Logs and Snags in a Shola Forest of Kerala, India     

U.M. Chandrashekara  V. Sibichan 《山地科学学报》2006,3(2):131-138

Introduction Dead wood is an important structural and functional component of a forest ecosystem(Fridman and Welheim 2000). Recent studies also indicate that dead wood is important for maintaining both plant and animal diversity in different forest ecosystems (Grove 2001) as it serve as an energy source (Bray and Gorham 1964) and habitat for an array of organisms. Dead wood can also help reduce erosion, increase soil organic matters (McFee and Stone 1966), and suitable conditions for seedli…  相似文献   

南海区多鱼种声学评估工作程序   总被引：3，自引：0，他引：3  

李永振  陈国宝  孙典荣  张旭丰 《广东海洋大学学报》2003,23(1):35-40

总结了利用SimradEK50 0声学系统进行了南海区多鱼种资源评估经验 ,介绍了多鱼种声学评估的工作流程 ,包括调查方案制定、声学数据采集、映像分析、积分值分配、资源量的计算方法等关键过程 ,同时及在工作中应该注意的细节。  相似文献   

The DynaMICCS perspective     

S. Turck-Chièze  P. Lamy  C. Carr  P. H. Carton  A. Chevalier  I. Dandouras  J. M. Defise  S. Dewitte  T. Dudok de Wit  J. P. Halain  S. Hasan  J. F. Hochedez  T. Horbury  P. Levacher  M. Meissonier  N. Murphy  P. Rochus  A. Ruzmaikin  W. Schmutz  G. Thuillier  S. Vivès 《Experimental Astronomy》2009,23(3):1017-1055

The DynaMICCS mission is designed to probe and understand the dynamics of crucial regions of the Sun that determine solar variability, including the previously unexplored inner core, the radiative/convective zone interface layers, the photosphere/chromosphere layers and the low corona. The mission delivers data and knowledge that no other known mission provides for understanding space weather and space climate and for advancing stellar physics (internal dynamics) and fundamental physics (neutrino properties, atomic physics, gravitational moments...). The science objectives are achieved using Doppler and magnetic measurements of the solar surface, helioseismic and coronographic measurements, solar irradiance at different wavelengths and in-situ measurements of plasma/energetic particles/magnetic fields. The DynaMICCS payload uses an original concept studied by Thalès Alenia Space in the framework of the CNES call for formation flying missions: an external occultation of the solar light is obtained by putting an occulter spacecraft 150 m (or more) in front of a second spacecraft. The occulter spacecraft, a LEO platform of the mini sat class, e.g. PROTEUS, type carries the helioseismic and irradiance instruments and the formation flying technologies. The latter spacecraft of the same type carries a visible and infrared coronagraph for a unique observation of the solar corona and instrumentation for the study of the solar wind and imagers. This mission must guarantee long (one 11-year solar cycle) and continuous observations (duty cycle > 94%) of signals that can be very weak (the gravity mode detection supposes the measurement of velocity smaller than 1 mm/s). This assumes no interruption in observation and very stable thermal conditions. The preferred orbit therefore is the L1 orbit, which fits these requirements very well and is also an attractive environment for the spacecraft due to its low radiation and low perturbation (solar pressure) environment. This mission is secured by instrumental R and D activities during the present and coming years. Some prototypes of different instruments are already built (GOLFNG, SDM) and the performances will be checked before launch on the ground or in space through planned missions of CNES and PROBA ESA missions (PICARD, LYRA, maybe ASPIICS).  相似文献   

Background studies for acoustic neutrino detection at the South Pole     

《Astroparticle Physics》2012,35(6):312-324

The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method to measure the flux of cosmogenic neutrinos expected on Earth. The energy threshold for this process depends strongly on the absolute noise level in the target material. The South Pole Acoustic Test Setup (SPATS), deployed in the upper part of four boreholes of the IceCube Neutrino Observatory, has monitored the noise in Antarctic ice at the geographic South Pole for more than two years down to 500 m depth. The noise is very stable and Gaussian distributed. Lacking an in situ calibration up to now, laboratory measurements have been used to estimate the absolute noise level in the 10-50 kHz frequency range to be smaller than 20 mPa. Using a threshold trigger, sensors of the South Pole Acoustic Test Setup registered acoustic events in the IceCube detector volume and its vicinity. Acoustic signals from refreezing IceCube holes and from anthropogenic sources have been used to test the localization of acoustic events. An upper limit on the neutrino flux at energies E_ν > 10¹¹ GeV is derived from acoustic data taken over eight months.  相似文献   

固定铝log(Q/K)图解在温泉中的应用     

张展适  孙占学  李满根  王素娟 《地球科学》2004,29(3):352-356

为探讨常规和固定铝log(Q/K)图解法对温泉系统是否有效 ,采用WATCH程序 ,对江西 3个温度较高的温泉 ,即庐山温泉、汤湖温泉和横泾温泉 ,进行了探测性的研究 .采用常规log(Q/K)图解法计算时 ,由于参加计算的 4个水样的铝含量均未检出 ,计算结果显示只有不含铝的矿物玉髓和方解石相交于温度 1 0 0℃附近 ,热储总体上没有达到平衡 .在采用了固定铝log(Q/K)图解法并同时考虑冷水的稀释作用计算后 ,中低温地热系统中常见的蚀变矿物如浊沸石、纤蛇纹石、萤石和玉髓均显示了较好的收敛性 ,收敛的温度大致在 1 0 0～ 1 4 0℃ .并且上述矿物组合可见于某些温泉的深部钻孔中 ,计算结果与实际地质情况相吻合 .结果表明固定铝log(Q/K)图解法可以恢复温泉系统的热平衡状态  相似文献   

基于浏览行为的网络地图用户兴趣模型研究     

王成舜  郑束蕾 《测绘与空间地理信息》2017,(3)

为准确表达用户兴趣,提升网络地图个性化服务效率,本文结合用户的操作行为与视觉行为,探讨了用户兴趣获取的原理与方法。结合Web日志与眼动数据的特点,提取网络地图的用户兴趣特征项,并利用熵权法对用户兴趣度进行估计。通过向量空间模型,构建网络地图用户兴趣模型,并开展验证实验对用户兴趣建模方法进行验证。  相似文献   

煤层含气量测井解释方法探讨   总被引：6，自引：1，他引：5  

潘和平  黄智辉 《煤田地质与勘探》1998,26(2):58-60

用多元线性回归建立煤层气含量与煤质参数、测井曲线值之间的回归方程,经F检验回归方程有效,但回归方程估算的煤层含气量与煤样解吸测定的含气量之间仍然存在较大的误差,为此利用BP神经网络进一步探讨它们之间的关系,实例表明预测精度较高。   相似文献   

小波变换多尺度地震波形反演   总被引：29，自引：5，他引：24       下载免费PDF全文

孟鸿鹰  刘贵忠 《地球物理学报》1999,42(2):241-248

完全非线性地震波形反演问题是石油地球物理勘探领域中一个非常重要而又难度很大的问题。本文提出了多尺度地震波形反演的小波变换方法,对于一维非线性地震波形反演问题,将该方法和已有的简单迭代法及多重网格法作了比较,数值实验结果表明,本方法效果较好。  相似文献   

实验室声发射三维定位及标本波速场各向异性研究   总被引：1，自引：0，他引：1  

蒋海昆  张流  王琦 《地震》1999,19(3):245-252

根据慢度离差法的基本原理,给出由遗传算法确定AE空间位置、发生时刻及慢度离差5个参量的具体方法。结合实验条件,通过数值试验对定位误差等问题进行探讨,并对真实AE定位的误差分布给出统计上的圈定。数值试验结果表明,算法具有较高的精度和较好的收敛性及稳健性;探头数量及布设方式对定位结果的优劣有影响, 4个以上探头有记录时,即可得到理想的结果;大的定位误差主要来源于台阵外部少数“ AE”的结果。到时测量的随机误差小于最小测量时间单位的50%时,平均有97%的“AE”定位误差分布在3 mm 范围内,小于物理不可分辨精度(探头直径)。  相似文献   

含偏心点声源的随钻测井声场模拟和地层各向异性反演研究   总被引：2，自引：0，他引：2       下载免费PDF全文

卫建清  何晓  李希强  陈浩  王秀明 《地球物理学报》2019,62(4):1554-1564

地层横波波速测量以及各向异性评价是目前随钻声波测井应用及方法研究的难题之一.针对这些问题,本文试图从钻铤上的偏心点声源在各向异性地层中的响应出发,寻求和探讨解决方案.我们基于三维有限差分模拟的随钻测井信号,研究了偏心点声源在水平横向各向同性(HTI)慢速地层井孔中激发声波传播规律,研究结果表明:在HTI地层中偏心点声源能够同时激发出快、慢两种波形,并且此两种波形中主要分别包含快、慢弯曲波,由于与钻铤波的耦合作用,其速度总是分别小于地层快、慢横波波速,所以无法直接用于地层横波波速的测量.但根据进一步的灵敏度分析可知当在3kHz以上时,它们的相速度分别对地层参数水平和垂直剪切模量(c66和c44)最为敏感.基于此特性,本文提出一种基于解析近似解的最小二乘拟合法,能够通过快、慢波频散曲线反演地层横波波速,所测值误差小于3%,并且具有很好的容错率和稳定性;进而由横波速度反演值评价地层各向异性大小.最后,地层快横波偏振方位可以利用垂直于偏心声源方向的偶极采集的信号能量变化曲线来获取.  相似文献