微型无人机在“现代摄影测量实习”课程教学改革中的应用

“现代摄影测量实习”是中国地质大学(北京)土地科学技术学院测绘工程专业的重要实习课程,直接关系到学生的测绘技能培养。本文以笔者的教学实践为基础,从教学内容、教学方法、实践过程等方面探讨“现代摄影测量实习”实践中的教学改革问题,以帮助测绘工程专业学生获得良好的现代摄影测量技能,提高其就业与科研核心竞争力。     

最近和即将发生的崩解事件不会削弱埃默里冰架的稳定性

冰架崩解约占南极物质损耗总量的一半。借助卫星遥感本世纪已经观测到多次大型崩解事件,引发了公众对气候变化问题的广泛关注。然而作为冰架消涨的自然循环,某些崩解事件只是周期性重现而并非近年来南极升温导致。2019年9月-10月,我们通过“哨兵一号”雷达卫星和“京师一号”小卫星完整地记录到发生在埃默里冰架前端的一次大型崩解事件,并利用冰流数值模式模拟了本次以及未来两次即将发生的崩解事件对该冰架的动力学影响。遥感观测表明,埃默里冰架前端发育有两条纵向、两条横向和一条斜向共五条大型裂隙。它们沿尖端继续向上游延伸可以造成三次崩解事件,其中第一次发生于2019年9月末,D28冰山随普里兹湾涡流向西北方向旋转漂移。依据前人推测的崩解周期,我们在模型中设置五组试验,选择露出海面体积、接地面积、冰流通量三个参数估算冰架对三次崩解的响应。结果表明,通过设计合理的网格系统,我们的模型能够捕捉到每次崩解事件释放的物理信号。三次崩解总体响应趋于一致,仅表现出微弱的差异。在一个60年的崩解周期内,三次崩解引发冰流加速70 m/a,前端减薄2 m,接地线退缩60 km2,共约造成40亿吨额外的物质损耗。然而上述变化仍然处于最新卫星估算误差内部,所以我们认为这些崩解事件并不会显著削弱埃默里冰架整体的稳定结构。考虑到这还是首次明确观测到该冰架进入新一轮崩解周期,未来仍必要收集更长时间序列的遥感资料用以验证模式结果。     

印度河上游Bagrot山谷降水稳定同位素变化及与水汽来源的关系

利用2015年8月至2016年7月在印度河上游流域Bagrot山谷降水稳定同位素（δ18O和δD）观测结果以及当地气象资料,利用同位素示踪及统计分析方法,并结合HYSPLIT模型,对研究区降水稳定同位素变化特征、大气水线以及水汽来源进行了分析。结果表明,观测期间Bagrot山谷降水稳定同位素的季节变化明显,δ18O与δD秋冬季偏低,春夏季偏高,且与气温变化一致,存在显著的温度效应,而降水量效应不明显。而且发现,研究区局地大气水线截距和斜率均低于全球的,反映了降水过程中云下二次蒸发作用较为强烈,特别是,不同的降水形态导致该研究区局地大气水线的斜率和截距不同。当液态降水（降雨）发生时,由于在较为干旱的气候环境下,雨滴在降落的过程中受到二次蒸发相对较强,使得局地大气水线的斜率和截距偏低;而当固态降水（降雪）发生时,由于温度较低,受再循环水汽和二次蒸发的影响较小,导致局地大气水线的斜率和截距均偏高。Bagrot山谷及其周边地区,从南到北局地大气水线的斜率相差不大,而其截距总体上随着纬度升高而降低,可能与云下二次蒸发导致稳定同位素发生的不平衡分馏逐渐强烈有关。通过Bagrot山谷站点降水稳定同位素观测结果并结合HYSPLIT模型的后向追踪,研究还发现,研究区全年主要受西风环流以及局地环流的影响。但与研究区以北的临近站点（慕士塔格、和田等）相比有所不同,由于Bagrot山谷位置更靠南,其仍然偶尔受到来自南方的海洋性水汽影响。这一研究结果可能对该地区树轮稳定同位素记录的解译具有一定的指示意义。     

吐哈盆地长流水地区铀矿成矿前景分析

在吐哈盆地中东部地区已投入部分铀矿找矿工作,但是没有取得较好的成果,本文拟对吐哈盆地中东部长流水地区铀成矿条件进行前景分析,对找矿提供一定的理论依据。研究区位于骆驼圈子浅凹陷中,南部蚀源区总体铀含量较高,目的层也具有较高的铀背景值,满足地下水的"补—径—排"条件,层间氧化带发育,通过钻探工作发现部分的铀异常以及铀矿化现象,具有较好的成矿条件。     

Examination of Extraordinary Transmission of Waves Propagation through Gaps of Vertical Thin Barriers in Channels by A Hypersingular Boundary Element Method

The extraordinary transmission(ET) phenomenon is examined for waves propagating through gaps of vertical thin barriers in channels with a hypersingular boundary element method model on the linear potential theory, and an estimate formula based on small gap approximation for predicting the number of ET frequencies is proposed.Numerical computations are carried out to examine the influences of barrier number, barrier interval, gap size, gap position and barrier arrangement on extraordinary transmission and wave height in the channel. It shows that all of those factors evidently affect the extraordinary transmission frequencies. The contours of wave amplitude show that very high waves can be excited in the basins between barriers at the extraordinary transmission frequencies. Proper arrangement of barriers in a channel can avoid the occurrence of ET phenomenon and reduce wave height in the channel.     

The genetic diversity,individual relatedness and possible mating system of an isolated population of the Cyprinid species Megalobrama pellgrini in upper reaches of the Changjiang (Yangtze) River,China

Megalobrama pellegrini is a cyprinid fish endemic to upper reaches of the Changjiang(Yangtze) River, China, which is also an important economic species in the local area. In recent years,resources of this species have decreased sharply and its conservation has drawn great attention. In the present study, we collected 120 individuals from the Longxi River, a tributary isolated from the main channel of the Changjiang River, where M. pellegrini is still relatively abundant. Using two different molecular markers, mitochondrial cytochrome b(cyt b) gene, and nuclear microsatellite(simple sequence repeat,SSR), we analyzed the genetic diversity of this isolated population. The results show that sequence genetic diversity was low(H_d:0.290 and P_i: 0.000 77 for cyt b gene),while the SSR genetic diversity was high(H_o:0.824 4±0.147 2,H_e: 0.823 510.145 1). Analysis indicated that this population had experienced a bottleneck,with inbreeding and small effective population size(around 50). Based on SSR data, relatedness analyzing revealed that the 120 samples were grouped into 10 completely independent clusters. It was inferred that the mating system of M. pellegrini was polygamy. We suggested that the low genetic diversity could be induced by the overfishing and inbreeding depression. Therefore, we suggested that the urgent conservation measures should be taken to control the overfishing and give better conditions for the fish to grow and spawn, then to restore population size.     

郯庐断裂带苏皖段及邻区b值时空特征研究

采用郯庐断裂带苏皖段及邻区近50 a的地震数据,在定量分析区域最小完备震级Mc和推导b值计算的极大似然法基础上,重点研究G-R关系,尤其是b值时空分布演化特征,并依据b值指示意义进行5级以上地震关联性和断裂带影响区域的构造应力分布状况分析.结果显示,依据b值的时间分布特征,研究区中强地震发生时段与中短期b值下降时段关联...     

4D-DECT对甲状旁腺腺瘤的诊断价值

目的:探讨甲状旁腺腺瘤(PA)的4D-DECT影像特征及物质成分信息,评价其定位及定性诊断价值.资料和方法:回顾性分析经手术及病理证实的53例PA患者的临床资料及4D-DECT影像资料,逐一观察并记录CT征象,分别对病变与邻近组织的CT衰减值(HU)、碘浓度、Rho、Z值及DEI进行测定及比较分析.结果:53例患者中,...     

“人工鲸落”型海洋牧场的理论基础与构建体系

海洋牧场作为新的生态型海洋渔业生产方式,同时也是我们获取优质蛋白的重要来源,近年来得到快速发展,目前已形成了增殖型、养护型和休闲型海洋牧场建设模式。随着海洋强国战略的加快实施,海洋牧场逐渐挺进深蓝,在其快速发展的同时也存在建设模式单一、同质化现象突出和生态承载力提升受限等问题,在一定程度上限制了海洋牧场的创新发展。而鲸落生态系统作为海洋生态系统的一部分,其生态作用对海洋牧场的发展将会起到显著的促进作用。文章在系统梳理海洋牧场发展历史和鲸落生态系统原理的基础上,把二者有机结合,将鲸落形成的生态原理充分运用到海洋牧场建设过程中,构建人工鲸落型海洋牧场技术体系和建设模式,通过人工方式充分发挥鲸落等大型动物外源性营养物质的规模化输入效应,提升海洋牧场区域生产力,进而提高资源养护与产出能力,以期为我国海洋牧场建设发展提供新的思路和方向参考。     

Direct constraint on cosmic neutrino mass using observational Hubble parameter data

In order to explore the properties of cosmic neutrinos, i.e. sum of the neutrino mass(∑m_ν) and the effective number of neutrino species(N_(eff)), which affects the Hubble expansion rate H(z)and the power of observational Hubble parameter data(OHD) in constraining cosmological parameters under the ΛCDM model, we utilize OHD to constrain the properties of cosmic neutrinos and apply an accurate H(z) function with mνand Neff. First, we simulate new OHD beyond the existing 43 OHD. According to the predictions of measurements of H_0(the current H(z) value), baryon acoustic oscillations(BAO) peaks, Sandage-Loeb(SL) test and cosmic microwave background(CMB), we assume observational accuracy up to 2% and redshift 0 z ≤5. With simulated H(z) data obtained from the fiducial model, we constrain the parameters including mνand Neff. When all parameters are set free, mν 0.196 eV(95%) and N_(eff)= 2.984 ± 0.826(68%) are obtained, and when fixing Neff as the standard baseline 3.046, we attain ∑m_ν 0.240 eV(95%). These constrained results are much tighter than the ones obtained by the current OHD, which makes the prospect of OHD in constraining cosmological parameters more promising as its accuracy and quantity grow.