基于TC35i和C8051F020的远程数据采集系统

本文提出了一种用混合信号系统级单片机C8051F020控制GSM网络引擎TC35i实现远程数据采集的方案。在描述了远程数据采集系统原理、构成和功能的基础上，对无线通讯模块及硬件和软件设计部分也进行了详细介绍。     

基于TC35i和C8051F020的远程数据采集系统

本文提出了一种用混合信号系统级单片机C8051F020控制GSM网络引擎TC35i实现远程数据采集的方案.在描述了远程数据采集系统原理、构成和功能的基础上,对无线通讯模块及硬件和软件设计部分也进行了详细介绍.     

Daytime VHF amplitude scintillations recorded at an Indian low-latitude station,Waltair (17.7°N, 83.3°E) during 1997–2003

In this research, it is presented the daytime amplitude scintillations recorded at VHF frequency (244 MHz) at an Indian low-latitude station, Waltair (17.7°N, 83.3°E) during seven continuous years (1997–2003). Contrary to the nighttime scintillation seasonal trends, the occurrence of daytime scintillations maximizes during summer followed by winter and the equinox seasons. The fade depths, scintillation indices and the patch durations of daytime scintillations are meager when compared with their nighttime counterparts. A co-located digital high frequency (HF) ionosonde radar confirms the presence of sporadic (Es) layers when daytime scintillations are observed. The presence of daytime scintillations is evident when the critical frequency of the Es-layer (foEs) is ≥4 MHz and Es-layers are characterized by a highly diffuse range spread Es echoes as can be seen on ionograms. It is surmised that the gradient drift instability (GDI) seems to be the possible mechanism for the generation of these daytime scintillations. It is quite likely that the spread Es-F-layer coupling is done through polarization electric fields (Ep) that develop inside the destabilized patches of sporadic E layers, which are mapped up to the F region along the field lines as to initiate the daytime scintillations through the GDI mechanism. Further, the presence of additional stratification of ionosphere F-layer, popularly known as the F3-layer, is observed on ionograms once the Es-layers and daytime scintillations are ceased.     

F12/环氧复合材料力学性能研究

测定了Ｆ１２／环氧复合材料的基本力学性能,并比较了Ｆ１２纤维在单向板、强力环及薄壁容器中的纤维强度转化率。实验结果表明,Ｆ１２／环氧单向复合材料与其ＮＯＬ环的拉伸强度相近,而薄壁容器中的复合强度约为单向拉伸强度的６０％,但三种复合材料的纤维强度转化率相近,约为（７０．１±１．６）％。     

一种用于ISA总线计算机1553B接口模块的设计

介绍一种用于ＩＳＡ总线计算机的低成本的１５５３Ｂ总线接口模块的设计,该设计使得１５５３Ｂ终端具有与美国ＤＤＣ－ＩＤＥＡ产品类同的功能,可进行１５５３Ｂ产品或系统的开发、仿真。简要介绍了模块的硬件设计和软件配置,罗列了其设计特点。     

日食对低纬地区f0F2和ICF的影响

研究了１９９５年１０月２４日日食过程中,我国低纬地区广州和海口的Ｆ２层临界频率ｆ０Ｆ２的高干扰重心频率ＩＣＦ变化过程,鉴于多次日 处低纬的两地ｆ０Ｆ２的日食变化形态不完全一样,以及多次日食期间同一地方ｆ０Ｆ２变化形态不完全一样,ＩＣＦ也并不像预想的那样降低,因而对于低纬电离层,动力学过程可能要比直接与太阳辐射有关的光化学过程起更为重要的作用。     

论赤道扩展F的密度不规则体(Ⅱ)

本文对等离子体中的电子和离子分别采用流体和动力论描述, 导出适于描述夜间赤道F层现象的若干非线性模型。由此证明赤道扩展F小尺度区域可存在大量偶极涡、孤子和孤子链等类型的密度不规则体。      

B／Al单向铺层复合板的力学性能及断裂行为的研究

研究了热压扩散结合工艺对Ｂ／Ａｌ复合材料的强度的影响,并对试样拉伸断口及断裂径进行了研究,分析表明,试样断口有三种断裂模型,断裂路径同热压工艺有密切的关系。     

赴英国学习培训考察报告

通过考察了解了英国目前的教育体制与职业培训体系以及作者对英国职业教育的印象、感触及启示。在不同的历史时期，英国职业教育及其培训的形式不同；英国颁布的一些法律对发展职业教育起到了非常重要的作用；政府在职业教育及其培训中扮演了重要的角色。     

Fundamental (f) oscillations in a magnetically coupled solar interior-atmosphere system – An analytical approach

Solar fundamental (f) acoustic mode oscillations are investigated analytically in a magnetohydrodynamic (MHD) model. The model consists of three layers in planar geometry, representing the solar interior, the magnetic atmosphere, and a transitional layer sandwiched between them. Since we focus on the fundamental mode here, we assume the plasma is incompressible. A horizontal, canopy-like, magnetic field is introduced to the atmosphere, in which degenerated slow MHD waves can exist. The global (f-mode) oscillations can couple to local atmospheric Alfvén waves, resulting, e.g., in a frequency shift of the oscillations. The dispersion relation of the global oscillation mode is derived, and is solved analytically for the thin-transitional layer approximation and for the weak-field approximation. Analytical formulae are also provided for the frequency shifts due to the presence of a thin transitional layer and a weak atmospheric magnetic field. The analytical results generally indicate that, compared to the fundamental value ($\omega =\sqrt{\mathit{gk}}$), the mode frequency is reduced by the presence of an atmosphere by a few per cent. A thin transitional layer reduces the eigen-frequencies further by about an additional hundred microhertz. Finally, a weak atmospheric magnetic field can slightly, by a few percent, increase the frequency of the eigen-mode. Stronger magnetic fields, however, can increase the f-mode frequency by even up to ten per cent, which cannot be seen in observed data. The presence of a magnetic atmosphere in the three-layer model also introduces non-permitted propagation windows in the frequency spectrum; here, f-mode oscillations cannot exist with certain values of the harmonic degree. The eigen-frequencies can be sensitive to the background physical parameters, such as an atmospheric density scale-height or the rate of the plasma density drop at the photosphere. Such information, if ever observed with high-resolution instrumentation and inverted, could help to gain further insight into solar magnetic structures by means of solar magneto-seismology, and could provide further insight into the role of magnetism in solar oscillations.