高糖化力根霉的分离及其制作“全曲清酒”的研究

采用直接分离法、稀释法和毛细管分离法等方法,从酒药和大曲中分离得到了几株高糖化力的根霉纯培养,并应用于“全曲清酒”的制作;用富含淀粉的甘薯为原料,可省略通常采用的复杂的“发酵”工艺过程,从而降低了成本,可在乡镇企业推广生产     

A Least-squares Approach to Depth Determination from Numerical Horizontal Self-potential Gradients

We have developed a least-squares minimization approach to depth determination of a buried ore deposit from numerical horizontal gradients obtained from self-potential (SP) data using filters of successive window lengths (graticule spacings). The problem of depth determination from SP gradients has been transformed into the problem of finding a solution to a nonlinear equation of the form f(z)=0. Formulas have been derived for vertical and horizontal cylinders and spheres. Procedures are also formulated to estimate the electrical dipole moment and the polarization angle. The method is applied to synthetic data with and without random noise. Finally, the validity of the method is tested on two field examples. In both cases, the depth obtained is found to be in a very good agreement with that obtained from drilling information.     

基于SPE与SPATT的水体中麻痹性贝类毒素检测方法构建与应用

为实现麻痹性贝类毒素(paralytic shellfish poisoning,PSP)的实时监控与提前预警,本研究构建了基于固相萃取技术(solid phase extraction,SPE)与固相吸附毒素跟踪技术(solid phase adsorption toxin tracking,SPATT)的水体中PSP检测方法,重点优化了吸附材料及前处理方法,评价了回收率、检出限等指标,并将方法应用于2019年春季秦皇岛山海关海域PSP消长过程的监测中,比较评估了两种方法的监控预警效果。结果表明:SPE方法选用ENVI-Carb 500mg/6mL固相萃取柱,过样体积为50mL,13种PSP组分的平均回收率为82.2%±10.0%、检出限为4.0-20.0ng/L;SPATT方法选用SP207大孔吸附树脂,洗脱时间为静置Id最佳,整体回收率约为9.2%;在实际应用中,结合产毒藻密度及贻贝富集毒素含量的变化,发现SPE方法的检测结果可实时表征海域PSP风险状况,对于贻贝中PSP的预警效果也显著优于SAPTT方法,后者不仅因监控方式相对滞后一个监测周期,且灵敏度及准确性均较差。对于秦皇岛海域,当SPE方法检测结果达到100ng STX eq/L时,该海域贻贝中PSP残留将具有潜在的食用安全风险,跟踪过程表明这一阈值可提前两周预警贻贝富集毒素含量超出我国限量标准(800μg STX eq/kg),这对于强化风险警示并制定防范措施具有积极作用。     

SP anomaly over doable line of poles-interpretation through log curves

In the analysis and interpretation ofsp anomalies, two-dimensional finite sheet models are equated to the double line of poles. The profiles over such a model being asymmetric with a minor positive peak and a major negative peak, a double logarithmic curve matching technique simpler than that of Meiser is suggested in the paper for easy and unique solution for all values of depth, dip and length. This technique along with a few others have been tested on two profiles across the sulphide deposit from the Rakha Mines, Singhbhum copper belt, India.     

The main structure and tectonic features of the Chernorud-Mukhor site on the western shore of Lake Baikal from TEM and SP measurements

Transient electromagnetic (TEM), self-potential (SP) and geoelectrical mapping measurements were carried out at the Chernorud-Mukhor site in the Priolkhonje area on the western shore of the Lake Baikal. All measurements were made along several profiles across the main strike of the regional Primorsky fault. TEM measurements were carried out in a time range from a few tens of microseconds to several tens of milliseconds. The most important result of the 1D modelling of TEM soundings is the discovery of nearly horizontal boundaries that divide high resistive overlying and well conducting underlying rocks. The resistivity of the former is in the range from 100 Ωm to 1000 Ωm, while the resistivity of the latter varies from less than 1 Ωm to several tens of Ωm. This good conductive zone could also be verified by geoelectrical mapping using Schlumberger array (AB/2=100 m). Due to high conductivity of the underlying rocks only the upper boundary of the conductive layer could be determined by TEM soundings. A regional SP anomaly with amplitude of about −450 mV has also been observed above the low resistivity zone indicating the electron nature of its conductance. Geologically, the conductive zone is represented by a graphite-bearing layer within the region of archean rocks. Since that layer extends over a large area, it may be used as a key in studying structures and tectonics of the Priolkhonje area. A 1D TEM geoelectric section shows a wide, gently sloping syncline as a probable base structure of the Chernorud-Mukhor site. Neotectonic faults divide the syncline into vertically displaced blocks that form a wide complicated graben with a total amplitude of about 250 m.     

卫星激光测距的电控系统设计与实现

给出的卫星激光测距的二轴系统实现了通过软件控制望远镜coude光路调整、接收系统SPAD和APD的自动切换、视场光阑大小的自动调节、以及发射光束指向的精确控制。该系统是基于MPC07运动控制卡,通过人机交互界面进行实时控制,旨在实现不同功能的调节,提高卫星激光测距的自动化程度。详细介绍了该系统的硬件组成、技术指标及软件工作方式。     

东天山星星峡缝合带早古生代强过铝质花岗岩的研究及其地质意义

铅炉子过铝质花岗岩带发育于中天山岛弧带南缘的星星峡缝合带内,为一长条形的二云母花岗岩。岩体地球化学特征是高Si、Al和K,低Mg、Fe的组份,全碱含量中等,σ=1.74～1.9,K_2ONa_2O,A/CNK1.1,属于高钾钙碱性过铝质花岗岩类(SP)。岩体的CaO/Na_2O和Al_2O_3/TiO_2比值都相对较低,分别为(0.06～0.07)和(48.9～55.3);REE、Nb、Y含量和Rb/Sr、Rb/Ba比值相对较高;Rb、Th和LREE相对富集,Ba、Si、Eu、Ti、P和HREE相对亏损;ε_(HF)(t)=-2.3～+1.6表明岩体还具有较高的锆石同位素特征,T_(2DM)变化范围为1573～1329 Ma。这些地质学和地球化学研究表明铅炉子二云母花岗岩形成于后碰撞的伸展环境中,是在高温、中低压条件下发生重熔形成的,其源岩为古老的地壳物质和年轻的增生物质通过物理风化作用形成泥质岩。本文通过测年获得二云母花岗岩锆石LA-ICPMS年龄为444.5±2.2 Ma,表明铅炉子过铝质花岗岩形成于晚奥陶世,是中天山岛弧带和公婆泉岛弧带的碰撞时间的上限,它也是中天山岛弧带与公婆泉岛弧带碰撞造山作用的产物,是中亚增生造山带的增生方式之一。     

日本鬼鲉蜇伤与P物质和生长抑素的关系及其粗毒对免疫细胞活性影响

１９９７年６月在山东省日照市岚山头附近海域收集日本鬼ｙｏｕ,采用放射凤学方法检测了注射毒腺粗提物大鼠局部肌肉组织、血浆、疹髓、延髓、中脑、下丘脑及免疫器官内Ｐ物质和生长抑素含量变化;用ＭＴＴ法检测了朱粗提物在整体和离体条件下对免疫细胞活性的影响;用生化方法检测了毒腺组织中透明质酸酶活性。结果表明,与对照组大鼠相比,实验组大鼠局部肌肉及延髓、中脑、胸腺中脾脏中Ｐ物质含量增加,而下丘脑中Ｐ物质含量下降     

Doppler-Zeeman mapping of the rapidly rotating magnetic CP star HD 37776

We present the results of our analysis of magnetic-field configuration and abundance anomalies on the surface of the rapidly rotating, chemically peculiar helium-strong variable B2 V star HD 37776 with unresolved Zeeman components of spectral lines. Simultaneous inversion of the observed Stokes I and V profiles, which realizes the method of Doppler-Zeeman mapping [1], has been applied for the first time. Spectroscopic observations were carried out with the Main stellar spectrograph of the 6-m Special Astrophysical Observatory telescope equipped with a Zeeman analyzer and a CCD array, which allowed spectra in right-and left-hand circularly polarized light to be taken simultaneously at a signal-to-noise ratio S/N≥200 [2]. The profile width of winged spectral lines (reaching 5 Å) is determined by Zeeman line splitting; however, the observed Zeeman components are blurred and unresolved because of the rapid stellar rotation. When solving the inverse problem, we sought for the magnetic-field configuration in the form of a combination of arbitrarily oriented dipole, quadrupole, and octupole placed at the stellar center. The observed Stokes I and V profiles for eight spectral lines of He, O II, Al III, Si III, and Fe III averaged over the visible stellar surface were used as input data. We constructed a model of the magnetic field from the condition of coincidence of magnetic maps obtained from different lines of different chemical elements and from the condition of a minimum profile residual. This model is a combination of centered coaxial dipole and quadrupole with the dominant quadrupole component at 30°<i<50°, β=40°, and a maximum surface field strength H _s=60 kG. A comparison of our abundance maps with the field configuration shows that the He concentration is at a maximum in the regions of maximum radial field, while the maximum concentrations of O, Al, Si, and Fe coincide with the regions of maximum tangential field.