中国上市公司会计信息披露制度研究

上市公司会计信息披露制度不仅保证公司创造价值最大化,而且保证价值在公司各相关利益者之间的公平分配,其核心目标是保护小股东权益.文章深入分析了中国上市公司会计信息披露制度所存在的公司内部治理和外部治理环境的缺陷,认为中国上市公司会计信息披露制度问题源于两方面:一是公司内部治理结构中缺乏为确保所披露的会计信息的质量所作出的有效的制度安排;二是公司外部治理环境中信息披露体系方面的制度缺陷.在保持适度的强制性会计信息披露的情况下,对改善我国上市公司会计信息披露制度提出建议.     

空气雾化喷嘴内液膜对雾化性能的作用

本文综合归纳数年来对空气雾化喷嘴内液膜厚度特性,液膜表面扰动波动态特性以及这些特性与雾化特性间的关系等方面的研究结果.着重指出在喷嘴唇口附近没有周期性的液流堆积现象,并且指出唇口液流堆积雾化论的问题所在.     

熵定律与大学教育可持续发展研究

本文针对在焙定律作用下，大学教育出现的无序化现象和各种有碍于大学教育可持续发展的因素进行了分析，并给出了解决这些问题的相应对策。     

高速风洞引射式进排气动力模拟试验研究

为了测定具有埋入式进气道的某航弹发动机进排气对航弹的气动影响量 ,采用引射式动力模拟器在FL 7高速风洞 ,首次在国内成功地进行了高速风洞进排气动力模拟试验。试验模型缩比为 1∶1 0 ,M =0 .7,P0j/P∞ =2 .62 ,Cφ=0 .79。试验结果表明 ,有动力后XD,CL,CD增加 ,Cma减少。试验表明在高速风洞中对于小尺寸的试验模型 ,采用引射式动力模拟器开展进排气动力模拟试验是一种简便适用的好方法     

无任何附加假设的梁的自由振动

本文不采用平面假设来研究梁的弯曲自由振动，也不采用剪切型振动假设研究短粗梁的自由振动，而用弹性力学的位移法导出了梁的自由振动微分方程，并推导了简支梁的自振频率的统一公式，其特殊情况即为有附加假设的自振频率公式。     

行星际空间MHD模拟激波跃变关系分析

分析了模拟得到的可以传播到1AU以远的日地空间磁流体力学激波与Rankine-Hugnoniot跃变关系的符合程度．通过对模拟激波的结构及其在传播过程中的演化进行的分析，提出了模拟激波的定位方法；基于所提出的定位方法，利用向长青提出的确定MHD激波局地参数的方法计算了模拟得到的激波与Rankine-Hugnoniot跃变关系的偏差．结果表明在激波传播到100Rs以后，激波对中前向快激波与Rankine-Hugnoniot关系的符合达到很高的程度，相对误差在10^-2数量级以内；并且在激波传播到150 Rs以后，相对误差在10^-3数量级以内．这个结果说明文中所使用的有限差分数值格式能较好地模拟激波．     

建立腔体热释电探测器相对光谱响应度标尺的研究

由于腔体热释电探测器在宽光谱范围内具有相对平坦的光谱响应度,因此经常被用作标定探测器相对光谱响应度的工作基准。但是在标定过程中通常认为腔体热释电探测器是无光谱选择性的,即R(λ)为常数。这样就会使测量结果不够准确,因此建立腔体热释电探测器相对光谱响应度的标尺是非常重要的。本文主要介绍了建立腔体热释电探测器相对光谱响应度标尺的原理和方法,并通过实验利用该方法建立了腔体热释电探测器相对光谱响应度的标尺,从而使该腔体热释电探测器成为红外光谱响应度测量装置的工作基准。     

无刷直流电动机的新型自适应模糊神经控制

 为无刷直流电动机提出了一种自适应模糊神经控制方法.这是一种建立在开关控制、模糊控制和自适应控制相结合基础上的控制方法,并用神经网络实现了模糊控制器和自适应机构.在无刷直流电动机的双闭环调速系统中,电流控制器是PI控制器;转速控制器是由1个开关控制器和1个包括自适应机构在内的模糊控制器相结合组成的,且用1个3层前向神经网络离线学习实现了模糊控制器,学习算法采用的是改进的BP算法.用1个单神经元通过在系统运行过程中的动态学习实现了自适应机构,学习算法选用了有监督的Hebb学习算法.由电机所处的运行阶段决定哪一个控制器工作.此控制算法的仿真结果说明,它使系统具有良好的动、静态特性和自适应性.     

Crystal orientation and morphology of a lamellae in wrought titanium alloys: On the role of microstructure evolution in b processing

To obtain high-quality aviation forgings of titanium alloys, b forging is an essential processing step which must be considered throughout a production process. In this work, the effect of b forging on the crystal orientation and morphology of lamellar a was experimentally investigated in a two-phase titanium alloy. Strong dynamic recovery during b working resulted in the formation of low-angle grain boundary(LAGBb) inside b grains. The lamellar a can penetrate through the LAGBb, leading to similar intra a LAGBs on subgrain boundaries. Deformation banding occurs at high strain rates, and both diffusive and sharp boundaries of deformation bands can be observed.A continuous change of the b orientation in diffusive boundaries results in the formation of fine and disordered a lamellae without intra-lamellar boundary to hold the Burgers orientation relationship(OR). On sharp boundaries, it is prone to producing continuous grain boundary a(aGB) with a highly similar orientation along the boundaries. Meanwhile, there may exist several lower-angle boundaries within the grain boundary a for a smoother orientation change on the b grain boundary.     

Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occultation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.