组成部分,但其成因一直存在争议.在塔什库尔干县的马尔洋地区,布伦阔勒群主要由石榴斜长角闪片麻岩和孔兹岩组成.根据地球化学特征,石榴斜长角闪片麻岩稀土元素配分曲线可以分为两种类型:一种稀土总量较高(∑REE=190.2×10-6 ～ 359.1×10-6),从轻稀土到重稀土逐渐亏损((La/Yb)N =4.28～5.79),与E-MORB类似;另一种稀土总量较低(∑REE=89.28×10-6～113.0×10-6),轻稀土亏损((La/Yb)N=0.59 ～0.84),重稀土曲线平坦((Gd/Yb)N =0.99 ～ 1.07),与N-MORB类似.微量元素蛛网图中石榴斜长角闪片麻岩具有Ba正异常,Sm、Cr、Zr、Hf和Ti的负异常,轻微的Nb、Ta的负异常,显示为岛弧拉斑玄武岩的特征.孔兹岩的原岩判别图解显示其原岩可能为岛弧环境沉积的页岩和硬砂岩.因此,推测塔什库尔干布伦阔勒群的石榴斜长角闪片麻岩和孔兹岩的原岩形成于岛弧环境.根据岩相学观察、矿物化学分析和温压计算,石榴斜长角闪片麻岩经历了三个变质阶段:M1为高压变质阶段,矿物组合为Grt+ Hbl(1)+ Pl1+ Qtz,变质温压条件为850～ 870℃/12.9 ～13.3kb;M2和M3为两期角闪岩相退变质阶段,矿物组合分别为Hbl2+ Pl2+Qtz和Hbl3+ Pl3+ Kfs+ Bt+ Qtz,变质温压条件分别为730 ～ 770℃/7.3～7.8kb和680 ～ 740℃/4.7 ～5.7kb.孔兹岩也经历了三个变质阶段,推测其早期M1阶段变质温压条件可能与石榴斜长角闪片麻岩的峰期变质阶段相同(850～870℃/12.9 ～ 13.3kb);峰期M2和峰期后M3阶段变质矿物组合分别为Grt2+ Pl2+ Bt2+ Sil+ Qtz和Grt3+ Pl3+ Bt3+Sil+ Mus+ Qtz,温压计算结果分别为800～830℃/7.9～9.2kb和670～700℃/5.1～5.6kb.孔兹岩的M1、M2和M3变质阶段对应于石榴斜长角闪片麻岩的M1、M2和M3变质阶段.上述温压计算结果形成顺时针的P-T轨迹,表现为峰期高压变质作用后叠加了由高角闪岩相-中压麻粒岩相到低角闪岩相的退变质作用,反映了西昆仑与碰撞相关的大地构造背景,这可能与海西期古特提斯洋的闭合有关,之后叠加了印支期构造抬升过程中的剪切作用.  相似文献   

三峡水库气候效应及2006年夏季川渝高温干旱事件的区域气候模拟   总被引：10，自引：1，他引：10  

吴佳  高学杰  张冬峰  石英  GIORGI F 《热带气象学报》2011,27(1):44-52

针对2006年夏季川(四川)渝(重庆)地区的高温干旱事件，使用RegCM3区域气候模式，采用双重嵌套和次网格(SUB-BATS)方法，进行中国和三峡地区2005—2006年气候50 km和10 km(通过SUB-BATS方法达到2 km)分辨率数值模拟，并在此基础上进行了三峡地区下垫面改变(三峡水库建成蓄水)的气候效应模拟试验，重点分析了模式对中国和三峡地区夏季气候和气候异常的模拟能力，以及三峡水库对气温和降水的影响。结果表明，模式能较好模拟出中国和川渝地区的气候及以2006年川渝地区高温干旱为代表的气候异常，双重嵌套和SUB-BATS方法的应用，使模式能够提供局地和区域气候更详细的信息。有无三峡水库的对比试验表明，水库对周边区域气温、降水的影响很小，大部分格点上的变化达不到90%统计信度检验标准，气温变化中少数通过检验的格点基本集中于水库水体本身，邻近区域内气温和降水的变化随距库区的距离变远而变得更弱。除了库区本身降温和降水减少外，模拟结果中出现的变化更多表现为模式中出现的噪音。2006年夏季的川渝高温干旱，更多是由于大的环流场造成的，与局地强迫的关系不大，三峡水库在其中所起的作用非常微弱，可以忽略不计。  相似文献   

青海省兴海县索拉沟铜多金属矿成矿地质特征与矿床成   总被引：1，自引：0，他引：1  

燕宁  李社宏  陆智平  王飞  李发明 《大地构造与成矿学》2011,35(1):161-166

通过对索拉沟铜多金属矿床的矿体特征、矿石组成、围岩蚀变特征分析和论述,以及对矿石的硫、铅同位素和包裹体均一温度的测试,结果显示矿石硫同位素834S值变化于-3.91‰-4.42‰,具有深源特征;铅同位素投影在造山带铅附近,模式年龄与区域中酸性岩体基本一致;矿物包裹体爆裂法测温范围在270℃-365℃间,反映成矿过程是一...  相似文献   

The early phase of multiple proto-stellar system emerging from collapse of molecular cloud under various initial thermal states     

Rafil Riaz  Suhail Zaki Farooqui  Siegfried Vanaverbeke 《Astrophysics and Space Science》2013,347(2):327-335

We report on the short timescale intensity fluctuations of PSR B1133+16 and PSR B1237+25 due to scintillation at 1.54 GHz. The structure functions of intensity fluctuations are constructed and the linear fittings are applied to the structure regime in log–log plots to get the slope values. The slope of the SFs for PSR B1237+25 are less than that of PSR B1133+16, and both of them are much less than 2. For PSR B1133+16, the slope values agree very well with a Kolmogorov spectrum predicted value 5/3, whereas PSR B1237+25 not. We investigate the dynamic spectrum and obtain its auto-correlation function (ACF). Scintillation parameters are obtained by fitting to the autocorrelation function of the dynamic spectrum. The observed diffractive interstellar scintillation (DISS) timescales agree well with the observations and are consistent with some expected values, but the observed de-correlation frequency bandwidths are much less than predicted ones. The expected refractive interstellar scintillation (RISS) timescales are also estimated by using our derived diffractive scintillation parameters. They are consistent with the timescales of slow pulse intensity fluctuations. We proposed that the short timescale of pulse intensity variations caused by the DISS are modulated by the slow variations due to the effects of RISS.  相似文献   

一种基于GNSS的可驯频标的设计与实现     

张帆  胡永辉  何在民 《时间频率学报》2013,36(1):28-32,53

重点介绍了GNSS可驯频标软件设计方法。在软件设计中,采用了滑动中位数方法以滤除测量数据中的奇异值;利用了Kalman滤波器对测量时差数据进行滤波以抑制测量噪声;提出了一种改进型的压控电压产生方法。采用GPS定时接收机1 PPS信号作为参考基准,对原来准确度为1×10-9恒温晶振进行驯服,驯服后频率准确度优于2×10-11。  相似文献   

恒包络AltBOC信号调制方式分析     

雷志远  郭际  卢晓春 《时间频率学报》2013,36(1):44-53

为便于理解恒包络AltBOC(constant envelope alternate binary offset carrier)信号调制方式,结合直观的信号相位图,从最基本的BOC信号入手,引出AltBOC信号最简单的双通道形式,进而到四通道,最终导出恒包络AltBOC信号表达式,并给出主要的数字特征。  相似文献   

Distribution of PSF of The Near Earth Object Survey Telescope     

《Chinese Astronomy and Astrophysics》2013,37(1):97-106

The CCD field of view of the Near Earth Object Survey Telescope (NEOST) is 1.94°xl.94°. As a wide-field telescope, the focusing based on a single star will lead to an uneven distribution of PSF (Point Spread Function) on the CCD image due to the field curvature. The features of the PSF distribution on the CCD image are studied. By fitting the relation between the defocusing and the FWHM (Full Width at Half Maximum) of PSF, the curved focal surface is simulated and therefore the best imaging plane is determined. Hereby, a focusing method based on the optimum imaging plane determined by judging the histogram of FWHM is proposed.  相似文献   

Research on Multiband Observations of X-ray Millisecond Pulsar J0437-4715     

《Chinese Astronomy and Astrophysics》2013,37(2):195-211

A study on the two-band observations of the millisecond pulsar J0437- 4715 is carried out based on the radio data of the Parkes Observatory of Australia and the X-ray data obtained with the ASM (All Sky Monitor) in the RXTE (Rossi X-ray Timing Explorer). For the radio observations of J0437-4715 the software TEMPO2 is applied to the calibration of the timing data of different terminal systems, thereby improving the accuracy of the timing model. By taking advantage of the all-weather observations of the ASM in the RXTE, the study of the medium- and long-term light variations of the pulsar J0437-4715 at the X-ray wavelengths is carried out by means of structure function, and it is found that this pulsar has a 620 d light period in the X-ray waveband.  相似文献