高灵敏度与高稳定性的飞机客舱内物品监测系统

介绍了一种新型的高稳定度、高灵敏度的飞机客舱内物品监测系统的工作原理和基本电路。该系统具有检测灵敏度高,抗干扰能力强,工作稳定可靠的特点。     

无陀螺磁控小卫星的大角度姿态捕获研究

为了解决无陀螺磁控小卫星的姿态稳定和捕获问题,本文针对偏置稳定的主动磁控小卫星姿态控制平台,基于磁控力矩的时间累积作用效果等效卫星角动量增量的规律,设计了一种仅利用角度反馈的卫星大角度磁捕获控制律。通过仿真和卫星在轨实测的验证,证明该方法具有良好的收敛效果和鲁棒性,工程实现简单,可靠性高,适用于中低轨道的通信小卫星。     

裂缝宽度对磁记忆信号的影响的研究

以经爆破试验的四件小钢管件裂纹为研究对象,找出裂纹宽度与磁记忆信号的关系,得出漏磁场变化梯度的最大值随裂缝宽度增加而增加。     

近室温磁制冷工质选择的热力学准则

对近年来在制冷界研究相当活跃的磁制冷的工质，尤其是近室温磁制冷的工质－铁磁材料，在外加磁场中的热力学特性进行了分析、讨论，并在此基础上总结了选取近室温磁制冷工质的理论依据和原则，使实际中的选择工作有了针对性，减少了盲目性。     

一种双管正激磁集成变换器

双管正激磁集成变换器的高频变压器磁芯双向磁化，提高了磁芯利用率。本文研究了导通占空比、开关管导通管压降以及变压器两原边的磁化电感等参数不一致时，导致变压器磁芯偏磁问题。磁芯的磁化状态虽受上述参数的不一致影响而出现单向磁化现象，但不会出现单向磁饱和，双管正激磁集成变换器仍能稳定工作，为能否采用平均电流控制模式或电压控制模式提供了理论依据。文中分析了变压器原边环流产生机理，提出了一种减小环流的方法。使环流减小一半。     

稀土磁弹簧吸振器特性的研究

首先简要介绍稀土金属制成的磁弹簧吸振器的构造和工作机理，然后着重介绍三种规格磁弹簧吸振器特性的测试、计算和分析，并对磁弹簧刚度的可调节性及其刚度与磁弹簧的有关参数间的关系进行了分析，最后得出了一些有实际应用价值的结论。     

风洞磁悬挂天平系统的数字控制

本文阐述了风洞磁悬挂天平系统数字控制器的工作原理、软硬件补偿及其配套的测量系统,并分析了数字控制器的特性及其与模拟控制器的本质区别。     

High magnetic gradient environment causes alterations of cytoskeleton and cytoskeleton-associated genes in human osteoblasts cultured in vitro

The effects of a high magnetic gradient environment (HMGE) on the cytoskeletal architecture and genes associated with the cytoskeleton in osteoblasts (MC3T3-E1 and MG-63 cells) were investigated using confocal microscopy, real-time polymerase chain reaction (PCR) and atomic force microscopy (AFM). The findings showed that, under diamagnetic levitation conditions, the architecture and average height of the cytoskeleton and surface roughness in osteoblasts were dramatically altered. HMGE affects cytoskeleton arrangement and cytoskeleton-associated gene expression.     

Mid 19th century minimum of galactic cosmic ray flux inferred from Ti in Allegan meteorite

Measurements of ⁴⁴Ti activity in meteorites show that the galactic cosmic ray (GCR) intensity has been declining in the interplanetary space during the past three centuries and has a component of cyclic variation, with periodicity of about 87 years [Taricco, C., Bhandari, N., Cane, D., et al. Galactic cosmic ray flux decline and periodicities in the interplanetary space during the last 3 centuries revealed by ⁴⁴Ti in meteorites. J. Geophys. Res. 111, A08102, 2006.]. In order to verify these results, we have measured ⁴⁴Ti activity in Allegan meteorite which fell in 1899 and in some other meteorites with better precision. The measurements confirm low cosmic ray flux and consequently high solar activity near the middle of 19th century.     

Study of correlations between waves and particle fluxes measured on board the DEMETER satellite

The topic of relativistic electron dynamics in the outer radiation belt has received considerable attention for many years. Nevertheless, the problem of understanding the physical phenomenon involved is far from being resolved. In this paper, we use DEMETER observations to examine the variations of the energetic electron fluxes and ELF/VLF wave intensities in the inner magnetosphere during the intense 8 November 2004 magnetic storm. Electron flux spectra and associated wave intensity spectra are analysed throughout the magnetic storm and common characteristics or differences to other storm events are retained. The overall objective of this study is to identify and derive parameters that are relevant for particle flux modelling; the time constant characterizing the persistent decay after particle enhancement was found to be one of these important model parameters.The analysis of the 8 November 2004 event reveals that for L-shell parameter higher than 4, an electron flux dropout is observed during the storm’s main phase for electrons in the energy range 0.1–1 MeV, as has been reported from other measurements. Characteristic wave spectra accompanying this phase are analysed. They show a typical enhancement in the frequency range 0.3–10 kHz at onset for all L-shell values under consideration (2 < L < 5). During the first stage of the recovery phase, the electron fluxes are increased to a level higher than the pre-storm level, whereas the level of wave intensity in the frequency range observed below 300 Hz is at its highest. In the second stage, the particle flux decrease goes hand in hand with a global wave activity decline, the relaxation time of the latter being smaller than the former’s one. In some other cases, long-lasting electron enhancement associated with constant wave activity has been observed during this latter stage. For the above mentioned storm, while at low L values the decay time constants are higher for low energy electrons than for high energy electrons, this order is reversed at high L values. At about L = 3.6 the time constant is independent of electron energy.