Change of Electronic Structure and Magnetic Properties with MgO and Fe Thicknesses in Fe/MgO/Fe Magnetic Tunnel Junction

The effects of the thickness of MgO and Fe on the electronic structure and magnetic properties of Fe/MgO/Fe magnetic tunnel junction was studied using the first principle method. Two series of models with MgO of different thicknesses: Fe(3)MgO(t)Fe(3) (t=1,3,5,7) and with Fe of varied thicknesses: Fe(t)MgO(3)Fe(t) (t=3,4,5,6,7) were established. Calculated results show that in all the models the magnetic moment of Fe increases at the Fe/MgO interface and surface as compared with that of the inner layers. The mag-netic moment of each Fe layer was found to be independent of MgO thicknesses, while the spin-polarization of Fe layer at the interface shows a slight change in function of the MgO thicknesses. The tunneling magnetoresistance (TMR) ratio estimated by the Julliere model has the same change tendency as the spin-polarization has, and the largest value is obtained at the MgO thickness of 5 atomic layers. When the Fe thickness increases, the spin-polarization of interface Fe layer follows up an increase with a decrease. The highest TMR value is achieved when the Fe thickness is of 4 atomic layers.     

核壳结构Fe/Al复合粉体的制备及其放热性能分析

为了解决微米铝粉燃烧动力学慢、点火延迟长、燃烧不充分等问题,以羰基铁为前驱体,用流化床化学气相沉积(FB-CVD)法对两种不同粒径的微米铝粉进行了包覆,利用SEM,XRD和TG-DSC对所制得的Fe/A1复合粉体进行了表征.结果表明铁层均匀致密地包覆在铝颗粒表面,由Q1铝粉所制备的样品中铁的含量分别为3.62％,7.82％,12.83％.铁的包覆对铝的放热性能有很大影响,复合粉体的高温放热峰温度相对于原始铝粉虽有所升高,但是其放热过程更迅速、更集中,氧化得更充分,1500℃时其增重由原始铝粉的20.74％提高到75.74％以上,铁的包覆量为7.82％的复合粉体增重可达到80.71％,其放热性能最优.     

纳米TiO2/Fe2O3复合材料的制备及其红外吸收性能研究

用溶胶-凝胶法制备了纳米TiO2／Fe2O3复合材料，并用XRD、TEM等方法对其进行了表征，给出了相关的工艺参数。研究了不同组分的纳米TiO2／Fe2O3的红外吸收特性。结果表明，纳米TiO2／Fe2O3复合材料在400cm^-1～1000cm^-1内随Fe2O3含量的增加，吸收峰明显宽化。     

ICP-AES法测定钛基复合材料中的Sn, Zr, Nb, Ta, Nd和Fe的研究

采用ICP-AES法对钛基复合材料中的合金元素Sn,Zr,Nb,Ta,Nd,Fe的测定进行了研究,着重进行了基体元素及待测元素Sn,Zr,Nb,Ta,Nd,Fe之间干扰试验及各元素在测定浓度范围内的线性相关性试验,进行了酸度试验及Ta,Nb,Zr的酸不溶试验,测定了钛基复合材料中上述六元素的含量,得到了较好的精密度和准确度.方法简便可靠,可获得满意的分析结果.     

Fe含量对2219铝合金锻件焊接组织与性能的影响

为研究杂质Fe元素对2219铝合金及其焊接接头的组织、性能以及电化学腐蚀性能等的影响,采用力学拉伸、焊接试验以及金相和扫描电镜等分析测试方法,对0.15%(w)至0.01%(w)等不同Fe元素含量的2219铝合金锻件进行实验研究和分析。研究表明:2219铝合金中经热变形加工存在网络状Al_2Cu变成颗粒状和纤维状的Al_7Cu_2(Fe,Mn)相,随着Fe含量由0.15%(w)降低至0.01%(w),合金固溶时效后的Al_7Cu_2(Fe,Mn)相显著减少,锻件强度和塑性显著提高;合金焊接接头断口由脆性断裂逐渐转变为韧窝尺寸细小的韧性断裂,尤其对于延伸率,提高至近1.4倍,强度和塑性显著提高;合金的自腐蚀电流逐渐减小,单位面积上的线性极化电阻增大,合金焊接接头的耐腐蚀性能显著提高。     

Fe83Ga17合金应力作用下磁化机理的研究

利用定向凝固方法制备出[110]轴向取向的Fe83Ga17合金，研究了Fe83Ga17合金的磁致伸缩性能，测量了Fe13Ga17的磁致伸缩系数和饱和磁化场、应用能量最低原理，研究了合金在磁场和应力作用下的磁化机理，构建了磁化模型计算结果与实验现象基本吻合，部分计算结果与实验数据存在一定的差别，表明理论模型还需进一步改进。     

粉末烧结法制备Al/Tb0.3Dy0.7Fe1.95磁致伸缩复合材料

采用粉末烧结法制备了Al/Tb0.3Dy0.7Fe1.95磁致伸缩复合材料,研究了烧结温度对烧结体的显微结构、相组成、磁致伸缩、抗压强度等性能的影响.研究结果表明,600 ℃烧结时,烧结体中仍主要存在Al与GMM合金相,烧结获得较理想的相分布状态.随着烧结温度的增加,复合体中非GMM相越来越多,原始相减少.当1200 ℃烧结时,烧结体中主要存在杂相,已几乎没有GMM相.随着烧结温度的增加,复合材料的λs和抗压强度明显下降,烧结温度为600 ℃时,烧结体的λs和抗压强度最大,分别为405×10-6和61.71MPa.其不足是,复合材料仍呈现明显的脆性特征.     

Microstructure and Mechanical Properties of Cross-rolled Ti50Ni47Fe3 Shape Memory Alloy

The microstructures, the phase transformation characteristics, and the mechanical properties of the Ti50Ni47Fe3 alloy in as-forged and as-cross-rolled states were investigated. It is found that, after cross-rolling, the phase transformation temperature （Ms） of the alloy decreases drastically and the grains get refined. Moreover, its yield strength and fracture strength after cross-rolling hit 540 MPa and 687 MPa respectively, up by about 200 MPa over those in as-forged state.     

Microstructure and Mechanical Properties of Cross-rolled Ti_(50)Ni_(47)Fe_3 Shape Memory Alloy

The microstructures, the phase transformation characteristics, and the mechanical properties of the Ti50Ni47Fe3 alloy in as-forged and as-cross-rolled states were investigated. It is found that, after cross-rolling, the phase transformation temperature (Ms) of the alloy decreases drastically and the grains get refined. Moreover, its yield strength and fracture strength after cross-rolling hit 540 MPa and 687 MPa respectively, up by about 200 MPa over those in as-forged state.     

合金化及热处理对Fe_3Al合金组织和性能影响

研究了不同的热处理条件及添加Mn,Mo,Nb,Cr,V,RE（La-Ce）等合金元素对Fe3Al合金组织和性能的影响。结果表明,Fe3Al合金在B2相区间保温淬火后的硬度值较小,在DO3相区短时间回火硬度值大幅增加,随回火时间延长硬度值呈降低趋势,在本实验的最长回火时间内（50h）硬度稍有提高;TEM分析表明,这与回火过程中DO3畴的尺寸变化有关;合金化后Cr和V的加入降低合金硬度,其它几种元素都提高了合金的硬度;SEM分析表明合金元素的作用机理不同：Cr软化了合金,Mo主要产生固溶强化,Mn、V、Nb加入后有第二相析出,RE元素主要偏析在晶界,细晶强化。     

反应铸造TiC／NiAl（Fe）复合材料的力学行为和强化机理研究

研究了反应铸造ＴｉＣ／ＮｉＡｌ（Ｆｅ）复合材料压缩、拉伸性能和强韧化机制。ＮｉＡｌ（Ｆｅ）合金的室温拉伸延伸率达１１％。含２０％ＴｉＣ颗粒的ＮｉＡｌ（Ｆｅ）基复合材料的室温拉伸率为２．５％。与多晶ＮｉＡｌ合金及其复合材料相比,２０％ＴｉＣ／ＮｉＡｌ（Ｆｅ）复合材料的室温拉伸延伸率明显提高。原位合成的ＴｉＣ增强颗粒在高温下具有明显的增强效果,含２０％ＴｉＣ增强颗粒复合材料的高温强度比基体合金高１００％。塑性的枝晶间区域的存在是ＮｉＡｌ（Ｆｅ）及其复合材料在室温塑性得以改善的主要机制。ＸＤ＋ＲＣ工艺导致的晶粒细化作用是ＮｉＡｌ（Ｆｅ）基复合材料的主要强化机制,位错强化和弥散强化对强度也有一定贡献。     

Fe2 O3 对碳热还原氮化SiO2 合成Si2 N2 O的催化效应及机理

采用碳热还原氮化SiO2的方法在1 500℃制备了Si2N2O,并通过XRD和热失重分析,研究了Fe2O3对合成Si2N2O的催化作用及机理。Fe2O3对Si2N2O的合成具有显著的催化作用,加入少量Fe2O3可以使SiO2的转化率达到100%。Fe2O3的催化机理为:一方面,Fe2O3被C还原为纳米铁单质,并与Si形成Fe-Si液相,该Fe-Si液相可溶解SiO2和C颗粒,促使SiOC中间相在较低温度下形成,从而显著降低碳热还原反应的开始温度。另一方面,Fe-Si液相中的CO2与FeSi反应,通过形成SiO和CO而加速碳热还原反应的进行。     

基于磁信号逆变技术的航姿系统综合检查仪设计

描述了一种快速地检测飞机航姿系统全套及部件200多个信号的航姿综合检查仪.该检查仪采用斩波放大及逆变技术实现了微弱磁信号采集的数字化处理,系统航向、姿态检测精度从原模拟式检测设备的1°提高到现在的0.1°,与原模拟式检查仪相比,维护效率提高了5倍以上.应用小波去噪抗干扰技术,滤除交流电源产生的噪声,从而大大降低系统的漏检率和误警率,整套系统性能及可靠性大大增强.     

一种电磁性复合材料的研究

通过对Fe3O4 化学镀Ag,提高其电导率,从而获得电磁性能优异的复合材料。进行化学镀之前,
要对Fe3O4 进行包括粗化、敏化和活化等预处理。测试结果表明:Fe3O4 表面成功包覆一层Ag,厚度大约为25
~100 nm,Ag 含量达到54. 47%;Ag/ Fe3O4 的电导率σ =347. 15 S/ cm,相比Fe3O4 升高了9 个数量级,饱和磁
化强度Ms =29. 8 emu/ g。     

压制工艺和粒径对粉末冶金Ti-1Al-8V-5Fe合金组织性能的影响

采用粉末冶金技术以氢化钛（TiH₂）粉和不同粒径的元素粉体为原料制备Ti-1Al-8V-5Fe（Ti-185）合金,研究了压制工艺对不同粒径元素粉制备的Ti-185合金组织及性能的影响。结果表明：当压制压力在800 MPa、保压时间80 s、压制速率为1 mm/s时,Ti-185生坯密度最高,为最佳压制工艺。由粒径较小元素粉制备得到的Ti-185合金晶粒越细小,合金的烧结致密度就越高。粉末粒径越小,烧结过程中合金元素实现合金化需要扩散的距离就越短,越有利于合金力学性能的提高,其中具有最小粒径的样品表现出最高的硬度（43 HRC）和强度（1 438 MPa）。     

ICP-AES法测定纯铜中的Bi,Sb,As,Fe,Ni,Pb,Sn,Zn,Ag的方法

研究了ICP-AES法测定纯铜中的Bi,Sb,As,Fe,Ni,Pb,Sn,Zn和Ag等9个元素的分析方法.进行了基体元素铜对9个分析元素的光谱干扰研究,选择了合适的分析谱线,同时测定了分析方法的检出限.     

The STEREO/IMPACT Magnetic Field Experiment

The magnetometer on the STEREO mission is one of the sensors in the IMPACT instrument suite. A single, triaxial, wide-range, low-power and noise fluxgate magnetometer of traditional design—and reduced volume configuration—has been implemented in each spacecraft. The sensors are mounted on the IMPACT telescoping booms at a distance of ～3 m from the spacecraft body to reduce magnetic contamination. The electronics have been designed as an integral part of the IMPACT Data Processing Unit, sharing a common power converter and data/command interfaces. The instruments cover the range ±65,536 nT in two intervals controlled by the IDPU (±512 nT; ±65,536 nT). This very wide range allows operation of the instruments during all phases of the mission, including Earth flybys as well as during spacecraft test and integration in the geomagnetic field. The primary STEREO/IMPACT science objectives addressed by the magnetometer are the study of the interplanetary magnetic field (IMF), its response to solar activity, and its relationship to solar wind structure. The instruments were powered on and the booms deployed on November 1, 2006, seven days after the spacecraft were launched, and are operating nominally. A magnetic cleanliness program was implemented to minimize variable spacecraft fields and to ensure that the static spacecraft-generated magnetic field does not interfere with the measurements.     

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.     

Ti的添加方式对反应钎涂碳化物／铁基合金复合涂层组织结构的影响

利用钛铁粉、纯钛粉、铬铁粉或纯铬粉、硼铁粉、镍粉、硅粉和胶体石墨粉,真空条件下通过反应钎涂在低碳钢基体表面制备与基体为冶金结合的碳化物/铁基合金复合涂层.研究Ti的添加方式对涂层组织的影响.试验结果表明,涂层组织结构由粘结相Fe基体相和增强相碳化钛、碳化铬构成.Ti的添加方式对涂层组织结构影响很大.不同的Ti添加方式,导致涂层中碳化钛形态及涂层致密度差别较大.分析认为,Ti的添加方式对涂层组织结构的影响是由于涂层TiC合成时受到的动力学条件不完全相同造成的.     

Fe/O Ratios in Interplanetary Shock Accelerated Particles

It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal in these observations.