声速剖面EOF重构的实测数据采样深度研究

经验正交函数（experiential orthogonal functions,EOF）是重构声速剖面（sound speed profile,SSP）的一种有效方法,利用部分实测数据结合历史剖面资料可以重构当前位置的声速剖面。针对实测数据的采样深度难以确定这一问题,本文介绍了一种基于历史声速剖面资料的实测数据采样深度选取方法,根据EOF空间函数的方差贡献率确定数据量,进而采用EOF算法重构全海深声速剖面。实验结果表明：采用该方法得到的数据重构的声速剖面与实测声速剖面具有较好的一致性,基于常梯度声线跟踪法得到的水深数据能够满足0.25%倍水深限差,有效波束比达到了100%,为实际测量作业中声剖数据的采样深度提供了参考。     

POISSON'S RATIO VARIATIONS OF CRUSTAL MEDIA BEFORE AND AFTER XINYUAN-HEJING MS6.6 EARTHQUAKE IN 2012

We analyzed the variation characteristics of Poisson's ratio in crustal media from January 2009 to December 2012 at 11 fixed seismic stations(for station SCH, it is from January 2006 to December 2012)within an epicenter distance of 200km of the Xinyuan-Hejing M_S6.6 earthquake in Xinjiang on June 30, 2012 using the methods of P wave receiver functions, H-κ stacking of receiver functions, and time sliding window, and obtained the following conclusions: (1)The crustal media's Poisson ratio of five stations in an epicenter distance less than 130km showed a significant and long-lasting decline about 2~3 years before Xinyuan-Hejing M_S6.6 earthquake. Taking the crustal Poisson ratio mean value as reference, the decrease ranges between 0.003 and 0.014, the decrease in 4 stations are more than twice the mean error. The variations of the Poisson's ratio in crust are characterized by "V" shape or "double V" shape. Earthquakes occur at the end of the formation of "V" shape. After the occurrence of earthquakes, the Poisson's ratio continues to rise. The earliest initial fall appeared in July 2009 at WUS station which has the minimum epicentral distance(77km). The Poisson ratio of the crustal media of 6 stations with epicentral distance more than 150km fluctuated up and down around the mean value, and there is no significant decline or persistent low value. (2)We analyzed the arrival-time variations of the quasi-repetitive receiver functions Ps converted wave(t_Ps)of the 3 stations WUS, SCH and XNY and found that the travel times of Ps converted waves became smaller in the crust before the earthquake and increased after the earthquake. (3)Through the comprehensive analysis on the descending process, decline ranges, variations process, duration of Poisson' ratio, the Ps converted waves arrival time variations, the original time of earthquake, and the number of stations, it is inferred that the cause for Poisson's ratio anomalous variations is the change of physical properties of crustal media in the process of earthquake preparation and occurrence. Since the variation characteristics of crustal media may be related to the earthquake magnitude, the size of seismogenic area, the medium properties under stations, and the focal distance, whether the medium variation characteristics exist before and after Xinyuan-Hejing M_S6.6 earthquake will need more earthquake cases analyses. (4)The H-κ stacking of receiver functions is used to calculate the velocity ratio. Because P-wave velocity is given, this method can only be applied when the Ps converted wave velocity of Moho surface of receiver functions changes before an earthquake. With the application of receiver functions to the analysis of more earthquake cases, we can gain more insights into the variation of crustal medium parameters during the seismogenic process. This observation indicates that the receiver function method may become a new approach to detect the Poisson's ratio change of the crustal media before strong earthquake under the condition of high seismic network density.     

多波束测深波束脚印位置归算模型研究

推导了多波束测深脚印位置归算模型,通过与CARIS软件进行实例比对,验证了该模型的有效性。在数据处理过程中,采用时标序列检索的方式处理导航时间延迟,取得了良好的效果;采用条带姿态进行姿态改正避免了"杠杆"旋转对边缘波束深度的影响。实例比对表明,该模型结果与CARIS软件输出结果一致。     

一种改善GPS接收机载波相位连续性的相位预测方法

针对GPS信号受短时遮挡等影响导致载波相位不连续问题,提出一种基于载波开环跟踪的相位预测方法。通过对失锁通道的多普勒进行精确预测实现对载波相位进行开环跟踪,重点改善接收机晶振钟漂对多普勒估计精度的影响。基于软件接收机对该方法进行性能评估,在部分GPS信号连续中断15 s情况下,其估计的载波相位误差小于1/4周的概率在90%以上。     

基于EGM模型的多波束无验潮测深技术应用

多波束水深测量中受潮汐因素的影响,测量垂直基准是变化的,具有瞬时性。传统多波束测量,需在测区内设立一个或多个验潮站进行同步水位观测,最终将水深归算到深度基准面上。针对多波束水深测量中垂直基准转换的复杂性问题,文中基于地球重力场模型,结合测区内实测的GNSS/水准数据,通过插值算法建立了测区范围内似大地水准面精化模型,构建了多波束无验潮水深测量的垂直基准转换模型。通过实例表明,该方法有效地消除了潮汐、动态吃水及涌浪等因素影响,直接获取深度基准面的水深值,提高工作效率,可满足近岸多波束水深测量的工作需求。     

多波束测深数据中系统偏差改正方法研究——以 2003 年 SeaBat900X 东海调查数据为例

多波束测量过程中,受到多种因素的影响,不可避免地存在各种误差,其中系统某个部件出现故障也不少见,如换能器、行波管、大功率微波开关或表层声速仪等器件功能不正常,引起多波束每 ping (一个发射接收周期） 数据中部分固定波束号的测深结果发生系统性偏移,以 2003 年东海调查 SeaBat900X 数据为例,其在垂直航向正投影平面上出现类似“W”字型的系统误差。本文基于该批次数据,系统分析了该类型系统偏差成因及外观表现,针对性提出基于等均值-方差拟合模型的改正方法,首先对异常区域和正常区域分别拟合地形趋势线,统计其均值和方差;然后以正常区域为基准,对异常区域内数据进行压缩和移动;最后通过面积差法,对数据中存在的折射残差进行消除,从而有效去除“W”型残差。文中实测数据验证了本文算法的有效性和可行性,对多波束其他类型的测深系统偏差处理具有一定的参考意义。     

卡尔斯伯格脊 60°~61°E洋脊段多波束后向散射特征及其对构造与岩浆作用强度的指示

多波束声纳数据可以有效记录海底地形地貌和底质特征信息。本文利用船载多波束数据对慢速扩张的卡尔斯伯格脊60°~61°E洋脊段的典型构造地貌单元的后向散射强度特征进行了研究,在此基础上,分析了该洋脊段的构造和岩浆作用强度特征。结果表明,洋脊段I以构造拉张作用占主导,脊轴及附近后向散射强度为-29 dB左右,裂谷壁高差可达1 200 m以上,裂谷内断裂发育,裂谷侧翼高度与裂谷宽度的比值为78.7~126.2,裂谷两侧翼部线性构造较少,但轴向正断层面更宽,倾角更小;与洋脊段裂谷中段相比,末端火山活动频率较低但喷发规模较大,火山机构数量和体积也更大,且可发育深大断裂获取深部热源。洋脊段II以岩浆作用占主导,脊轴及附近后向散射强度达-35 dB,裂谷内轴向火山脊发育,裂谷壁高差小于500 m,裂谷侧翼高度与裂谷宽度的比值为77.6~116.8,裂谷两侧翼部线性构造数量众多、长宽比较大且呈近似对称,相邻线性构造之间沉积物广泛分布。通过提取挖掘与底质属性密切相关的多波束后向散射强度数据,结合海底地形地貌的分析,可以为洋中脊的构造和岩浆作用强度的定量研究提供有效的证据。     

混浊水域多波束反向散射强度传播损失改正

为了改善现有的反向散射强度传播损失改正方法在混浊水域适应性较弱的问题,提出了混浊水域声传播损失计算模型。首先利用不同深度的海洋环境参数构建声波吸收系数剖面,然后基于声速,沿波束传播路径,对每个波束分层计算传播损失。实验分析表明,本方法传播损失改正效果最佳,其Spearman等级相关系数绝对值仅为0.04,远小于传统模型和TVG改正,大大减弱了混浊水域情况下多波束回波强度与传播距离的相关性,有效改善了多波束声呐图像的质量。     

Investigation of LO-Coupled Noise for a Sideband Separation Superconducting SIS Receiver

The Superconducting Superconductor-Insulator-Superconductor (SIS) receivers have become the preferred method for (sub)millimeter-wave radio astronomical observations due to the extremely low receiver noise temperature. The coupling noise of the local oscillator (LO) system is also a part of the receiver noise. In many years of astronomical observations, it is found that the LO-coupled noise cannot be completely ignored, which has a certain impact on the sensitivity of astronomical observations. The noise temperature of the superconducting SIS receiver was tested using two different kinds of signal generators as the primary signal source of the LO system. It is found that the base noise output by the signal generator can be coupled into the receiver to increase the receiver noise. By adding a narrow band filter to the output of the signal generator, the base noise of the signal generator can be filtered out, and this part noise of the receiver can be eliminated, the overall noise of the receiver is reduced, and the sensitivity of the telescope is improved.