不同碳氮比对辽河口湿地总氮去除的影响

于2010年5月～10月采用现场模拟培养法探讨了辽河口芦苇湿地沉积物中的总氮去除效果,并分析了不同梯度C/N比(5∶1、10∶1、15∶1)对沉积物中总氮去除效果的影响。结果表明:在自然状态下,有植被芦苇湿地总氮去除率比无植被湿地高;当施加C/N因素后可以提高沉积物中总氮去除率,C/N比对裸滩湿地中氮的去除效果比芦苇湿地明显;在有植被芦苇湿地中C/N比为10时总氮去除率最高,而在无植被湿地中C/N比值为15时总氮去除率最高;8月份各实验组中总氮去除率最高。影响辽河口湿地沉积物脱氮效果主要环境因子还有温度、盐度、含水率和pH等。     

半叶马尾藻多糖的一般生殖毒性

交配前雄性大鼠分别按每 kg 体质量1.25、2.50、5.00 g 的剂量灌服半叶马尾藻多糖,连续灌胃60 d,雌性大鼠分别以相同剂量连续灌胃14 d,以雄雌1∶1的比例合笼5 d,每天做阴道分泌物涂片检查,见精子者记为妊娠第1天,交配后雄鼠处死,测定血清睾酮(T)水平,取雄鼠附睾进行精子成活率、精子计数和精子畸形率测定,计算睾丸、附睾脏器比,并进行病理组织学检查;雌鼠继续灌胃至妊娠7 d,于妊娠14 d 处死,计算受孕率、着床数、黄体数、死胎、活胎和吸收胎,测定血清促卵泡生成素(FSH)、黄体生成素(LH)和雌二醇(E2)水平,计算脏器比并进行病理组织学检查.结果显示,给药组大鼠的精子成活率、精子计数、精子畸形率、受孕率、着床数、黄体数、死胎、活胎、吸收胎、睾丸、附睾和卵巢脏器比以及血清 T、FSH、LH 和 E2水平与对照组相比差异无统计学意义(P >0.05),生殖器官病理组织学检查未见明显异常.在本实验条件下,半叶马尾藻多糖对大鼠无明显生殖毒性     

甲烷水合物CO2置换开采研究现状与展望

天然气水合物广泛存在于海底沉积物和大陆永冻区,是一种潜在的能源资源。CO2置换法开采天然气水合物,不仅可以从水合物藏中开采出天然气,还能够使空气中的CO2以水合物的形式长期埋存于地下。本文从可行性、微观机理及影响因素等方面,总结了甲烷水合物CO2置换法开采的研究现状,论述了目前研究中存在的问题及不足,并对以后的研究工作提出了一些展望和建议。     

新丰江中心地震台日常数据处理软件

根据新丰江中心地震台实际业务工作的需要,在Visual C++6.0平台上,使用ActiveX Data Objects(ADO)技术,通过客户/服务器(C/S)模式访问MySQL数据库表,并基于MFC(微软基本类库,Microsoft Foundation Classes)的OLE(对象链接嵌入,Object Linking and Embedding)编程方法操作EXCEL报表文件,开发出一套地震数据处理软件,完成台站日常数据的录入、查询、修改、转换和报表输出等工作,实现地震台站的无纸化、网络化办公,提高工作效率。     

基于ArcGIS的地震烈度图快速生成技术研究与实现

利用C#程序,实现现场烈度调查信息的录入。根据录入的离散点源信息,通过ArcGIS的分析功能,绘制出地震烈度分布图。     

Orbits of Comets C/1845 L1 (Great June Comet) and C/1846 D1 (de Vico)

Orbits are calculated for Comet C/1845 L1 (the Great June Comet) and C/1846 D1 (de Vico), the former based on 157 observations in right ascension and 152 in declination and the latter on 10 and 9, respectively. Both orbits are hyperbolic and statistically distinguishable from parabolas. Statistical tests indicate that the residuals are random and thus the orbits satisfactory. The Great June Comet is in no way associated with the comet Tycho Brahe observed in 1596 (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

CCD and photon-counting photometric observations of asteroids carried out at Padova and Catania observatories

We present the results of observational campaigns of asteroids performed at Asiago Station of Padova Astronomical Observatory and at M.G. Fracastoro Station of Catania Astrophysical Observatory, as part of the large research programme on Solar System minor bodies undertaken since 1979 at the Physics and Astronomy Department of Catania University. Photometric observations of six Main-Belt asteroids (27 Euterpe, 173 Ino, 182 Elsa, 539 Pamina, 849 Ara, and 984 Gretia), one Hungaria (1727 Mette), and two Near-Earth Objects (3199 Nefertiti and 2004 UE) are reported. The first determination of the synodic rotational period of 2004 UE was obtained. For 182 Elsa and 1727 Mette the derived synodic period of 80.23±0.08 and , respectively, represents a significant improvement on the previously published values. For 182 Elsa the first determination of the H-G magnitude relation is also presented.     

Comparison of the X-ray and optical variabilities in the Seyfert galaxy 3C 120

Based on our UBV RI observations and X-ray data from the RXTE satellite, we have investigated the variability of the galaxy 3C 120 over the period 1996–2008. The relative variability amplitude in the U and B bands without any subtraction of the contribution from the underlying galaxy is 23 and 22%, respectively, against 21% in the X-ray band. The autocorrelation function based on the B-band data is considerably wider than that based on the X-ray data. The structure functions on a time scale from 1 to ～100–300 days in the X-ray and optical spectral ranges have the form of a power law (SF ～ τ ^b ). However, their indices differ significantly: b = 0.42 in the X-ray band and b = 1.36 in the B band. Considering the X-ray and optical variabilities as a superposition of independent flares in a wide range of durations, we may conclude that the amplitudes of short flares in the X-ray band are higher than those in the optical one and, conversely, the relative amplitudes of long flares in the X-ray band are slightly lower than those in the optical one, i.e., short events dominate in the X-ray band. The optical flux variations in the R _c and I _c bands lag significantly behind those in the B band, by 3.9 _?0.7 ^+1.0 and 6.2 _?0.6 ^+1.1 days, respectively, if the lag is estimated from the centroid of the cross-correlation function. The X-ray variability on a time scale of about 1800 days (～5 yr) lags behind the B-band variations by 5.3 _?3.3 ^+2.7 days, but the confidence level of this estimate is only 87%. A more detailed analysis of the correlation between the X-ray and optical emissions has revealed a fairly complex picture: different degrees of correlation between the optical and X-ray fluxes are observed at different times.     

C.T.R. Wilson versus G.C. Simpson: Fifty years of controversy in atmospheric electricity

Two British scientists, G.C. Simpson and C.T.R. Wilson, held contrasting views on the electrical polarity of thunderclouds for nearly half of the 20th century. Simpson's perspective was dominated by the measured charge on rain, by the breaking drop theory for the charging of raindrops, and later, by the branching behavior of lightning flashes. Wilson's view was dominated by his work on the field changes accompanying lightning, by his knowledge of the corona current from the ground beneath electrified clouds, and ultimately by his unifying global circuit hypothesis, requiring a source current to maintain a negatively charged Earth against dissipation. Simpson's observed tripole structure of thunderclouds provided partial resolution to the controversy, but the main positive dipole supported Wilson's view, which survives today.