蒙脱石中性化改性实验研究

使用表面活性剂HDTMAB对含有蒙脱石等粘土矿物的膨润土进行不同程度的有机改性,并利用自由膨胀率的实验方法定量描述改性膨润土在水以及甲苯介质中的膨胀规律。对实验结果进行数学分析后发现,随着改性剂用量的加大,改性膨润土在水介质中的自由膨胀率明显降低,而在甲苯介质中的自由膨胀率显著上升,当改性剂用量约为15%时,改性膨润土在水以及甲苯介质中都没有发生剧烈膨胀。依照上述膨润土的改性方法,对胜利油田提供的岩心样品进行了有机改性,并得到了相同的规律。由此得出,严格控制改性剂用量可以实现蒙脱石的中性化改性。利用这一规律,将适量的改性剂注入地下,既能够缓解油气田储层中蒙脱石的水敏膨胀危害,又不会造成过量的油脂分子吸附于矿物表面。     

南沙群岛海域近海面粗糙度、中性曳力系数及总体交换系数研究

根据 1 994年 9月 1 8— 30日南沙群岛海域渚碧礁的近海面大气湍流观测实验资料 ,分别计算了该海域光滑海面和粗糙海面上的空气动力粗糙度 (z0 )、中性曳力系数 (CDN)。利用Brutsaert的假定 ,推导了一组求取标量粗糙度 (zT,zQ)、整体输送系数 (感热交换系数CHN、水汽交换系数CEN)的公式。在此基础上分别计算和分析了该海域近海面光滑海面和粗糙海面上z0 ,zT,zQ,CDN,CHN,CEN 及它们关于水平风速u分量的分布 ,并得到了一些有意义的结论。     

The influences of environmental factors on the air-sea coupling coefficient

The response relationship between equivalent neutral wind speed anomaly(ENWSA) and sea-air temperature difference anomaly(SATDA) has been analyzed over four typical sea regions, i.e., the Kuroshio Extension, the Gulf Stream, the Brazil-Malvinas Confluence and the Agulhas Return Current. The results show that ENWSA is more sensitive to SATDA than sea surface temperature anomaly(SSTA), which implies that SATDA seems to be a more suitable parameter than SSTA to analyze the mesoscale air-sea interac...     

不同类型糖源对大菱鲆脂肪代谢酶活性和脂肪酸组成的影响

以初始体质量(8.77±0.16)g的大菱鲆(Scophthalmus maximus)幼鱼为研究对象,在室内流水系统中进行9周的养殖实验,比较分析饲料中3种不同类型的糖源(葡萄糖、蔗糖和糊精)对大菱鲆脂肪代谢相关酶活性和肌肉脂肪酸组成的影响。结果表明,不同类型的糖源显著影响肝脏中与脂肪合成相关的葡萄糖-6-磷酸脱氢酶(G6PD)和苹果酸酶(ME)的活性(P0.05)。饲料糖源为葡萄糖时,大菱鲆肝脏中G6PD和ME的活性显著高于其他处理组,而蔗糖和糊精处理组之间没有显著差异。对与脂肪分解代谢相关酶的活性分析表明,肠道脂肪酶的活性受饲料中不同糖源的影响显著(P0.05);肝脏脂蛋白脂酶的活性在糖源为葡萄糖时显著低于其他处理组(P0.05);不同糖源对肝脂酶的活性无显著影响(P0.05);糊精组的总脂酶活性显著高于葡萄糖组(P0.05)。葡萄糖组大菱鲆肌肉中的C16∶0和C18∶0的含量显著高于糊精组,而C16∶1和C18∶1n-9的含量显著低于糊精组(P0.05)。研究表明,饲料中不同类型的糖源对大菱鲆肌肉脂肪酸的影响集中在饱和脂肪酸和单不饱和脂肪酸上,而对多不饱和脂肪酸的影响有限。     

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具非线性扩散系数的中立抛物型方程的振动结果

研究一类具非线性扩散系数的中立抛物型方程的振动性,利用Green定理和时滞微分不等式,获得了该类方程在Robin边值条件下所有解振动的若干充分性判据。结论充分表明振动是由时滞量引起的。     

Hemispheric Imaging of Galactic Neutral Hydrogen with a Phased Array Antenna System

The thousand element array (THEA) system is a phased array system consisting of 1 m² tiles having 64 Vivaldi elements each, arranged on a regular 8-by-8 grid, which has been developed as a demonstrator of technology and applicability for SKA. In this paper we present imaging results of Galactic neutral hydrogen with THEA. Measurements have been taken using a dense 2-by-2 array of four tiles as a four tile adder. The results are compared with results from the Leiden-Dwingeloo Survey, showing qualitative agreement, but also indicating that further studies are needed on the instrumental characteristics.     

米曲霉中性蛋白酶特性的研究

研究了米曲霉中性蛋白酶的特性。结果表明，米曲霉中性蛋白酶的最佳提取方法为加入pH7．2的缓冲液研匀，置恒温（30℃）培养箱中提取30min．每10min搅动1次，最后用4层纱布过滤。酶反应最适温度为55℃，最适pH值为7．2。NaCl和EDTA对其有一定的抑制作用。酶的热稳定性好．在45℃的温度下处理24h后，酶活力仍有45．5％。米曲霉中性蛋白酶与培养物一起保存时，稳定性也较好，在4℃保存一个月后，酶活力几乎无变化。     

Low energy neutral atoms imaging of the Moon

Imaging of low-energy neutral atoms (LENAs) in the vicinity of the Moon can provide wide knowledge of the Moon from the viewpoint of plasma physics and planetary physics. At the surface of the Moon, neutral atoms are mainly generated by photon-stimulated desorption, micrometeorite vaporization and sputtering by solar wind protons. LENAs, the energetic neutral atoms with energy range of 10-500 eV, are mainly created by sputtering of solar wind particles. We have made quantitative estimates of sputtered LENAs from the Moon surface. The results indicate that LENAs can be detected by a realistic instrument and that the measurement will provide the global element maps of sputtered particles, which substantially reflect the surface composition, and the magnetic anomalies. We have also found that LENAs around dark regions, such as the permanent shadow inside craters in the pole region, can be imaged. This is because the solar wind ions can penetrate shaded regions due to their finite gyro-radius and the pressure gradient between the solar wind and the wake region. LENAs also extend our knowledge about the magnetic anomalies and associated mini-magnetosphere systems, which are the smallest magnetospheres as far as one knows. It is thought that no LENAs are generated from mini-magnetosphere regions because no solar wind may penetrate inside them. Imaging such void areas of LENAs will provide another map of lunar magnetic anomalies.