素环上的一类非全局可导映射

设R是包含非平凡幂等元且有单位元的素环, Q={T∈R: T2=0}且δ: R→R是一个映射(无可加假设). 用代数分解方法证明了： 如果对任意的A,B∈R且［A,B］B∈Q, 有δ(AB)=δ(A)B+Aδ(B), 则δ是一个可加导子, 其中［A,B］=AB-BA为Lie积.     

具有条件（S）的关联BCK—代数的理想之若干等价条件

研究了具有条件（S）的关联BCK－代数理想的条件问题，得到了十余个等价命题。     

3-硝基-1,2,4-三唑酮-5(NTO)的铅盐[Pb(NTO)_2·H_2O]的晶体结构

3-硝基-1,2,4-三唑酮-5(NTO)的铅盐[Pb(NTO)_2·H_2O]的晶体结构已经测定.该晶体属单斜晶系,空间群为C_(2h)~5-P_(1/n)~2.晶胞参数:a=0.72589nm,b=1.21243nmc=1.22875nm,β=90.41°.结构测定表明,两个NTO五元环平面的二面角为82.42°,有一分子水参与配位,重原子铅的配位数为6。     

润滑脂及其添加剂剖析

本文主要介绍采用柱层析分离与红外光谱配合,对从美国进口的特种润滑脂进行剖析,使用渗析法将润滑脂中基础油抽提出,用柱色谱分离出润滑脂中抗氧剂等四种添加剂,并由红外光谱图获得其相应的结构范围,柱色谱洗脱剂通过寻找薄层包谱展开剂来选择,洗出液用薄层层析跟踪,按跟踪薄层结果,将柱层析收集相同的纯组分合并驱除溶剂作红外光谱分析。     

菲涅耳半波带法公式A_K=a_1/2±a_k/2中K值的范围

本文对在点光源照明情况下,用菲涅耳半波带法求考察点P合振幅的近似公式A_k=a_1/2±a_k/2中K值的适用范围进行了讨论,纠正了某些光学书籍中对K值范围加以限制的结论     

关于对外加剂与水泥适应性的分析

简要论述了混凝土外加剂与水泥的适应性及其影响因素和改善措施，可供混凝土试验员、混凝土生产与施工人员，以及工程管理、监理人员阅读参考。     

加法保幂等的注记

设R是一个含1的连通交换环,且R上每个幂等阵都相似于对角阵,Mn(R)表示环R上n×n矩阵全体.刻画了当2为R中的单位时,从M2(R)到Mm(R)(m=2,3)的保幂等加法映射形式.     

The Film-forming Properties of Propylene Carbonate (PC) on Graphite Anodes

1 Results Propylene carbonate (PC) is well known having a series of excellent properties including low melting point,wide liquid-phase range and wide electrochemical window.In addition,PC is well compatible with different cathode materials.However,the poor compatibility of PC with graphite anode limits the utilization of PC solvent into lithium ion batteries.It is generally accepted that PC molecules co-intercalate into graphite interlayer with solvated Li ions and cause exfoliation of graphite structur...     

Energetic particle radiations measured by particle detector on board CBERS-1 satellite

Using the data measured by energetic particle detector on board CBERS-01 and -02 for the past five years, statistics was made to show the general features of MeV electrons and protons along a solar synchronous orbit at an altitude of 780 km. This height is in the bottom region of the Earth's radiation belts. Detectors are inside the satellite cabinet and such continuous monitoring of particle radiation environment inside a satellite has seldom conducted so far. After a proper and careful treatment, it is indicated that the data inside satellite are well correlated with the radiation environment outside. Be-sides the agreement of the general distribution characteristics of energetic electrons and protons with similar observations from other satellites, attention is particularly paid to the disturbed conditions. Variations of particle fluxes are closely related with solar proton events, in general, electron fluxes of outer belt are well correlated with Dst index after three days' delay while the electron injection occurred almost at the same day during great magnetic storms. It is confirmed that both energetic electrons and protons appear in the Polar Cap region only after the solar proton events.     

Plasma sheet stretching accompanied by field aligned energetic ion fluxes observed by the NUADU instrument aboard TC-2

The NUADU (NeUtral Atom Detector Unit) instrument aboard TC-2 recorded 4л solid angle images of charged particles (E >180 keV) spiraling around the magnetic field lines in the near-Earth plasma sheet (at ~ -7 RE, equatorial dawn-to-night side) during a geomagnetic storm (Dst =-219 nT) on August 24, 2005. Energetic ion beam events characterized by symmetrical, ring-like, solid angle distributions around ambient magnetic field lines were observed during a 34-minute traversal of the plasma sheet by the TC-2 spacecraft. Also, observations during these multiple crossings of the plasma sheet were monitored by the magnetometer experiment (FGM) aboard the same spacecraft. During each crossing, a whistler-mode chorus enhancement was observed in the anisotropic area by the TC-2 low frequency electromagnetic wave detector (LFEW/TC-2) at a frequency just above that of the local lower hybrid wave. A comparison of the ion pitch angle distribution (PAD) map with the ambient magnetic field shows that an enhancement in the field aligned energetic ion flux was accompanied by tailward stretching of the magnetic field lines in the plasma sheet. In contrast, the perpendicular ion-flux enhancement was accompanied by a signature indicating the corresponding shrinkage of the magnetic field lines in the plasma sheet. Since both parallel ion-flux and perpendicular ion-flux enhancements occurred intermittently, the data were interpreted to imply a dynamical, oscillatory process of the magnetic field line (stretching and shrinking) in the near-Earth plasma sheet, which might have acted to help establish an interaction region in this area which would support continuous aurora-substorm triggering during the ongoing magnetic storm. The whistler-mode chorus may have been produced due to ion gyro-resonance during particle pitch angle diffusion after the plasma sheet compression.