基于功能核磁共振成像的右脑额下回情绪处理

视觉刺激引起的情绪唤起是日常生活中的一种常见现象。本文通过功能核磁共振成像了解与视觉情绪刺激相关的脑功能归属。15位女性在其一个月经周期内接受了3次或更多的功能核磁共振扫描,实验中视觉刺激的形式包括成人影片与图片,平均所有测试结果得到了平均脑兴奋图。在平均脑兴奋图中可以发现,图片和影片形式的刺激均能有效地引起额下回的兴奋,与其他的兴奋脑区不同,呈现明显的右侧优势。根据实验结果,本文首次提出了右脑额下回在视觉感情信息处理中起到一定的作用,并且提出大脑额下回功能的优势化是双向而不是单向（向左侧）集中的。     

真空与磁场热处理改善FeCo合金的软磁性能

针对发电机中转子用FeCo合金(国产牌号1J22)进行了组织结构与磁性能的研究.通过对该合金进行真空处理以及磁场热处理,研究了组织结构对软磁性能的影响规律;研究了附加磁场强度以及热处理温度对磁场处理效果的影响,并结合该合金的磁致伸缩伸缩系数的变化规律,分析了磁场热处理效果的微观机制.当合金组织为轧制态时,磁场热处理效果不明显;在合金的再结晶温度以上进行磁场热处理时,获得了显著的磁场热处理效果,矫顽力下降至72A/m(0~9Oe)以下.     

Element and Isotopic Fractionation in Closed Magnetic Structures

Recent papers have suggested that the slow solar wind is a super-position of material which is released by reconnection from large coronal loops. This reconnection process is driven by large-scale motions of solar magnetic flux driven by the non-radial expansion of the solar wind from the differentially rotating photosphere into more rigidly rotating coronal holes. The elemental composition of the slow solar wind material is observed to be fractionated and more variable than the fast solar wind from coronal holes. Recently, it has also been reported that fractionation also occurs in 3He/4He. This may be interpreted in the frame-work of an existing model for fractionation on large coronal loops in which wave-particle interactions preferentially heat ions thereby modifying their scale-heights. This revised version was published online in June 2006 with corrections to the Cover Date.     

航天测绘发展现状与展望

航天测绘是全球基础测绘的主要手段,包括卫星地形测量、卫星重力测量、卫星磁力测量、卫星测高、卫星海洋测量等。航天测绘工程的发展经历了“返回型测绘卫星”工程、“传输型测绘卫星”工程和部分“集成型测绘卫星”工程。首先梳理了国际卫星测量的发展历史和现状,阐述了我国航天测绘各个阶段所发挥的作用,并分析了存在的问题,最后对航天测绘的未来发展提出了思路。     

多种软磁合金及金属非晶材料的磁屏蔽性能研究

针对部分航天器组件易受磁场影响的问题,文章选取了6种目前常用的软磁合金及金属非晶材料,研究了它们对于弱磁场波动、稳恒磁场以及低频交流磁场的屏蔽效果,结果表明,材料的磁导率与矫顽力对磁屏蔽性能有较大影响,其中矫顽力与磁屏蔽性能的负相关性更好,即矫顽力越低,材料的磁屏蔽性能越好。对于测试的6种材料,铁镍合金材料与钴基非晶材料的磁屏蔽性能优于其他4种,铁镍合金材料在1 kHz以下磁屏蔽性能更佳,钴基非晶材料在50 kHz以下具有一定磁屏蔽效果。     

某箭载综合放大器电磁兼容(EMC)设计

介绍了某箭载综合放大器的功能、原理、电磁兼容(EMC)设计及相应的EMC试验情况,并针对仪器在试验中出现的问题,进行了EMC改进设计和理论分析及试验验证。采取在敏感电路处增加高频旁路电容的改进措施后,仪器的电磁兼容性能得到增强,通过试验考核,表明改进设计合理有效。相应的EMC设计方法对其他箭载电子设备也有参考意义。     

新型切向磁钢混合励磁同步电机结构与原理

混合励磁电机兼具永磁电机高效率和电励磁电机励磁可调的优点。文中提出两种全新的具有轴向磁分路的混合励磁电机:两端轴向磁分路和单端轴向磁分路混合励磁同步电机。它们都是在切向磁钢永磁同步电机的基础上,将转子极靴沿轴向延伸,利用附加气隙及导磁桥形成轴向磁分路。阐述了两种新型电机的结构及原理,分析了两种电机的磁路特点,并给出其等效磁路。对比研究表明:单端轴向磁分路混合励磁电机轴向磁路短,电励磁效率高,是一种性能优越的混合励磁电机结构拓扑。     

磁悬浮多电发动机的研究

多电发动机是一个新概念的航空动力装置,是现代科技与航空动力科技相结合的方向。本文通过无人机用磁悬浮多电发动机的设计、转子模拟试验研究、辅助轴承试验研究等有关多电发动机部分关键技术的研究和发动机台架试车情况的描述,介绍了磁悬浮多电发动机试验研究概况。     

异常SSC事件的行星际原因分析

磁暴急始(SSC)是强烈太阳风动压或行星际激波与磁层相互作用的结果.通常SSC事件的上升时间在4～10 min,我们把上升时间超过15 min的SSC事件称为异常SSC事件.本文利用地磁SYM-H指数鉴别出了5个有地磁观测历史以来发生的上升时间大于15 min的异常SSC事件,并利用Wind,ACE,IMP 8,Goes,Geotail多点卫星太阳风观测数据和地磁观测数据,分析了异常SSC事件的行星际原因.结果表明,异常SSC事件通常都是强烈行星际扰动引起的,5个异常SSC事件有4个对应于行星际激波,有3个对应于多步太阳风动压跃变,有1个对应于行星际电场大幅度变化;由行星际激波产生的异常SSC事件,其上升时间依赖于行星际激波的方向,方向相对于日地连线越偏,上升时间越长;异常SSC事件上升时间与行星际磁场方向关系不明显.      

Sawtooth substorms generated under conditions of the steadily high solar wind energy input into the magnetosphere: Relationship between PC, AL and ASYM indices

Periodicity in occurrence of magnetic disturbances in polar cap and auroral zone under conditions of steady and powerful solar wind influence on the magnetosphere is analyzed on the example of 9 storm events with distinctly expressed sawtooth substorms (N = 48). Relationships between the polar cap magnetic activity (PC-index), magnetic disturbances in the auroral zone (AL-index) and value of the ring current asymmetry (ASYM index) were examined within the intervals of the PC growth phase and the PC decline phase inherent to each substorm. It is shown that the substorm sudden onsets are always preceded by the PC growth and that the substorm development does not affect the PC growth rate. On achieving the disturbance maximum, the PC and AL indices are simultaneously fall down to the level preceding the substorm, so that the higher the substorm intensity, the larger is the AL and PC drop in the decline phase. The ASYM index increases and decreases in conformity with the PC and AL behavior, the correlation between ASYM and PC being better than between ASYM and AL. Level of the solar wind energy input into the magnetosphere determines periodicity and intensity of disturbances: the higher the coupling function E_KL, the higher is substorm intensity and shorter is substorm length. Taking into account the permanently high level of auroral activity and inconsistency of aurora behavior and magnetic onsets during sawtooth substorms, the conclusion is made that auroral ionosphere conductivity is typically high and ensures an extremely high intensity of field-aligned currents in R1 FAC system. The periodicity of sawtooth substorms is determined by recurrent depletions and restorations of R1 currents, which are responsible for coordinated variations of magnetic activity in the polar cap and auroral zone.