基于IHO S-44不同测量等级的船速控制研究

通过船不同航速下对海底地形测量影响的仿真,给出相应情况下多波束测深仪波束对测区的覆盖情况,得出了航速不当时将无法实现对测区全覆盖的结论。据此问题推导了基于国际海道测量标准的船速控制模型,并针对SeaBat8101多波束测深仪给出不同测量等级的船速控制指标。     

光谱和体重对刺参耗氧率和排氨率的影响

实验采用室内受控的方法,研究了不同光色下,大(73.32±1.73) g、中(46.71±0.15) g和小(25.67±0.25) g 3种规格刺参(Apostichopus japonicus)的耗氧率和排氨率的变化.实验采用红、橙、黄、绿、蓝色和对照组(白色)6种光照处理.研究结果表明:光谱对刺参的耗氧率和排氨率均有显著性影响(P<0.05),3种规格刺参的耗氧率趋势相同:白色＞红色、黄色、绿色、蓝色＞橙色;3种规格刺参的排氨率有相似的变化趋势:白色＞红色＞橙色、绿色、黄色、蓝色.刺参的体重与单位体重耗氧率及排氨率之间的回归关系均可以表示为R=aW~b,耗氧率a值在0.005 9～0.012 1之间,b值范围是1.119 7～1.214 6,排氨率a值的变动范围为0.004 2～0.02,b值的变动范围为0.455 3～0.867 8.这说明光谱对刺参的耗氧率和排氨率有显著性的影响,丰富了刺参的基础研究,对于刺参养殖生产有一定的指导意义.     

2005～2015年中国高校科研人才的时空变化及影响因素分析

基于2005~2015年全国统计年鉴数据,采用统计地图法和空间自相关分析,分析中国高校科研人才的时空分布特征（不包括港澳台数据）,并采用面板负二项回归模型,识别高校科研人才空间分布的决定因素。研究结果表明:①中国的高校科研人才分布表现出较强的空间不均衡性,总体趋势为东南密集,西北稀疏,科研人才高度集中在北京、天津、上海;②高校科研人才分布具有一定的空间集聚特征,其热点地区为北京、天津、上海和江苏等沿海省市,冷点地区集中分布在广大的西部地区和黑龙江省。2005~2015年,高级职称人才的空间集聚程度有所减弱,而中初级职称科研人才的空间集聚程度有所加强;③人才政策、高等教育规模和层次、公共服务水平和信息化水平是所有高校科研人才空间分布的主要影响因素。从职称差异的角度来看,薪酬和失业率等经济因素仅对初级职称科研人才的分布有影响,医疗、文化公共服务水平和人才政策仅对中高级职称科研人才的分布有影响,高等教育的规模与层次对各种职称人才的分布均有影响;从地区差异的角度来看,西部地区高校科研人才受到经济因素影响更为明显,而中东部高校科研人才受到公共服务水平影响的更为明显。     

东北三省城乡协调发展格局及影响因素

以东北三省36个地区为研究对象,系统构建了城乡协调的指标体系,采用基尼系数、空间自相关和空间回归等方法探讨了2005年、2010年和2015年东北三省城乡协调的空间格局和影响机制。研究表明:① 东北三省城乡协调度的区域差异不断扩大且具有明显的空间集聚特征,但集聚程度趋于减弱。② 不同地区城乡协调水平变化各异。研究期内,大连市和锦州市一直处于高水平城乡协调状态,朝阳市长期处于低水平城乡协调状态。鹤岗市和七台河市城乡协调度位次上升最明显,哈尔滨市和辽源市城乡协调度位次下降最显著。③ 从空间格局来看,中级城乡协调区增多且向北移动,初级城乡协调区减少且向中部集中,“南北高,中间低”的城乡协调格局基本形成。与此同时,城乡协调的冷热点均不断收缩,空间极化效应趋于减弱。④ 城镇化和农业规模化经营是促进东北城乡协调发展的主要力量,工业化并未显著促进东北城乡协调发展且与城乡协调发展负相关,农业现代化经营对城乡协调发展有正向作用,交通因素在近些年的促进作用逐渐凸显,经济发展水平与信息化水平对东北城乡协调发展的作用还不明显。     

1997—2017年塔克拉玛干沙漠腹地降水特征

利用塔克拉玛干沙漠腹地塔中气象站1997—2017年逐日和逐时降水资料,分析塔克拉玛干沙漠腹地降水日变化特征、极端强降水特征及其天气背景。结果表明：1997—2017年研究区降水量呈增加趋势、降水日数呈减少趋势,大雨雨量和雨日明显增加,降水呈增强演变。降水多见于6月,最大雨强为8.4 mm·h^-1。降水量日变化呈多峰特征,降水量最大值出现在23：00,06：00是降水频次最多时刻。降水强度和降水频次对降水量作用不同,午后至前半夜强度大,频次少;而后半夜至清晨频次多,强度小。降水以短历时降水为主,其中1～3 h的短历时降水对总降水量贡献率高达61.76%。日降水和小时降水的99百分位强度阈值分别为15.3 mm·d^-1和6.0 mm·h^-1,大于90百分位极端降水量占总降水量贡献率近半。极端强降水天气发生在南疆盆地受北纬40°以南低槽、切变槽或弱的气旋式风场控制地区,南疆盆地提前增湿,民丰850 hPa比湿接近或超过10 g·kg^-1的背景下,降水连续性较差,多中小尺度引发局地短时降水。     

水资源约束下的河西走廊城市经济脆弱性时空演变及其影响因素

城市经济脆弱性作为当前脆弱性研究中的重要领域,为人-地系统耦合研究提供了新的视角,并为城市可持续健康发展提供有益的决策支持和管理方法。依据城市经济脆弱性内涵,基于暴露度、敏感性、适应能力构建了城市经济脆弱性评价指标体系,运用熵权TOPSIS法评价河西走廊地区及区域内五市的城市经济脆弱性,并采用障碍度模型识别影响区域城市经济脆弱性变化的因素。结果显示：（1）2006—2015年,河西走廊地区城市经济脆弱性呈现出先曲折下降（2006—2011年）再波动上升趋势（2012—2015年）;（2）河西走廊地区的城市经济脆弱性具有明显的空间特征,经历了东西高、中部低到整体较高的演变过程;（3）阻碍河西走廊地区城市经济脆弱性降低的障碍因子由适应能力逐步转变为暴露度。针对河西走廊地区各市主要障碍因子,提出针对性优化措施。     

湍流度随高度的变化及其对城市宏观地形的依赖

分别构建广州主建成区垂直比例尺为1﹕2 000、1﹕1 000和1﹕500的3个建筑物模型,利用大型边界层风洞,在西北和东南两风向下,基于中性流模拟分析了复杂城市地形下湍流度随高度的变化及其对宏观地形的依赖。结果表明：风廓线指数α与不同高度的湍流度之间的关系密切,利用现有模型,根据4类粗糙度边界层和不同垂直比例尺,可确定相应的湍流度随高度变化模型的主要系数,预测精度高。城市地形下最大湍流度面发育在0~0.2 h之间狭窄的范围内。用湍流度形态指数β来表征湍流度随高度的变化,无论城市屋脊还是平坦地形,随着风程区的延伸,廓线的指数α升高,湍流度形态指数β降低。表明同一高度湍流度值具有由迎风区、丘顶区向背风区增高,沿风程逐渐增大的规律,对地形部位和风程的依赖性强,与来流翻越简单地形时的特征一致。     

On the Collision Nature of Two Coronal Mass Ejections: A Review

Observational and numerical studies have shown that the kinematic characteristics of two or more coronal mass ejections (CMEs) may change significantly after a CME collision. The collision of CMEs can have a different nature, i.e. inelastic, elastic, and superelastic processes, depending on their initial kinematic characteristics. In this article, we first review the existing definitions of collision types including Newton’s classical definition, the energy definition, Poisson’s definition, and Stronge’s definition, of which the first two were used in the studies of CME–CME collisions. Then, we review the recent research progresses on the nature of CME–CME collisions with the focus on which CME kinematic properties affect the collision nature. It is shown that observational analysis and numerical simulations can both yield an inelastic, perfectly inelastic, merging-like collision, or a high possibility of a superelastic collision. Meanwhile, previous studies based on a 3D collision picture suggested that a low approaching speed of two CMEs is favorable for a superelastic nature. Since CMEs are an expanding magnetized plasma structure, the CME collision process is quite complex, and we discuss this complexity. Moreover, the models used in both observational and numerical studies contain many limitations. All of the previous studies on collisions have not shown the separation of two colliding CMEs after a collision. Therefore the collision between CMEs cannot be considered as an ideal process in the context of a classical Newtonian definition. In addition, many factors are not considered in either observational analysis or numerical studies, e.g. CME-driven shocks and magnetic reconnections. Owing to the complexity of the CME collision process, a more detailed and in-depth observational analysis and simulation work are needed to fully understand the CME collision process.     

Long term evolution of distant retrograde orbits in the Earth-Moon system

This work studies the evolution of several Distant Retrograde Orbits (DROs) of varying size in the Earth-Moon system over durations up to tens of millennia. This analysis is relevant for missions requiring a completely hands off, long duration quarantine orbit, such as a Mars Sample Return mission or the Asteroid Redirect Mission. Four DROs are selected from four stable size regions and are propagated for up to 30,000 years with an integrator that uses extended precision arithmetic techniques and a high fidelity dynamical model. The evolution of the orbit’s size, shape, orientation, period, out-of-plane amplitude, and Jacobi constant are tracked. It has been found that small DROs, with minor axis amplitudes of approximately 45,000 km or less decay in size and period largely due to the Moon’s solid tides. Larger DROs (62,000 km and up) are more influenced by the gravity of bodies external to the Earth-Moon system, and remain bound to the Moon for significantly less time.     

Effects of Salinity Fluctuation Frequency on the Growth, Molting Rate and Hemolymph 20-Hydroxyecdysone Concentration in Juvenile Chinese shrimp, Fenneropenaeus chinensis

This experiment was conducted to examine the effects of salinity fluctuation frequency on the growth, molting rate and hemolymph 20-hydroxyecdysone (20-HE) concentration for juvenile Fenneropenaeus chinensis with an initial wet body weight of 1.115 g±0.012 g. The salinity of the control treatment (represented by D0) was 28 throughout the experiment, whereas treatments D2,D4, D6 and D8 were subjected to different salinity fluctuation frequencies of 2, 4, 6 and 8d, respectively. The range of salinity fluctuation was 4. The salinity in treatments D2, D4, D6 and D8 was kept at 28 for 2, 4, 6 and 8d, respectively; each original salinity was decreased abruptly to salinity 24, which first lasted for another 2d and was then raised to its initial value 28. This constituted a salinity fluctuation cycle and afterwards the cycle repeated. It was found that: 1) The weight gain of shrimp in treatment D4 was 202.9% and significantly higher than that in treatment D0 (P<0.05). The molting rate in treatment D2 was the lowest, while that in treatment D6 was the highest and significantly higher than those in treatments D0 and D2 (P<0.05). 2) The hemolymph 20-HE concentration of shrimps in all treatments was at low levels and increased first gradually during the inter-molt period and then increased sharply. It reached a peak value during the pre-molt stage, and then decreased abruptly during the post-molt stage when the lowest level occurred. 3) During the post-molt stage, the hemolymph 20-HE concentration in treatment D2 was 7.47pgμL-1 and significantly higher than that in treatment D0(P<0.05). There were, however, no significant differences in hemolymph 20-HE concentration among all five treatments during the inter-molt stage (P>0.05). During the pre-molt stage, the hemolymph 20-HE concentration in treatment D6 was significantly higher than that in treatment D0(P<0.05), whereas the hemolymph 20-HE concentration in treatment D2 was significantly lower than that in other treatments (P<0.05). Adequate salinity fluctuation promoted the molting rate through increasing hemolymph 20-HE concentration at the pre-molt stage.