Seismic data reconstruction based on iterative linear expansion of thresholds

Based on the compressive sensing,a novel algorithm is proposed to solve reconstruction problem under sparsity assumptions.Instead of estimating the reconstructed data through minimizing the objective function,the authors parameterize the problem as a linear combination of few elementary thresholding functions,which can be solved by calculating the linear weighting coefficients.It is to update the thresholding functions during the process of iteration.The advantage of this method is that the optimization problem only needs to be solved by calculating linear coefficients for each time.With the elementary thresholding functions satisfying certain constraints,a global convergence of the iterative algorithm is guaranteed.The synthetic and the field data results prove the effectiveness of the proposed algorithm.     

大棚蔬菜最低气温预报及冻害防御技术

在大棚蔬菜低温冻害防御中,通过搭建拱棚加盖不同层塑料内膜的大棚温度调控模式应用广泛。通过对不同层塑料内膜覆盖的大棚小气候环境温度观测,分析了棚内外日最低气温的相关关系,建立了棚内小气候环境日最低气温的一元线性回归预测模型,应用气象台天气预报中的日最低气温预报开展了大棚小气候环境的日最低气温预报,根据预报结果和蔬菜冻害指标,确定大棚增温防冻需要加盖塑料内膜的层数,提出大棚蔬菜内膜覆盖方式的冻害防御对策,为设施农业提供安全生产保障依据。     

The evolution of the z distribution of normal neutron stars in the Galaxy

Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Secular period decreasing of detached chromospherically active binaries

The long-term orbital period changes of a large sample of detached chromospherically active binaries (CABs) were studied. Eleven such systems were found to be undergoing secular period decreases with the rates of ?6.3×10^?9 to ?1.1×10^?6 days per year. The period decreasing rates are found to vary depending on the orbital period. The longer the orbital period is, the more rapidly the period decreases. Following Stepien (Mon. Not. R. Astron. Soc. 274:1019, 1995), the period decreasing rate predicted by angular momentum loss (AML) caused by magnetic wind is computed for each system. A comparison between the observed and calculated period decreasing rates shows that the former values are obviously larger than the latter by 1–3 orders of magnitude. It suggests that the magnetic wind is not likely the determinant mechanism driving the AML in these systems. Finally, the orbital angular momentum (AM) and the rate of AML, $\dot{J}$ , are computed for each system. It shows that the AM have a similar change with the orbital period like dP/dt does, but $\log\dot{J}/J$ presents no strict changing with the kinematical ages.     

鲁豫交界地区尾波Q_c值分析研究

该文对濮阳台记录的21次地震进行了地震波衰减研究,讨论了地球介质品质因子随频率变化的关系;利用不同地震采用不同流逝时间的尾波品质因子测定方法,有效去除了由于不同地震或同一地震的地震散射波在纵向介质中穿透深度的不同而导致对品质因子测量结果的影响,从而有利于扑捉到品质因子的异常变化特征与地震孕育过程的关系。利用改进后的模型,对鲁豫交界地区尾波值进行了计算,得到了该地区品质因子随频率的变化关系和区域介质衰减的时间变化特征。     

藏南亚东地区片麻状黑云花岗闪长岩LA-ICP-MS锆石U-Pb测年青藏高原羌塘南部晚古生代地幔柱?——来自基性—超基性岩的地球化学证据

羌塘南部地区大面积出露基性—超基性火成岩。基性岩墙和玄武岩沿龙木错-双湖板块缝合带的南侧呈近东西向分布,大地构造位置位于冈瓦纳大陆北缘,分布范围西起国境线,东到双湖地区,总长约800km,形成时代集中在晚石炭世—早二叠世(284~318Ma),反映出岩浆的快速侵位-喷溢的过程。基性岩墙和玄武岩主要为碱性系列岩石,少数为亚碱性系列,Ti和Fe的含量均比较高,Mg#比较低,表明它们都是原始岩浆经不同程度分异结晶后的残余熔体。基性岩墙和玄武岩的稀土元素、微量元素、形成环境等均与板内玄武岩或典型的地幔柱成因玄武岩具有相似的特点。另外,苦橄质岩石多与基性岩墙和玄武岩一起产出,主要为单斜辉石橄榄岩和二辉橄榄岩,矿物成分贫挥发性组分,主量、稀土和微量元素的特点反映出其很可能代表了地幔柱原始岩浆结晶的产物而非岩浆捕获体,而且其源区很可能为石榴子石二辉橄榄岩。由此,初步认为羌塘南部基性岩墙和玄武岩为地幔柱的头部减压熔融的产物,而苦橄质岩石为地幔柱尾柱通道熔融的产物。     

青藏高原羌塘南部晚古生代地幔柱?——来自基性-超基性岩的地球化学证据

羌螗南部地区大面积出露基性一超基性火成岩.基性岩墙和玄武岩沿龙木错-双湖板块缝合带的南侧呈近东西向分布,大地构造位置位于冈瓦纳大陆北缘,分布范围西起国境线,东到双湖地区,总长约800km,形成时代集中在晚石炭世-早二叠世(284～318Ma),反映出岩浆的快速侵位-喷溢的过程.基性岩墙和玄武岩主要为碱性系列岩石,少数为亚碱性系列,Ti和Fe的含量均比较高,Mg#比较低,表明它们都是原始岩浆经不同程度分异结晶后的残余熔体.基性岩墙和玄武岩的稀土元素、微量元素、形成环境等均与板内玄武岩或典型的地幔柱成因玄武岩具有相似的特点.另外,苦橄质岩石多与基性岩墙和玄武岩一起产出.主要为单斜辉石橄税岩和二辉橄榄岩,矿物成分贫挥发性组分,主量、稀土和微量元素的特点反映出其很可能代表了地幔柱原始岩浆结晶的产物而非岩浆捕获体,而且其源区很可能为石榴子石二辉橄榄岩.由此,初步认为羌塘南部基性岩墙和玄武岩为地幔柱的头部减压熔融的产物,而苦橄质岩石为地幔柱尾柱通道熔融的产物.     

藏北羌塘自然保护区生态-特种旅游开发的SWOT分析

用SWOT分析模式对藏北羌塘自然保护区发展生态旅游的可行性和潜力进行了客观分析,羌塘自然保护区发展生态旅游业的优势有：高原原始自然景观独特,自然资源丰富,具有独一无二的可研究性,具有原生态的藏传文化。劣势有：可进入性差,资源开发程度低,旅游配套设施不完善,自然和文化生态环境脆弱。机遇有西藏旅游市场的开放,西部大开发和国家政策的支持,国内外旅游需求的持续增长,交通条件改善。挑战有生态旅游与生态保护的矛盾,区内旅游分割竞争格局,国内市场竞争日益激烈。认为在羌塘自然保护区发展生态旅游,优势与劣势同样显著,机遇和挑战并存,并据此提出在生态保护的基础上适度开发高端特种旅游产品,打造特种旅游品牌,构架保护区生态旅游“点-轴”系统开发模式,整合资源,走联合发展的道路,从而保障羌塘地区的持续有效发展。