东南极中山站陆缘固定冰2011/2012年度的时空变化

Annual observations of first-year ice(FYI) and second-year ice(SYI) near Zhongshan Station, East Antarctica,were conducted for the first time from December 2011 to December 2012. Melt ponds appeared from early December 2011. Landfast ice partly broke in late January, 2012 after a strong cyclone. Open water was refrozen to form new ice cover in mid-February, and then FYI and SYI co-existed in March with a growth rate of 0.8 cm/d for FYI and a melting rate of 2.7 cm/d for SYI. This difference was due to the oceanic heat flux and the thickness of ice,with weaker heat flux through thicker ice. From May onward, FYI and SYI showed a similar growth by 0.5 cm/d.Their maximum thickness reached 160.5 cm and 167.0 cm, respectively, in late October. Drillings showed variations of FYI thickness to be generally less than 1.0 cm, but variations were up to 33.0 cm for SYI in March,suggesting that the SYI bottom was particularly uneven. Snow distribution was strongly affected by wind and surface roughness, leading to large thickness differences in the different sites. Snow and ice thickness in Nella Fjord had a similar "east thicker, west thinner" spatial distribution. Easterly prevailing wind and local topography led to this snow pattern. Superimposed ice induced by snow cover melting in summer thickened multi-year ice,causing it to be thicker than the snow-free SYI. The estimated monthly oceanic heat flux was ～30.0 W/m2 in March–May, reducing to ～10.0 W/m2 during July–October, and increasing to ～15.0 W/m2 in November. The seasonal change and mean value of 15.6 W/m2 was similar to the findings of previous research. The results can be used to further our understanding of landfast ice for climate change study and Chinese Antarctic Expedition services.     

丁字湾近岸海域表层沉积物粒度特征及沉积动力环境

根据丁字湾近岸海域126个表层沉积物样品粒度分析结果,对沉积物类型和粒度参数分布进行了总结。在此基础上,利用粒径趋势分析模型(GSTA)和沉积动力判别图解,探讨了表层沉积物的运移趋势及沉积水动力规律。结果表明,丁字湾近岸海域表层沉积物类型共有8种,其中砂、砂质粉砂和粉砂分布最广泛;平均粒径具有从岸向海逐渐变细的特征,分选性、偏度和峰度分别具有较差—差、正偏—极正偏、中等的特征;粒度运移趋势分析反映出湾口海岸附近泥沙由两侧向湾口中心运移,远离海岸泥沙由北西向南东偏东方向运移;沉积动力判别图解揭示出丁字湾海域沉积水动力具有整体较强,由岸向海方向逐渐减弱的特征。     

低分子质量κ-卡拉胶钾的酶法制备及其对原发性高血压大鼠降血压作用的研究

为了探究低分子质量κ-卡拉胶钾对原发性高血压大鼠(spontaneously hypertensive rat, SHR)血压的影响,以κ-卡拉胶粉为原料,酶解法和醇沉法相结合制备分子质量为3.5 kDa的低分子质量κ-卡拉胶寡糖(low-molecular-weightκ-carrageenan, LC)。将LC与KCl溶液混合,经醇沉操作除去游离的钾离子,以此获得高结合率的低分子质量κ-卡拉胶钾(low-molecular-weightpotassiumκ-carrageenan,LCP),使得LC中结合型钾元素的含量由原先的6.5%上升至8.7%。各组灌胃剂量:实验组600mg/kgLCP,空白组灌胃蒸馏水,阳性对照组10 mg/kg卡托普利。结果显示, LCP对SHR有稳定且持续的降压作用,与空白组相比,显著降压18mmHg。LCP显著降低了RAS系统中肾素(P0.05)和血管紧张素Ⅱ(AngⅡ)(P 0.01)的水平,推测LCP的降压机理可能是降低了RAS系统的活化程度;此外, LCP显著降低了血液中脂多糖(LPS)的水平(P 0.05),并显著改善了肠道上皮结构的完整性。     

小钦岛土壤理化性质及其影响因子

利用样带与样方结合法进行野外调查,测定土壤主要理化指标,基于SPSS 24. 0进行皮尔逊(Pearson)相关性分析、单因素方差(One-way ANOVA)分析和最小显著差数法(LSD)多重比较,对小钦岛土壤理化性质的统计学特征及其影响因子进行研究.小钦岛土壤砾石比和含水量平均值分别为20. 04%、7. 35%;铵态氮、速效钾、速效磷、有机质含量平均值分别为23. 67、212. 77、16. 15mg/kg、28. 34 g/kg,分别属于五级、一级、三级和三级水平,大部分属于三级土壤;有机质与含水量、铵态氮、速效磷均呈显著正相关.土壤理化性质主要受植被和坡向影响.通过丰富、加深对庙岛群岛的研究,旨在为海岛的生态保护及开发提供参考.     

小钦岛土壤理化性质及其影响因子

目的：观察外伤一方加减治疗手足外伤的临床疗效。方法：将手足外伤患者80例随机分为2组,每组各40例,对照组采用西医常规治疗,治疗组在对照组治疗基础上加本院自制的外伤一方治疗。比较2组患者的综合疗效、VAS评分及满意率。结果：总有效率治疗组为100.0%,对照组为85.0%,组间比较,差异有统计学意义（P＜0.05）;2组疼痛VAS评分及患者满意率比较,差异均有统计学意义（P＜0.05）。结论：外伤一方加减治疗手足外伤有较好的临床疗效,能明显降低患者疼痛程度,提高患者治疗满意度。     

Molecular analyses of bacterioplankton communities with highly abundant Vibrio clades: a case study in Bohai Sea coastal waters

We investigated the bacterioplankton abundance, community composition and the associated Vibrio clades of natural seawater in Bohai Sea coastal waters. Seawater samples (10 L in triplicate) were collected at 0.5, 3, and 5 m depths near the coastal aquaculture zone of the Bohai Sea on May 12, 2016. Real-time PCR and 16S rRNA gene amplicon high-throughput sequencing methods were employed by which 485 operational taxonomic units (OTUs) at a 97% sequence similarity level were generated. Gammaproteobacteria, Alphaproteobacteria, and Bacteroidetes were the most abundant groups, accounting for 49.5%, 23.5%, and 18.9% of the total assemblage, respectively. Obvious variations in Pseudoalteromonas, Vibrio, and Octadecabacter , which were the most abundant genera, could be observed among diff erent samples. Notably, the results of Vibrio -specifi c real-time PCR indicated that Vibrio had extremely high 16S rRNA gene copy numbers. The 16S rRNA gene sequencing results across all the samples also indicated that they occupied a large proportion of the total assemblage. Both the alpha diversity and major bacterioplankton group Pseudoalteromonas had significant correlations with the concentration of PO4^3-. Overall, studies on bacterioplankton communities with highly abundant Vibrio clades can provide interesting insight into the microbial function and health assessment of the Bohai Sea coastal ecosystem.     

A deep learning approach for detecting candidates of supernova remnants

Detecting supernova remnant(SNR) candidates in the interstellar medium is a challenging task because SNRs have weak radio signals and irregular shapes. The use of a convolutional neural network is a deep learning method that can help us extract various features from images. To extract SNRs from astronomical images and estimate the positions of SNR candidates, we design the SNR-Net model composed of a training component and a detection component. In addition, transfer learning is used to initialize the network parameters, which improves the speed and accuracy of network training. We apply a T-T plot(of the different brightness temperatures of map pixels at two different frequencies) to calculate the spectral index of SNR candidates. To accelerate the scientific computing process, we take advantage of innovative hardware architecture, such as deep learning optimized graphics processing units, which increases the speed of computation by a factor of 5. A case study suggests that SNR-Net may be applicable to detecting extended sources in the images automatically.     

Calibration of the DAMPE Plastic Scintillator Detector and its on-orbit performance

The DArk Matter Particle Explorer(DAMPE) is a space-borne apparatus for detecting the highenergy cosmic-ray-like electrons, γ-rays, protons and heavy ions. The Plastic Scintillator Detector(PSD)is the top-most sub-detector of the DAMPE. The PSD is designed to measure the charge of incident highenergy particles and it also serves as a veto detector for discriminating γ-rays from charged particles. In this paper, a PSD on-orbit calibration procedure is described, which includes the five steps of pedestal, dynode correlation, response to minimum-ionizing particles, light attenuation function and energy reconstruction.A method for reconstructing the charge of incident high energy cosmic-ray particles is introduced. The detection efficiency of each PSD strip is verified to be above 99.5%; the total efficiency of the PSD for charged particles is above 99.99%.     

Searching for GeV gamma-ray emission from the bulge of M31

The three major large-scale, diffuse γ-ray structures of the Milky Way are the Galactic disk,a bulge-like GeV excess towards the Galactic center, and the Fermi bubble. Whether such structures can also be present in other normal galaxies remains an open question. M31, as the nearest massive normal galaxy, holds promise for spatially-resolving the γ-ray emission. Based on more than 8 years of Fermi-LAT observations, we use(1) disk,(2) bulge, and(3) disk-plus-bulge templates to model the spatial distribution of the γ-ray emission from M31. Among these, the disk-plus-bulge template delivers the best-fit, in which the bulge component has a TS value 25.7 and a photon-index of 2.57 ± 0.17, providing strong evidence for a centrally-concentrated γ-ray emission from M31, that is analogous to the Galactic center excess. The total0.2–300 GeV γ-ray luminosity from this bulge component is(1.16 ± 0.14) × 1038 erg s-1, which would require ～ 1.5 × 105 millisecond pulsars, if they were the dominant source. We also search for a Fermi bubble-like structure in M31 using the full dataset(pass8), but no significant evidence has been found.In addition, a likelihood analysis using only photons with the most accurate reconstructed direction(i.e.,PSF3-only data) reveals a 4.8 σ point-like source located at ～10 kpc to the northwest of the M31 disk, with a luminosity of(0.97 ± 0.27) × 1038 erg s-1 and a pho@ton-$i·nd3 ex of 2.31 ± 0.18. Lacking a counterpart on the southeast side of the disk, the relation between this point-like source and a bubble-like structure remains elusive.     

基于几何配准的多模式SAR影像配准及其误差分析

星载合成孔径雷达影像干涉处理时所需方位向配准精度因成像模式的差异而有所不同,目前在精密轨道条件下以几何配准为基础辅以影像信息的配准方案因其严格的理论模型和较高的精度成为干涉处理的首选。本文以TerraSAR-X影像为例,论证了不同成像模式影像所需的配准精度和卫星轨道精度,并通过理论分析和试验证明了精密轨道条件下,利用几何配准即可满足TerraSAR-X等卫星的条带模式影像干涉处理的需要;聚束模式影像需要在几何配准的基础上利用影像相干性或谱分集进一步优化配准结果。鉴于增强谱分集偏移量估计精度最高,本文进一步利用增强谱分集对比分析了不同轨道不同DEM条件下的几何配准误差。研究结果表明:卫星轨道切向误差是几何配准的主要误差源,目前常用3种DEM几何配准差异远小于0.001个像素,均可满足Sentinel-1影像干涉配准的需要。