一种高频雷达回波谱反演海浪的新算法     

常广弘  黎明  楚晓亮  纪永刚  于长军 《中国海洋大学学报(自然科学版)》2015,45(2):127-133

在高频地波雷达海浪谱反演问题中,广泛采用的Barrick后向散射公式属于第一类非线性Fredholm积分方程。此类积分方程的解在本质上是不适定的,加之高频雷达二阶回波信号信噪比较低,使得反演海浪谱存在解不稳定的问题。本文提出一种稳定且低复杂度的反演算法,此算法首先根据高频雷达一阶回波谱测量海浪方向,并将其引入积分方程求解过程,减少求解变量的个数,降低反演算法的复杂度。为解决反演结果不稳定的问题,使用Tikhonov正则化方法并利用广义交叉验证法(GCV)确定其正则化系数。通过在不同测试条件下对反演算法的仿真测试分析,表明此方法具有运算量小、稳定性好的特点。  相似文献   

3维场景植被冠层多波段模拟研究进展     

张阳  柳钦火  覃文汉  刘强  李静  杜永明  谢东辉  黄华国  杨乐  倪文俭 《遥感学报》2015,19(6):894-909

植被冠层辐射散射信号中蕴含了丰富的植被信息,通过构建植被冠层辐射散射模型,可以实现植被结构等生物物理参数的遥感定量反演。迄今为止,可见光/近红外、热红外、微波波段均已发展了大量的模型,这些模型在参数反演方面各具优势,但不同波段的模型又有其自身的局限性。跨波段的联合模拟可以实现模型间的优势互补,进而提高地表参数的反演精度,近年来已有学者专注于可见光/近红外与热红外模型,热红外与微波模型,主被动微波模型,以及可见光/近红外与微波模型的联合模拟和协同反演,但多是两两联合,且主要是基于经验模型或解析模型。基于3维场景的植被冠层辐射散射特性模拟模型可以细致刻画不同组分的结构和空间分布特征,对于由植被结构引起的多次散射和组分比例变化的考虑具有优势。本文主要介绍了3维模拟模型在可见光/近红外、热红外和微波波段,以及跨波段联合模拟方面的研究进展,从模型机理、场景统一、以及组分理化参数的统一的角度,探讨了构建多波段3维模拟系统的可行性,展望了多波段3维模拟模型的发展趋势。  相似文献   

人体乳腺癌矿化的同步辐射研究     

孟繁露  李源  李艳  王长秋  鲁安怀  梅放 《岩石矿物学杂志》2015,34(6):957-962

同步辐射具有常规光源不可比拟的优良性能,可用于微量生物矿化样品的物相、结构、形貌和成分研究。本文利用基于同步辐射光源的X射线粉末衍射(SR-XRD)、傅立叶变换红外光谱(SR-FTIR)、X射线荧光分析(SR-XRF)和X射线三维成像,对人体乳腺癌矿化进行了表征。研究表明,乳腺癌矿化的主要矿物物相为碳羟磷灰石,含有Sr、Zn等微量元素,其中砂粒体矿化具有独特的分层结构。研究结果为乳腺癌的病理研究和诊断提供了矿物学参考信息。  相似文献   

MIS 6期以来热带西太平洋降雨与ITCZ的关系     

张帅  李铁刚  常凤鸣  俞宙菲  王海霞 《第四纪研究》2015,35(2)

通过Ontong-Java海台KX97322-4孔沉积物中浮游有孔虫表层种Globigerinoides ruber的Mg/Ca海表温度(SST)并结合其δ18O得到过去约200ka B.P.以来当地水文(盐度和降雨)指标,结果表明从MIS 6期以来,热带太平洋暖池区温度变化存在明显的冰期-间冰期波动,降温幅度超过3℃.通过与赤道东太平洋对比表明热带太平洋在过去冰消期和冰期中的升温阶段呈现出类El Ni(n)o的状态,向两极输送水汽和热量.在冰消期,热带太平洋纬向温度梯度降低,全球升温,全球冰量下降.在冰期中升温阶段(MIS 6)热带太平洋纬向温度梯度降低时全球冰量却持续增加,可能此时输送热量不足以使两极冰川融化,带来的水汽又促进了两极冰川的形成.通过与中国石笋记录和热带降雨记录对比,表明热带太平洋纬向温度梯度的变化与热带辐合带(ITCZ)的移动密切相关,并且影响到东亚夏季风的降雨状况,热带太平洋类ENSO过程可能对ITCZ的变化存在内部系统调谐的作用.  相似文献   

核幔耦合对地球自由核章动的激发影响   总被引：1，自引：0，他引：1       下载免费PDF全文

崔小明  孙和平  徐建桥  周江存  陈晓东 《地球物理学报》2018,61(9):3584-3591

地球自由核章动（FCN）是地幔与液核相互作用的重要动力学现象，其激发机制涉及地表流体层、地幔和地核等圈层之间的耦合，此前研究多利用地表流体层角动量数据单独研究其对FCN的激发，对核幔耦合的影响考虑不足.本文基于角动量守恒理论分析了核幔耦合对FCN周期及振幅的影响，并结合多个大气及海洋角动量函数时间序列首次估算了核幔耦合在FCN激发过程中的贡献.结果表明核幔耦合对FCN周期产生的固定和时变影响对FCN激发的作用均不可忽视，尤其时变影响可达几十个微角秒，对于进一步解释FCN时变特征非常重要；核幔耦合对FCN振幅的直接影响是地表流体层的激发与实测FCN不相符的主要原因，黏滞、电磁和地形等耗散耦合的存在对地表流体的激发振幅有67%左右的减弱效果.  相似文献   

Optimum size and density of surface grid arrays for retrieving accurate shear-tensile fracturing of microearthquakes     

Yi Ren  Yongtao Gao  Shunchuan Wu  Václav Vavryčuk 《Geophysical Prospecting》2020,68(8):2347-2360

Surface arrays became an important tool for monitoring the induced seismicity in hydraulic fracturing experiments and for assessing the impact of fluid injection on the fracturing process of microearthquakes. The layout of sensors plays a key role in this task because it controls the accuracy of event locations and retrieved seismic moment tensors. We simulate various configurations of grid sensor arrays characterized by a different number of sensors, array span, sensor spacing, depth of sources and various shear/tensile source mechanisms of events. The moment tensor inversion is carried out using synthetically calculated P-wave amplitudes with added random noise. A bias in the solutions is evaluated by errors in the double-couple percentage of inverted moment tensors because the double-couple errors inform us about the sensitivity of the network to detect the shear/tensile fracturing mode of induced microearthquakes. The results show that the accuracy of the double-couple percentage is mostly controlled by the offset-to-depth ratio R defined as the ratio of half of the network size to the event depth. The optimum value of R is in the range of 0.75–1.5 irrespective of the type of the focal mechanism. If 121 (11 × 11) sensors are distributed in a regular grid and recorded data are characterized by a 10% random noise, the double-couple error is less than 6%. This error increases, if R is not optimum or if the number of sensors is reduced. However, even sparse arrays with 49 (7 × 7) or 16 (4 × 4) sensors can yield a reasonable accuracy, provided the surface grid arrays are designed to have an optimum size.  相似文献   

Application of surface-wave tomography to mineral exploration: a case study from Siilinjärvi,Finland     

Federico Da Col  Myrto Papadopoulou  Emilia Koivisto  Łukasz Sito  Mikko Savolainen  Laura Valentina Socco 《Geophysical Prospecting》2020,68(1):254-269

In order to assess the feasibility and validity of surface-wave tomography as a tool for mineral exploration, we present an active seismic three-dimensional case study from the Siilinjärvi mine in Eastern Finland. The aim of the survey is to identify the formation carrying the mineralization in an area south of the main pit, which will be mined in the future. Before acquiring the data, we performed an accurate survey design to maximize data coverage and minimize the time for deployment and recollection of the equipment. We extract path-averaged Rayleigh-wave phase-velocity dispersion curves by means of a two-station method. We invert them using a computationally efficient tomographic code which does not require the computation of phase-velocity maps and inverts directly for one-dimensional S-wave velocity models. The retrieved velocities are in good agreement with the data from a borehole in the vicinity, and the pseudo three–dimensional S-wave velocity volume allows us to identify the geological contact between the formation hosting most of the mineralization and the surrounding rock. We conclude that the proposed method is a valid tool, given the small amount of equipment used and the acceptable amount of time required to process the data.  相似文献   

地表数据驱动的与层相关的层间多次波消除方法及应用          下载免费PDF全文

刘战  刘洪  孙军  邓世广  冯海新 《地球物理学报》2019,62(6):2227-2236

基于反馈模型的地表相关多次波消除方法SRME(Surface-Related Multiple Elimination)近年来已得到了广泛的应用.利用共聚焦点CFP(Common Focus Point)道集代替炮集,可以将该方法扩展至层间多次波的消除.地表数据驱动的层间多次波消除方法直接利用地表观测数据进行层间多次波预测,避免了构建CFP道集所需的聚焦运算,特别是与层相关的层间多次波消除方法有效提高了多次波预测的计算效率.但地表数据驱动的与层相关的层间多次波消除方法并没有从理论上被严格地推导证明,其与CFP方法之间的关系亦未被讨论.本文在CFP方法的理论基础上推导了地表数据驱动的与层相关的层间多次波消除方法,阐明了CFP方法与地表数据驱动方法之间的内在联系.并将该方法应用于模型数据和野外实际数据,应用实例表明了所提方法的有效性.  相似文献   

隐伏正断层错动致地表破裂变形特征的研究     

齐剑峰  郝文拯  王晓明  张江伟 《震灾防御技术》2019,14(3):628-639

通过建立三维计算模型，对隐伏正断层在均匀错动、倾斜错动和翘倾错动方式下地表土体的应力路径、破裂和变形特征进行了研究。根据地表破裂临界值，分析了工程建设“避让带”的宽度和起始位置的变化特征。根据行业规范，提出工程建设“关注带”的确定方法，分析了“关注带”的宽度和起始位置的变化特征，得到以下主要结论:①在断层错动过程中，位于两侧的地表土体应力路径变化明显不同，下盘一侧和上盘一侧分别以三轴拉伸和三轴压缩为主；②地表强变形带与地表破裂带的分布并不一致，需要综合考虑等效塑性应变和总位移比2个指标来评价同震地表错动对建筑物的影响；③当隐伏断层错动的垂直位移达到3m时，工程建设“避让带”的宽度在10—90m范围内变化，受上覆土体厚度和断层倾角的影响最大，而工程建设“关注带”的宽度在150—400m范围内变化，受上覆土体的性质影响最大。  相似文献   

Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo     

Tan Bao-lin  Cheng Jun  Tan Cheng-ming  Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.  相似文献