高职学校教学质量保障系统与教学评价体系研究

本文通过对教学质量的再认识,分析了当前影响高校教学质量的因素,构建了高校教学质量保障系统,制定了高职教学评价指标体系。     

功率超声换能器应用与设计

本文主要介绍了功率超声在工业方面的应用，并介绍了清洗用功率超声换能器的设计，详细阐述了其结构特点、振动方程、振速分布及应力分布等。     

The shuttle development and its growth potential

During the next two decades, we will establish the foundation for the 21st century's accomplishments in space. The Space Shuttle vehicle will become the cornerstone for that foundation by providing economical opportunities for space exploration and utilization.Reusability of the Shuttle vehicle is the key to its economy. The major developmental challenges encountered in the Shuttle program are typified by the complexities involved in designing the reusable propulsion and thermal protection subsystems. We successfully met such challenges and are nearing the launch of the first Shuttle orbital flight.Our immediate goal is to enter the Space Shuttle operational phase because only then will we fully understand the unique capabilities of the Shuttle. Concurrent with our effort to begin Shuttle operations are our initial efforts to expand Shuttle capabilities, extending them significantly beyond those of the current baseline system.Shuttle payload capacity and mission-duration capabilities are to increase considerably during the next decade. Just as present Shuttle performance specifications and development timetables were guided by the space program plans and forecasts of the 1960s, so will the development of long-range space programs be determined by our near-future achievements. We anticipate that the Space Shuttle will play a critical role in those achievements.     

Background in space-borne low-energy γ-ray telescopes

The scope of observational astronomy in the gamma-ray region of the spectrum is vast. The intimate relationship of these energetic photons with their parent particles and fields provides a direct probe of the high-energy physics phenomena which take place throughout the Universe. As an added bonus the gamma-ray domain contains a wealth of diagnostic information within discrete emission lines, which are derived from a variety of processes including nuclear de-excitation, cyclotron emission, and matter-antimatter annihilation. Consequently observational gamma-ray astronomy addresses directly some of the most fundamental problems in both physics and astrophysics. However, low-energy gamma-rays are the most penetrating photons encountered in nature, and, whilst this factor provides a deep probe of cosmic objects, it ensures that gamma-ray telescopes are massive, both in terms of the stopping power required in the detector systems as well as their shields. Furthermore, the intimate relationship of gamma-rays with nuclear de-excitations ensures that the telescope itself becomes a bright source of background noise, a factor which is aggravated by the necessity that gamma-ray telescopes are obliged to operate in regions pervaded by intense particle fluxes. The background noise experienced in gamma-ray telescopes is, therefore, both high and extremely complex in its origin, and due to the high-energy content of individual photons, their numbers which arrive from distant cosmic sources are necessarily low, even for those objects which radiate the bulk of their power at gamma-ray wavelengths. Current gamma-ray telescopes are thus obliged to operate under conditions of intrinsically low signal-to-noise ratio and it is vital that techniques are developed which reduce the background noise level to more acceptable levels, thus improving the sensitivity. To achieve such a goal, a thorough understanding of the sources of background noise is first required before effective measures can be taken for its reduction.In this paper the sources of background noise are reviewed with the aim to obtain a quantitative analysis of individual contributions, as derived from the various classes of irradiative particle fluxes. The estimated contributions from the individual sources are combined in order to evaluate the total background level of a given telescope in a specific radiation environment, which for practical considerations generally relates to the orbit choice and detailed design of the telescope. The published background noise spectra of a number of past missions are compared to the computed values so as to provide an assessment of the validity of the overall calculations. The level of agreement achieved indicates that a good understanding of the sources of background noise exists. Finally some possibilities for the improvement of the sensitivity of future gammaray telescopes, in terms of the reduction of the background noise, are discussed.     

NGC 4151 and MCG 8-11-11: Two X-ray seyfert galaxies with strong soft γ-ray emission

During a balloon flight of the MISO telescope on the 30th September 1979, the Seyfert galaxies NGC 4151 and MGC 8-11-11 were studied in the hard X-ray range (E_X > 20 keV) and low-energy -ray range up to 19 MeV. An emission at the 4.5 level above 20 keV (4 above 260 keV) was detected in the direction of NGC 4151. -ray emission at the 3.9 level above 90 keV was also observed from the direction of MCG 8-11-11. The emission photon spectrum shows a high-energy cutoff at about 3 MeV. A large amount of the observed low-energy -ray diffuse background could be produced by a few percent of the X-ray emitting Seyfert galaxies having a -ray luminosity comparable to that observed from the regions of NGC 4151 or MCG 8-11-11.     

Adenine synthesis in interstellar space: mechanisms of prebiotic pyrimidine-ring formation of monocyclic HCN-pentamers

The question whether the nucleobases can be synthesized in interstellar space is of fundamental significance in considerations of the origin of life. Adenine is formally the HCN pentamer, and experiments have demonstrated that adenine is formed under certain conditions by HCN pentamerization in gas, liquid, and condensed phases. Most mechanistic proposals invoke the intermediacy of the HCN tetramer AICN (4), and it is thought that adenine synthesis is completed by addition of the 5(th) HCN to 4 to form amidine 5 and subsequent pyrimidine cyclization. In this context, we have been studying the mechanism for prebiotic pyrimidine-ring formation of monocyclic HCN-pentamers with ab initio electronic structure theory. The calculations model gas phase chemistry, and the results primarily inform discussions of adenine synthesis in interstellar space. Purine formation requires tautomerization of 5 to the conjugated amidine 6 (via hydrogen-tunneling, thermally with H(+) -catalysis, or by photolysis) or to keteneimine 7 (by photolysis). It was found that 5-(N'-formamidinyl)-1H-imidazole-4-carbonitrile (6) can serve as a substrate for proton-catalyzed purine formation under photolytic conditions and N-(4-(iminomethylene)-1H-imidazol-5(4H)-ylidene)formamidine (7) can serve as a substrate for uncatalyzed purine formation under photolytic conditions. The absence of any sizeable activation barrier for the cyclization of 7 to the (Z)-imino form of 9H-adenine (Z)-2 is quite remarkable, and it is this feature that allows for the formation of the purine skeleton from 7 without any further activation.     

车用开关磁阻电机起动／发电／助力一体化系统研究

介绍了一种基于DSP和CPLD的车用开关磁阻电机起动/发电/助力一体化系统。该系统研制了一台3 kW12/10结构开关磁阻电机作为机电能量转换装置,采用TM S320F 240型DSP和EPM 7128S型CPLD构成数字控制器,可实现汽车的起动、助力、发电等一体化功能。在控制策略上,起动时以获得最大电磁转矩为优化目标,助力时兼顾转矩和效率,发电时则根据蓄电池的荷电情况自动选择恒流充电和恒压充电。实验结果表明,本文提出的车用开关磁阻电机起动/发电/助力一体化系统具有优良的电动、发电及缺相运行性能,能满足汽车的起动、助力、发电等一体化功能要求。     

Hard X-ray observations of Cygnus X-1 with the MISO telescope

The black hole candidate Cygnus X-1 was observed in the hard X ray - soft γ ray energy range by the MISO telescope on two different occasions: in September 1979 and May 1980. We have measured two hard X-ray states of the source: in 1979 the observed spectrum confirms the superlow state measured in the same period by the HEAO-3 satellite, while in 1980 the MISO X-ray data are consistent with the so called low state of Cygnus X-1. In both occasions, no γ -ray excess has been observed above 200 KeV.     

新型双脚步推式微型进给机构的研究

相对于传统“尺蠖式”进给原理，模仿人走路的方式，提出“双脚步推式”进给原理。利用压电元件为驱动源，研制出在大范围内，具有很高分辨力，同时能够连续平稳进给的微型进给机构。该机构的优点概括为：１）不论压电元件的电致伸缩量是多么的有限，利用“双脚步推式”进给原理，可以实现连续平稳的大范围进给；２）在开环控制状态下，该机构能够得到高于０．１μｍ的位移分辨力；３）系统结构简单，控制容易，性能稳定。     

邹炳锁 材料科学专家

<正>作为材料科学与工程领域的专家,您主持研究的许多成果达到了国内领先、国际先进水平,请您介绍一下您所从事的研究工作及取得的研究成果和进展。邹炳锁:我们开展的工作主要是半导体的光电行为,探索其在能