高职"机务维修"专业实训教学存在的问题及对策

近年来，高职教育机务专业在我国有了很大发展，为我国航空事业培养了大批的专业技术人才，但由于民航业的快速发展和传统教育观念的影响，机务专业在实训教学环节中显露出了一些问题与不足，针对这些问题，深入探讨了高职教育机务专业在实训教学中应采取的一些措施及对策。     

Mercury’s Birkeland current system

A consideration is given to the generation of field-aligned currents under different solar wind conditions. The preliminary results from a set of resistive MHD calculations indicate that the field-aligned current system could be significantly changed by the orientation of the interplanetary magnetic field. For most of the cases studied, the total current is less than or on the order of 10⁵ A. Even though this current is at least a factor of 10 smaller than its counter part at Earth, it might still produce some important dynamical effects with interesting consequence on the sporadic behavior of Mercury’s atomic sodium emission.     

我国利润表编制中存在的问题与改进

文章论述了利润表设计的理论依据,通过我国利润表同国外利润表比较,发现我国利润表的编制基础对会计信息的陈报存在不利影响,并结合实际情况,提出了未来利润表改进办法.     

管理信息系统的特征及发展趋势

文章从“四字格”在报刊译文中的主要作用及其运用场合两个方面进行了较为详细的探讨，并对如何恰当地运用“四字格”词组作了简要的阐明。     

有关航天遥感图像地面分辨率的札记

通常所言的航天遥感图像的地面分辨率只是与图像细部特征尺度相对应的地面尺度。对有关航天遥感图像地面分辨率的几个问题进行了讨论。     

地面长时间微重力装置原理及设计

采用串联的Maxwell摆作为主机构，可以实现地面上长时间、低速度的连续失重环境，解决了地面上长时间失重伴随的速度无限增大及加速度反弹问题。     

军用ATS测试总线技术的现状与发展趋势

总线技术,特别是外部总线技术在装备自动测试系统(ATS)中占有十分重要的地位,是构成装备自动测试系统的桥梁与纽带.本文较为详细地介绍了现有军用ATS中常用的几种外部总线,并对主要外部总线的性能进行了比较;对军用ATS外部总线技术的发展趋势进行了展望,指出带热插拔功能的USB总线及满足高吞吐量、长传输距离的总线将成为未来总线发展的趋势.     

多电飞机大功率高压直流起动发电机系统研究与实现

起动发电（SG）一体化是多电飞机（MEA）和全电飞机（AEA）机载主电源系统的重要特征与关键技术。高压直流电源（HVDC）系统输出不受交流电频率约束，电机可工作在更高转速从而提高功率密度，且易于并联提高供电可靠性，已经成为飞机电源系统的重要发展方向。提出三级式高压直流起动发电系统架构，阐述了其组成和工作原理，分析了发电和起动模态下永磁发电机（PMG）、励磁机（ME）和主电机（MG）的运行特性，以及发电模态下励磁机的恒流源和电流放大器特性；研究了起动模态下主电机的转矩产生机理和影响因素以及励磁机单相交流励磁特性。研制成功120 kW/270 V高压直流起动发电机系统，构建起动发电一体化实验平台，完成了发电及发动机模拟起动运行实验，实验与仿真结果一致，为大功率高压直流起动发电系统在新一代飞机上的应用奠定了理论和技术基础。     

Energy spectrum of proton flux near geomagnetic equator at low altitudes

The results of proton energy (tens keV – several MeV) spectrum measurements near geomagnetic equator (L < 1.15) at low altitudes (<1000 km) are presented. We used data of experiments onboard ACTIVE, SAMPEX, NOAA TIROS-N satellites and SPRUT-VI (MIR station) and cover a time range of about 30 years (including previous measurements). It was found that the kappa-distribution function fits the experimental spectrum with the best correlation coefficient. A comparison of energy spectra of near-equatorial protons and ring-current protons was made. Using the estimation of the life time of near-equatorial protons we explain the difference in spectral indices of radiation belt and near-equatorial proton formation. We conclude that the ring current is the main source of the near-equatorial protons.     

Statistical study of the detection of solar protons of highest energies at 20 January 2005

On January 20, 2005, 7:02–7:04 UT the Aragats Multichannel Muon Monitor (AMMM) registered enhancement of the high energy secondary muon flux (energy threshold ∼5 GeV). The enhancement, lasting 3 min, has statistical significance of ∼4σ and is related to the X7.1 flare seen by the GOES satellite and the ground level enhancement detected by the world-wide network of neutron monitors and by muon detectors. The most probable proton energy corresponding to the measured 5 GeV muon flux is within 23–30 GeV. Due to upmost importance of the detection of solar particles of highest energies in presented paper we perform detailed statistical analysis of the detected peak. The statistical technique introduced in the paper is also appropriate for the searches of sources of ultra-high energy cosmic rays.