三个文蛤家系双列杂交设计在两种环境下的配合力及杂种优势分析

A 3×3 complete diallel cross comprising three families of the clam Meretrix meretrix(P1, P2 and P3) was used to determine the combining ability of parental families and heterosis of F1 under indoor and openair environments for growth traits. Analysis of variance for shell length and whole body weight indicated highly significant cross effects, environment effects and the interaction of cross by environment. General combining ability(GCA) and specific combing ability exhibited great variation among crosses and between two environments. Pooled over environments, P2 was the top combiner among the three parental families for both traits studied. The cross of P1 and P3 had the highest SCA. Additionally, significant reciprocal effects were observed. For individual environment, about half of the crossbred combinations showed favorable Mid-parent heterosis(MPH)(1%) for the shell length and whole body weight. Our data has shown that non-additive genetic and reciprocal effects constituted the major sources of genetic variation for both shell length and whole body weight, which indicates that crossbreeding among selective families could further explore the heterotic effects.     

利用卫星云图估算焦作市4-9月12h降水

利用2004-2006年FY-2C卫星云图资料,统计了云顶亮温与焦作市降水量的关系;并根据相邻两张云图中云顶低亮温中心移动的距离和时间,确定云的移速。在此基础上,建立了层状云和积状云降水估算方程。经对2005-2006年估算结果统计,层状云有无降水预报准确率为80%;对4次积状云降水的估算结果为1次漏报、1次降水量级误差较大、2次预报正确,准确率达50%。     

热带气旋快速加强与海表温度分布统计特征研究

为加强海表温度对热带气旋快速加强影响的认识,利用中国气象局上海台风研究所整编的热带气旋最佳路径数据集和欧洲中尺度天气预报中心提供的海温数据,选取1979−2019年期间的西北太平洋热带气旋,统计分析了海温和热带气旋强度快速变化的特征。研究结果表明：（1）约90%的热带气旋快速加强发生在夏季和秋季,分别占快速加强总次数的32.8%和56.4%,绝大部分热带气旋以跨越1个强度等级的快速加强为主,由强热带风暴快速加强到台风和由台风快速加强到强台风是出现次数较多的两种情况。（2）夏季大于28℃,秋季大于27.5℃的海表温度条件有利于热带气旋快速加强,较低强度等级的热带气旋需要更高的海表温度（> 29℃）才易出现快速加强;热带气旋快速移动有利于其中心处海温维持较高状态。（3）海温的时间变率在±0.2℃/(6 h)内,水平空间梯度低于0.4℃/(°)是热带气旋快速加强的有利条件;热带气旋强度越强,越需要平稳的海表温度环境。（4）热带气旋处于强热带风暴及以上级别时,仅利用海表温度条件对其是否发生快速加强的判断准确性较好。这一工作量化了有利于热带气旋加强的海表温度环境,为业务上基于海表温度定量预报热带气旋强度演变提供了一种技术参考。     

top-hat变换与庐枞矿集区大地电磁强干扰分离

作为一种非线性信号处理方法,基于数学形态学的广义形态滤波已经展现出其在大地电磁时间域信号去噪中的作用;然而,广义形态滤波在滤除大地电磁时间域信号中噪声波形的同时,也滤除了时间域信号中包含有用信息的缓变化。针对这一问题,提出一种基于数学形态学top-hat变换的大地电磁时间域噪声压制方案,利用top-hat变换对波峰和波谷的检测能力,采用直线型结构元素,对大地电磁时间域信号进行去噪。用该方法对庐枞矿集区大地电磁实测数据进行处理后,数据的标准差与曲线相似性参数都优于处理前数据,表明所提方法能够去除噪声波形并保留时间域信号的缓变化,恢复受噪声污染的大地电磁时间域信号,提高大地电磁视电阻率曲线的质量。     

厦门港疏浚弃土吹填造陆物理模型试验研究

通过厦门港潮汐水流整体物理模型试验，掌握了厦门港十万吨级深水航道二期工程疏浚弃土吹填造陆各方案实施前后港池航道水流流态，为规划设计单位和决策部门利用疏浚弃土吹填造陆提供可靠的科学依据，试验结果表明，海沧吹填工程可作为一期吹填方案，鸡屿西吹填造陆工程可作为海沧吹填工程的后续工程，仅从水流角度考虑，象鼻嘴吹填造陆方案1是可行的。     

利用高分辨率航天遥感影像实现城市3维可视化

利用高分辨率遥感影像提取地物数据，并采取面向对象的空间数据模型对数据进行管理，使用虚拟现实技术对城市景观进行3维重建，然后利用有理函数数学模型表示遥感影像与地面之间的构像关系。使用纹理映射技术，构建具有高度真实感的城市3维景观图。     

The inner solar system cratering record and the evolution of impactor populations

We review previously published and newly obtained crater size-frequency distributions in the inner solar system. These data indicate that the Moon and the terrestrial planets have been bombarded by two populations of objects. Population 1,dominating at early times, had nearly the same size distribution as the present-day asteroid belt, and produced heavily cratered surfaces with a complex, multi-sloped crater size-frequency distribution. Population 2, dominating since about 3.8–3.7 Gyr,had the same size distribution as near-Earth objects(NEOs) and a much lower impact flux, and produced a crater size distribution characterized by a differential –3single-slope power law in the crater diameter range 0.02 km to 100 km. Taken together with the results from a large body of work on age-dating of lunar and meteorite samples and theoretical work in solar system dynamics, a plausible interpretation of these data is as follows. The NEO population is the source of Population 2 and it has been in near-steady state over the past ～ 3.7–3.8 Gyr; these objects are derived from the main asteroid belt by size-dependent non-gravitational effects that favor the ejection of smaller asteroids. However, Population 1 was composed of main belt asteroids ejected from their source region in a size-independent manner, possibly by means of gravitational resonance sweeping during orbit migration of giant planets;this caused the so-called Late Heavy Bombardment(LHB). The LHB began some time before ～3.9 Gyr, peaked and declined rapidly over the next ～ 100 to 300 Myr,and possibly more slowly from about 3.8–3.7 Gyr to ～2 Gyr. A third crater population(Population S) consisted of secondary impact craters that can dominate the cratering record at small diameters.     

斜长石韵律环带的结晶速率方程及其动力学机制

根据物理化学基本原理,建立了斜长石韵律环带形成的数学模型。从晶体生长的基本原理出发,提出了按非连续机制生长的斜长石晶体结晶速率表达式。该速率表达式具有过饱和→成核→耗尽循环的反馈特征。斜长石中小尺度韵律环带起因于自组织过程,而与环境因素无关。其成因对应着相对静态的环境。     

贵州关岭生物群中植物化石的发现及其意义

关岭生物群是近年来在我国贵州关岭地区瓦窑组中发现的一个十分重要的生物群 ,其中的植物化石经研究计有 Equisetites cf.arenaceus(Jaeger) Bronn.、Ctenozamitessarrani Zeiller。依据植物化石 C.sarrani常见于晚三叠世和 E.cf.arenaceus系似木贼属中较古老的类型 ,指出含植物化石的地层时代为晚三叠世卡尼期。瓦窑组系海相沉积 ,其中的植物化石无疑为异地埋藏 ,但从化石通常保存尚好来看 ,估计搬运的距离不会很远 ,它们可能是从距海岸不远的陆地被河流带到较平静的海湾或海槽而沉积下来的。此外 ,从该组植物茎干化石具清楚的年轮分析 ,推测卡尼期时 ,贵州关岭一带为非热带雨林地区 ,一年中气候不是四季如一 ,而是有明显的季节变化     

波包传播诊断的理论基础和计算方法

文中提出了一种新的利用实际观测资料研究波包传播的诊断方法 (WPD) ,并通过理想资料和实际资料的计算证明了该方法的可用性和广泛性