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1.
AST3-2 (the second Antarctic Survey Telescope) is located in Antarctic Dome A, the loftiest ice dome on the Antarctic Plateau. It produces a huge amount of observational data which require a more efficient data reduction program to be developed. Also the data transmission in Antarctica is much difficult, thus it is necessary to perform data reduction and detect variable and transient sources remotely and automatically in Antarctica, but this attempt is restricted by the unsatisfactory performance of the low power consumption computer in Antarctica. For realizing this purpose, to develop a new method based on the existing image subtraction method and random forest algorithm, taking the AST3-2 2016 dataset as the test sample, becomes an alternative choice. This method performs image subtraction on the dataset, then applies the principle component analysis to extract the features of residual images. Random forest is used as a machine learning classifier, and in the test a recall rate of 97% is resulted for the positive sample. Our work has verified the feasibility and accuracy of this method, and finally found out a batch of candidates for variable stars in the AST3-2 2016 dataset.  相似文献   
2.
The uv-faceting imaging is one of the widely used large field of view imaging technologies, and will be adopted for the data processing of the low-frequency array in the first stage of the Square Kilometre Array (SKA1). Due to the scale of the raw data of SKA1 is unprecedentedly large, the efficiency of data processing directly using the original uv-faceting imaging will be very low. Therefore, a uv-faceting imaging algorithm based on the MPI (Message Passing Interface)+OpenMP (Open Multi-Processing) and a uv-faceting imaging algorithm based on the MPI+CUDA (Compute Unified Device Architecture) are proposed. The most time-consuming data reading and gridding in the algorithm are optimized in parallel. The verification results show that the results of the proposed two algorithms are basically consistent with that obtained by the current mainstream data processing software CASA (Common Astronomy Software Applications), which indicates that the proposed two algorithms are basically correct. Further analysis of the accuracy and total running time shows that the MPI+CUDA method is better than the MPI+OpenMP method in both the correctness rate and running speed. The performance test results show that the proposed algorithms are effective and have certain extensibility.  相似文献   
3.
Machine learning has achieved great success in many areas today. The lifting algorithm has a strong ability to adapt to various scenarios with a high accuracy, and has played a great role in many fields. But in astronomy, the application of lifting algorithms is still rare. In response to the low classification accuracy of the dark star/galaxy source set in the Sloan Digital Sky Survey (SDSS), a new research result of machine learning, eXtreme Gradient Boosting (XGBoost), has been introduced. The complete photometric data set is obtained from the SDSS-DR7, and divided into a bright source set and a dark source set according to the star magnitude. Firstly, the ten-fold cross-validation method is used for the bright source set and the dark source set respectively, and the XGBoost algorithm is used to establish the star/galaxy classification model. Then, the grid search and other methods are used to adjust the XGBoost parameters. Finally, based on the galaxy classification accuracy and other indicators, the classification results are analyzed, by comparing with the models of function tree (FT), Adaptive boosting (Adaboost), Random Forest (RF), Gradient Boosting Decision Tree (GBDT), Stacked Denoising AutoEncoders (SDAE), and Deep Belief Nets (DBN). The experimental results show that, the XGBoost improves the classification accuracy of galaxies in the dark source classification by nearly 10% as compared to the function tree algorithm, and improves the classification accuracy of sources with the darkest magnitudes in the dark source set by nearly 5% as compared to the function tree algorithm. Compared with other traditional machine learning algorithms and deep neural networks, the XGBoost also has different degrees of improvement.  相似文献   
4.
Two photometric follow-up transit (primary eclipse) observations on WASP-43 b and four observations on TrES-3 b are performed using the Xuyi Near-Earth Object Survey Telescope. After differential photometry and light curve analysis, the physical parameters of the two systems are obtained and are in good match with the literature. Combining with transit data from a lot of literature, the residuals (O ? C) of transit observations of both systems are fitted with the linear and quadratic functions. With the linear fitting, the periods and transit timing variations (TTVs) of the planets are obtained, and no obvious periodic TTV signal is found in both systems after an analysis. The maximum mass of a perturbing planet located at the 1:2 mean motion resonance (MMR) for WASP-43 b and TrES-3 b is estimated to be 1.826 and 1.504 Earth mass, respectively. By quadratic fitting, it is confirmed that WASP-43 b may have a long-term TTV which means an orbital decay. The decay rate is shown to be P? = (?0.005248 ± 0.001714) s·yr?1, and compared with the previous results. Based on this, the lower limit of the stellar tidal quality parameter of WASP-43 is calculated to be Q*1.5×105, and the remaining lifetimes of the planets are presented for the different Q* values of the two systems, correspondingly.  相似文献   
5.
戴勇  高立新  姚丽  朱培育  格根  王磊 《地震》2019,39(3):106-114
2013年6月16日, 中国大陆西部出现地磁低点位移。 异常出现后一个月内, 位于低点位移分界线附近发生7月22日岷县、 漳县交界6.6级地震。 本文通过采用实测低点时间减去理论低点时间的方法剔除低点时间经度效应, 并以剔除经度效应后低点时间为0 h的等值线作为低点位移分界线, 2013年岷县—漳县6.6级地震震中处于6月16日地磁低点位移分界线上。 对异常期间的中国大陆地区地磁垂直分量日变形态进行统计, 发现其存在显著的分区特征, 低点时间为正的区域内日变化形态基本呈现W型, 低点时间为负的区域内日变化形态主要呈现V字型特征。 低点位移异常日期间, 中国大陆存在显著的高梯度带, 本文采用梯度值定量描述低点时间空间变化程度。 在6月13日正常日期间, 中国大陆地区未出现梯度值大于1.5 h/(°)的区域, 在6月16日异常日期间, 出现梯度值大于1.5 h/(°)的区域, 2013年岷县—漳县6.6级地震位于高梯度区边缘。  相似文献   
6.
倪红玉  刘泽民  洪德全  赵朋  汪小厉 《地震》2019,39(3):138-148
本文首先通过Snoke发展的利用P波、 SV波和SH波的初动和振幅比方法计算秦岭—大别东段2008年以来83次ML≥2.5地震的震源机制解, 然后通过FMSI方法反演得到平均应力场的方向特征: 近东西向的水平挤压和近南北向的水平拉张作用, 与参数统计结果一致; 进而通过震源机制的一致性参数分析应力场方向的变化信息。 分析表明震源机制解呈现了由变化紊乱、 偏离平均应力场到变化一致、 趋于平均应力场再到变化紊乱、 偏离平均应力场的变化过程, 在显著地震前, 研究区整体的震源机制一致性参数处于持续低值状态; 计算了2008年以来93次ML≥2.5地震的视应力, 拟合视应力与震级的关系, 分析扣除震级影响的差视应力随时间变化特征, 近似反映研究区应力大小的变化。 分析表明显著地震前研究区的差视应力值呈现出明显的先上升后下降的变化过程, 在下降过程中发生地震; 最后利用震源机制一致性参数和差视应力综合分析研究区的应力状态, 均表明显著地震前震源区的构造应力场增强。 目前研究区的震源机制一致性参数较高、 差视应力较低, 研究区的应力水平较低。  相似文献   
7.
河南新郑—太康断裂东段土壤气体地球化学特征   总被引:2,自引:0,他引:2  
土壤气浓度测量能够揭示断裂位置和活动特征。 由于河南新郑—太康断裂北西向隐伏断裂带空间定位精度有待提高, 以及2016年5月该区出现地下逸出气异常的宏观现象, 在太康县西近垂直于断裂走向布设了一条长约13 km的NE—NNE走向的地球化学观测剖面, 用于分析隐伏断层浅层位置及其与地下逸出气宏观异常的关系。 观测结果表明: 该剖面的异常段与该区浅层地震勘探显示的断裂带地表出露位置相吻合, 其中Rn体积活度和H2、 CO2浓度异常揭示出南段有4条断层, 北段有2条断层, 且均具有高角度特征, 南段的CO2浓度异常区与地下逸出气宏观异常位置相符, 但代表构造特征的Rn体积活度和H2浓度没有出现异常, 认为与构造关系不密切。  相似文献   
8.
利用Snoke方法求解和收集得到的77次中小地震的震源机制解资料,采用Gephart应力张量反演方法,获得了郯庐断裂带鲁苏皖段构造应力场,最大主压应力方位角为80°,最小主压应力方位角为172°,最大、中等和最小主压应力倾角分别为15°、65°和19°,反映了研究区处于近EW向水平作用和近NS向的水平拉张作用环境下。根据地震活动、地质构造及震源机制解差异,我们将郯庐断裂带鲁苏皖段分5个区段开展研究,结果显示:5个分区应力场存在局部差异,最大主压应力方位角处于63°~88°之间,从北往南总体方向成顺时针偏转的趋势。跨郯庐断裂带两侧的应力场研究结果显示,从西到东最大主压应力方向有一个逆时针偏转的趋势,西侧最大主压应力方向更接近EW向,东侧更接近NE向,郯庐断裂带内处于两侧的过渡地段。  相似文献   
9.
黑龙江省多宝山—大新屯地区,铜矿以中—晚加里东期多宝山式斑岩型、燕山早期三矿沟式矽卡岩型为主,晚古生界海底火山岩有关喷发—沉积型铜锌矿床,具优越的成矿潜力,不同时期、类型铜矿床在空间分布上明显受古生代海相火山岩—碳酸盐岩建造控制,并具有"上金下铜"的斑岩—热液型铜金矿成矿系统的特征。金矿以燕山晚期三道湾子式浅成低温热液型金成矿作用强烈为特点;持续时间由早石炭世—早—中侏罗世的韧性剪切—走滑作用、中侏罗世为主要伸展期的变质核杂岩有关的金成矿作用,以及奥陶纪浊积岩(卡林型)有关金成矿作用,以中—小规模金矿床(点)为主;金矿受北西向、北东向的火山构造、变质核杂岩构造和韧性剪切—走滑作用控制,显示出良好的金找矿前景;结合近期的铜金矿重大勘查进展和成果,总结成矿规律,梳理了制约着铜金多金属矿找矿突破的关键地质问题,提出找矿方向和今后勘查工作部署建议。  相似文献   
10.
陈虹  田蜜  武国利  胡健民 《地质论评》2014,60(6):1437-1452
位于南秦岭构造带南缘的勉略(勉县—略阳)洋是东古特提斯洋的北侧分支洋盆,在勉县—略阳地区发育有典型的蛇绿岩组合。然而,由于中三叠世晚期开始的碰撞造山作用以及之后陆内变形作用的改造,对于勉略洋盆在构造带东段的裂解和演化过程并不清晰。本文对发育于东南秦岭构造带内的基性岩墙群进行了岩石学、岩石地球化学、同位素年代学等方面的研究。结果表明,基性岩脉以辉长岩、辉绿岩等基性岩为主,其SiO 2含量为41.89%~49.75%,属基性—超基性岩类,并具有富钠、高钛的碱性岩特征。岩石的稀土、微量元素和Sr—Nd同位素特征与板内洋岛玄武岩(OIB)特征一致,岩浆源于具有地壳混染的板内洋岛玄武岩型地幔源区。该类基性岩脉顺层侵入到早古生代早期地层中,通过基性岩脉中的锆石SHRIMP测年获得岩脉顺层侵位的时代为晚志留世早期(约422 Ma)。这种岩浆作用很可能与古特提斯洋初始裂解有关,并导致南秦岭构造带内地壳伸展、基性岩浆侵位,该过程与南秦岭构造带北缘的商丹(商南—丹凤)原特提斯洋的消减和陆内俯冲可能相关。  相似文献   
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