大气中痕量有机胺测量方法的研究进展

作为大气中最重要的含氮有机化合物,有机胺易与硫酸、硝酸气体生成胺盐,促进新颗粒的形成,同时也可与臭氧、OH自由基、NO₃自由基发生氧化反应,是二次气溶胶的前体物.综述了国内外关于大气有机胺检测技术的研究进展,对常规的离线检测技术和在线质谱技术进行了介绍和对比,重点介绍了质谱法工作原理以及测定大气有机胺的优越性,并对其未来发展进行了展望.     

低高度角大气静力学延迟修正的改进

进行低高度角观测是GPS(Global Positioning System)气象学的发展趋势,其中发展高精度的低高度角的大气静力学延迟修正是主要的关键技术.比较了3种计算无线电波从空间到地面接收机的大气静力学延迟修正方法:(1)在大气球对称假设下用探空气球资料路径积分得到大气静力学延迟;(2)在大气球对称假设下用NCEP(National Centers for Environmental Prediction)再分析资料得到大气静力学延迟;(3)用Niell的大气静力学映射函数得到大气静力学延迟.与2001年中国地区89个探空气球站资料计算得到的大气静力学映射函数比较结果显示:NCEP再分析资料路径积分的方法在低高度角(5°以下)的精度好于Niell映射函数模型约5倍.     

The evolution of the z distribution of normal neutron stars in the Galaxy

Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Linear stability for some symmetric periodic simultaneous binary collision orbits in the four-body problem

We apply the analytic-numerical method of Roberts to determine the linear stability of time-reversible periodic simultaneous binary collision orbits in the symmetric collinear four-body problem with masses 1, m, m, 1, and also in a symmetric planar four-body problem with equal masses. In both problems, the assumed symmetries reduce the determination of linear stability to the numerical computation of a single real number. For the collinear problem, this verifies the earlier numerical results of Sweatman for linear stability with respect to collinear and symmetric perturbations.     

Primordial non-Gaussianity from LAMOST surveys

The primordial non-Gaussianity (PNG) in the matter density perturbation is a very powerful probe of the physics of the very early Universe. The local PNG can induce a distinct scale-dependent bias on the large scale structure distribution of galaxies and quasars, which could be used for constraining it. We study the detection limits of PNG from the surveys of the LAMOST telescope. The cases of the main galaxy survey, the luminous red galaxy (LRG) survey, and the quasar survey of dif- ferent magnitude limits...     

可口革囊星虫(Phascolosoma esculenta)铁结合

以克隆获得的可口革囊星虫(Phasolosma esculenta)、枝吻纽虫(Dendrorhynchus zhejiangensis)、泥蚶(Tegillarca granosa)、缢蛏(Sinonovacula constricta)、仿刺参(Apostichopus japonicus)和白肛海地瓜(Acaudina leucoprocta)6种无脊椎动物的铁结合蛋白基因为基础, 通过NCBI检索下载相应的氨基酸序列, 采用SingalP程序查找信号肽, 用TMHMM程序搜寻预测跨膜区, 采用Clustal W程序多序列比对, 构建进化树。对其编码蛋白的信号肽、跨膜区以及磷酸化位点等进行分析。结果表明, 6种动物的铁结合蛋白都没有信号肽, 也无跨膜区, 不可能是膜上的受体或定位于膜上, 均为胞外蛋白。泥蚶的ferritin有4个磷酸化位点, 仿刺参ferritin有10个, 枝吻纽虫有8个, 白肛海地瓜有9个, 可口革囊星虫和缢蛏的ferritin未搜寻到磷酸化位点。6种铁结合蛋白的疏水性有一定的差异, 最大值在1.0—1.6之间, 最小值在?3.3—?2.8之间。可口革囊星虫和仿刺参的铁结合区域特征序列完全相同, 与文昌鱼、缢蛏、泥蚶、牡蛎、盘鲍有2个氨基酸差异, 与人、小家鼠和叉尾有1个氨基酸差异。     

锦州湾沉积物重金属污染特征及基于三角模糊数的生态风险评价

在锦州湾海域采集了20个表层沉积物样品, 测定Pb、Cr、Zn、Cu、As、Hg等6种重金属含量。数据分析表明Hg变差系数最大, 存在较重的污染。区域分布特征分析表明, 除了重金属Cr外, 其他五种重金属元素在沉积物中的含量均具有明显的由近岸向远岸逐渐降低的趋势, 说明陆源输入可能是锦州湾重金属污染的主要原因。通过聚类分析, 将研究海域分成三个区域, 采用三角模糊数处理和表征重金属含量, 对其进行生态风险评价(取可信度A=0.90), 结果表明重金属污染顺序是: Hg>Zn>Cu>Pb>As>Cr, 其中Hg和Zn在三个区都达到高污染程度。由于Hg极高的生物毒性, 使得该海域的生态风险都达到了极高的水平。     

绿鳍马面鲀(Navodon septentrionalis)CYP19a基因克隆与表达特征分析

利用简并引物扩增及RACE全长克隆技术, 克隆得到绿鳍马面鲀(Navodon septentrionalis)CYP19a基因cDNA全长序列。通过多序列比对, 发现具有芳香化酶特定保守序列, 包括一个I-螺旋区, 一个Ozol肽区, 一个亚铁血红素结合区域以及一个芳香化酶特异性结合区域。通过RT-PCR技术检测了其在绿鳍马面鲀成鱼各组织表达的情况, 发现其CYP19a基因只在卵巢中有表达; 同时也分析了其在不同卵巢发育期的表达情况, 发现CYP19a在卵黄发生后期表达量达到最高值, 卵巢退化吸收期表达量达到最低值。     

The improvement of the one-dimensional Mellor-Yamada and K-profile parameterization turbulence schemes with the non-breaking surface wave-induced verticalmixing

Both the level 2.5 Mellor-Yamada turbulence closure scheme(MY) and K-profile parameterization(KPP) are popularly used by the ocean modeling community.The MY and the KPP are improved through including the non-breaking surface wave-induced vertical mixing(Bv),and the improved schemes were tested by using continuous data at the Papa ocean weather station(OWS) during 1961–1965.The numerical results showed that the Bv can make the temperature simulations fit much better with the continuous data from Papa Station.The two improved schemes overcame the shortcomings of predicting too shallow upper mixed layer depth and consequently overheated sea surface temperature during summertime,which are in fact common problems for all turbulence closure models.Statistical analysis showed that the Bv effectively reduced the mean absolute error and root mean square error of the upper layer temperature and increased the correlation coefficient between simulation and the observation.Furthermore,the performance of vertical mixing induced by shear instability and the Bv is also compared.Both the temperature structure and its seasonal cycle significantly improved by including the Bv,regardless of whether shear instability was included or not,especially for the KPP mixing scheme,which suggested that Bv played a dominant role in the upper ocean where the mean current was relatively weak,such as at Papa Station.These results may provide a clue to improve ocean circulation models.