甲醛对Nessler法和次氯酸酚盐法测定养殖水体总氨氮的影响

水体中含一定浓度的甲醛 ,用 Nessler法测得的总氨氮 (TAN)浓度远远高于实际浓度 ,差异百分数最高达 4 5 0 .0 6 % ;用次氯酸酚盐法测得的总氨氮 (TAN)浓度则明显低于实际浓度 ,差异百分数最高可达 84 .77%。甲醛浓度范围为 10～ 4 0 mg/ L、TAN浓度为 1～ 10 mg/ L,通过双因素有重复观察值的交叉实验 ,得到如下矫正式 :(1)用 Nessler法测 TAN时 ,Y=4 .0 5 2 9- 0 .0 72 4 x1+ 0 .2 0 6 4x2 ,标准误差为 1.3381;(2 )用次氯酸酚盐法测 TAN时 ,Y=0 .1196 + 0 .0 345 x1+ 1.0 0 2 2 x2 ,标准误差为 0 .4 6 2 7。 Y为 TAN实际浓度 (mg/ L) ,x1为甲醛浓度 (mg/ L) ,x2 为测得的 TAN浓度(mg/ L )。比较含氨氮水体与不含氨氮水体中的甲醛浓度 ,方差分析结果表明 ,没有显著差异。     

东海放射虫甘葡萄虫科的一新属及其两新种

1958-1961年在东海陆棚区进行放射虫的调查研究时,发现甘葡萄虫科(Glycobotrydidae)的一新属及其两新种。     

不同海域沉积物对尿素吸附的实验模拟研究

本文对采自渤海、黄海和东海3个典型海域的沉积物进行了尿素吸附/解吸的实验室模拟研究,用Freundlich吸附模型和Henry吸附模型分析了不同沉积物对尿素吸附的热力学特性,并研究了温度、沉积物粒径、有机质含量等因素对尿素在沉积物表面吸附的影响。结果表明,沉积物对尿素的吸附/解吸过程总体呈现3个阶段:快速吸附阶段（0~5 h）—慢速吸附阶段（5~12 h）—平衡阶段（12 h之后）。当水体中的尿素浓度较低时,沉积物解吸释放尿素,随着上覆水中尿素浓度逐渐增加,沉积物对上覆水中的尿素产生吸附行为,各海区沉积物对尿素的吸附能力由强至弱依次为渤海、东海、黄海,这可能与沉积物的类型有关。Freundlich方程和Henry方程均可模拟沉积物对尿素的吸附,温度、粒径以及沉积物中有机质含量等因素均对尿素在沉积物上的吸附产生影响,随着温度升高,尿素在沉积物上的吸附量变小,沉积物粒径越小,有机质含量越高,吸附尿素的能力越强,因此,揭示尿素在沉积物表面的环境行为时,必须考虑以上因素的影响。     

Compact and tunable mid-infrared source based on a 2 μm dual-wavelength KTiOPO4 intracavity optical parametric oscillator

Using a double resonant KTiOPO₄ (KTP) intracavity optical parametric oscillator operating at degenerated point of 2 μm, we demonstrate a unique mid-infrared source based on difference frequency generation in GaSe crystal. The output tuning range is 8.42-19.52 μm, and a peak power of 834 W for type-I phase matching scheme and 730 W for type-II phase matching scheme are achieved. Experimental results show that this oscillator is a good alternative to the generator of a compact and tabletop mid-infrared radiation with a widely tunable range.     

石笋氧同位素和微量元素记录的陕南地区4200～2000a B.P.高分辨率季风降雨变化

基于陕南祥龙洞石笋XL2的19个230Th年龄、218个氧同位素分析以及896个Sr/Ca分析数据,高分辨率重建了4200～1972a B.P.期间陕南地区季风降雨变化.重建结果显示陕南地区这一时期季风降雨有显著的127～105a和57a周期,可能分别受控于太阳活动、PDO和/或AMO的变化.重建时段有3次百年尺度的干旱事件,分别发生于2200～2100a B.P.,2900～2700a B.P.和3600～3400a B.P.,其中2900～2700a B.P.干旱事件对应于北大西洋地区2.8ka冷事件.对比研究显示,尽管祥龙洞石笋和董哥洞石笋δ18O记录整体一致,但除了2900～ 2700aB.P.干旱事件之外,其他两次干旱事件在董哥洞石笋记录中并不明显.而尽管总体上祥龙洞和和尚洞石笋δ18O记录的差异要大,但XL2的3次干旱事件在和尚洞记录都有明显体现.有精确年代控制的祥龙洞、董哥洞及和尚洞石笋氧同位素记录的差异,揭示晚全新世我国季风降雨在十一百年尺度存在区域差异.     

Origin and evolution of oilfield brines from Tertiary strata in western Qaidam Basin: Constraints from <Superscript>87</Superscript>Sr/<Superscript>86</Superscript>Sr, δD, δ<Superscript>18</Superscript>O, δ<Superscript>34</Superscript>S and water chemistry

Chemistry of major and minor elements, ⁸⁷Sr/⁸⁶Sr, δD, δ¹⁸O and δ³⁴S of brines were measured from Tertiary strata and Quaternary salt lakes in the western Qaidam Basin. The water chemistry data show that all oilfield brines are CaCl₂ type. They were enriched in Ca²⁺, B³⁺, Li⁺, Sr²⁺, Br⁻, and were depleted in Mg²⁺, SO₄ ²⁻, which indicated that these brines had the characteristics of deeply circulated water. The relationship between δD and δ¹⁸O shows that all data of these brines decline towards the Global Meteoric Water Line (GWL) and Qaidam Meteoric Water Line (QWL), and that the intersection between oilfield brines and Meteoric Water Lines was close to the local spring and fresh water in the piedmont in the western Qaidam Basin. The results suggest that oilfield brines has initially originated from meteoric water, and then might be affected by water-rock metamorphose, because most oilfield brines distribute in the range of metamorphosing water. The ⁸⁷Sr/⁸⁶Sr values of most oilfield brines range from 0.71121 to 0.71194, and was less than that in salt lake water (>0.712), but close to that of halite in the study area. These imply that salt dissolution occurred in the process of migration. In addition, all oilfield brines have obviously much positive δ³⁴S values (ranging from 26.46‰ to 54.57‰) than that of salt lake brines, which was caused by bacterial sulfate reduction resulting in positive shift of δ³⁴S value and depleteed SO₄ ²⁻ in oilfield brines. Combined with water chemical data and δD, δ¹⁸O, ⁸⁷Sr/⁸⁶Sr, δ³⁴S values, we concluded that oilfield brines mainly originate from the deeply circulated meteoric waters, and then are affected by salt dissolution, water-rock metamorphose, sulfate reduction and dolomitization during the process of migration. These processes alter the chemical compositions of oilfield brines and accumulate rich elements (such as B, Li, Sr, Br, K and so on) for sustainable utilization of salt lake resources in the Qaidam Basin.     

文登市天福国土资源所全面加强基层队伍建设

天福国土资源所,前身文城土地管理所,2001年机构改革时,成为文登市国土资源局在天福路街道办事处的派出机构,现有干部职工4人。近年来,在文登市国土资源局和天福路街道办事处的正确领导和大力支持下,该所坚持以人为本抓素质,健全制度抓规范,廉洁勤政抓服务,全面加强队伍建设,有力地促进了国土资源事业发展。建所以来,年年被评为局先进集体,连续3年在办事处的行风建设民主评议活动中名列第一。     

信风驱动的中国季风区石笋δ18O与大尺度温度场负耦合——从年代际变率到岁差周期的环流效应纪念GNIP建网50周年暨葫芦洞石笋末次冰期记录发表10周年

中国季风区很多单点石笋氧同位素记录与集成的大区域温度场在长时间尺度上呈负耦合变化模式.通过理论计算和观测记录校准分析,温度效应和雨量效应均不能加以解释.从环流效应角度分析,发现信风张弛既控制了中国季风区石笋δ18O的主要变化趋势,也决定了西太平洋暖池的温度高低和面积大小,而后者在很大程度上影响着全球温度的走向,因此可确认,二者的负耦合是信风决定的“一因二果”.进而分析了中国季风区石笋δ18O短尺度环流效应响应于ENSO循环的机理,并在此基础上,借助模式结果,将环流效应概念推广到轨道尺度,由此获得中国季风区石笋δ18O序列缺失偏心率周期等问题的初步解答.     

Differential rotation of some HK-Project stars and the butterfly diagrams

We analyze the long-term variability of the chromospheric radiation of 20 stars monitored in the course of the HK-Project at the Mount Wilson Observatory. We apply the modified wavelet algorithm for this set of gapped time series. Besides the mean rotational periods for all these stars, we find reliable changes of the rotational periods from year to year for a few stars. Epochs of slower rotation occur when the activity level of the star is high, and the relationship repeats again during the next maximum of an activity cycle. Such an effect is traced in two stars with activity cycles that are not perfectly regular (but labeled “Good” under the classification in [Baliunas, S.L., Donahue, R.A., Soon, W.H., Horne, J.H., Frazer, J., Woodard-Eklund, L., Bradford, M., Rao, L.M., Wilson, O.C., Zhang, Q. et al., 1995. ApJ 438, 269.]) but the two stars have mean activity levels exceed that of the Sun. The averaged rotational period of HD 115404 is 18.5 days but sometimes the period increases up to 21.5 days. The sign of the differential rotation is the same as the Sun’s, and the value ΔΩ/Ω=-0.14. For the star HD 149661, this ratio is −0.074. Characteristic changes of rotational periods occur over around three years when the amplitude of the rotational modulation is large. These changes can be transformed into latitude-time butterfly diagrams with minimal a priori assumptions. We compare these results with those for the Sun as a star and conclude that epochs when surface inhomogeneities rotate slower are synchronous with the reversal of the global magnetic dipole.     

阿克苏初秋一次暴雨过程诊断分析

本文利用常规地面与高空观测资料、自动站逐时资料、NECP1°×1°再分析资料,对阿克苏地区2015年9月7日局地暴雨进行分析。结果表明,造成此次暴雨的主要原因有(1)中尺度分析暴雨发生前阿克苏处于高能高湿不稳定区域;(2)08时至20时探空图中湿层、风向以及不稳定能量的突变预示了强对流天气的发生;(3)暴雨过程的大部分水汽是通过低层偏东气流输送,水汽的来源主要为孟加拉湾,其次北疆短波槽及蒙古槽也提供了少量水汽(4)锋区加强、垂直风切变增大、水平风速辐合提供了热力及动力条件,垂直速度伸展高度影响了对流云厚度及高度。(5)地面风速辐合触发对流,加之较好的地面热力条件以及一定的地形增益暴雨强度。(6)地面辐合线及偏东风输送位置影响暴雨落区。