在 Si 上生长的 GaAs 外延薄膜的近红外光致发光(英文)

在Ｓｉ上生长的异质ＧａＡｓ外延薄膜（记作ＧａＡｓ／Ｓｉ）中，存在着深能级，它们是由各类缺陷的各种不同荷电态所导致的。这些缺陷则是由于ＧａＡｓ与Ｓｉ之间存在着很大的晶格失配及热膨胀系数差异所引起的。研究了与ＧａＡｓ／Ｓｉ的深能级有关的变温与变激发强度的近红外光致发光谱。实验中所用的ＧａＡｓ／Ｓｉ样品是用ＭＯＣＶＤ方法生长的，而且具有不同的［Ａｓ］／［Ｇａ］比。利用组态模型，通过测量发光峰在半极大处的全宽度随温度的变化，获得了Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ位移。考虑了ＧａＡｓ／Ｓｉ的带隙随温度与随失配形变的移动。利用所获得的Ｆｒａｎｃｋ－Ｃｏｎｄｏｎ位移及带隙移动，修正了施主－受主对、导带－受主及施主－价带间跃迁的能量关系式，给出了新的表达式。按照建立的新的跃迁能量表达式及ＧａＡｓ／Ｓｉ外延薄膜发光谱的特征，鉴定出ＧａＡｓ／Ｓｉ中的三个发光峰属施主－受主对复合发光，另外两个发光峰则是由Ａｓ填隙－Ｇａ空位的复合发光中心所产生。     

在Si上生长的外GaAs的深化能级研究

本文对在Ｓｉ衬底上用金属－有机的化学汽相沉积法生长的ＧａＡｓ外处膜中的１．０４ｅＶ发射作了变温与变激发强度的近红外光致发光研究。该１．０４ｅＶ发射可用由Ｖ＾１－ＡＳ施主及Ｖ＾１－ＧＡ受主所组成的施主－受主对的复合发光来给予很好解释。     

ACTA AERONAUTICA ET ASTRONAUTICA SINICA

ＡＢＳＴＲＡＣＴＳ（Ｖｏｌ．２０，Ｎｏ．３）Ｐｒｅ－ｐｏｓｔｂｕｃｋｌｉｎｇａｎａｌｙｓｉｓｏｆｃｏｍｐｏｓｉｔｅｌａｍｉｎａｔｅｓｗｉｔｈｄｅｌａｍｉｎａｔｉｏｎｄａｍａｇｅ．ＳＵＮＸｉａｎ－ｎｉａｎ，ＣＨＥＮＨａｏ－ｒａｎ（ＤｅｐａｒｔｍｅｎｔｏｆＥｎｇｉｎｅｅｒｉｎｇＭｅｃｈａｎｉｃｓｏｆＤａｌｉａｎＵｎｉｖｅｒｓｉｔｙｏｆＴｅｃｈｎｏｌｏｇｙ，Ｄａｌｉａｎ１１６０２３，Ｃｈｉｎａ），ＣＨＥＮＳｈａｏ－ｊｉｅ（ＳｈｅｎｇｙａｎｇＡｉｒｃｒａｆｔＲｅｓｅａｒｃｈＩｎｓｔｉｔｕｔｅ，Ｓｈｅｎｙ…     

显示控制管理处理机验收试验程序的实现

介绍了显示控制管理处理机（ＤＣＮＰ）验收测试程序的编制.ＤCＭＰＡＴＰ程序由三部分组成：测试主机程序、ＤＳ１７５０程序和通讯模拟器程序．其中，测试主机和通讯模拟器的程序用ＶｉｓｕａｌＢａｓｉｃ５．０ｆｏｒＷｉｎｄｏｗｓ９５语言编制，ＤＳ１７５０端的程序用１７５０Ａ汇编语言编制。     

FATIGUE DISLOCATION CONFIGURATIONS IN HEXAGONAL ZIRCALOY-4

ＦＡＴＩＧＵＥＤＩＳＬＯＣＡＴＩＯＮＣＯＮＦＩＧＵＲＡＴＩＯＮＳＩＮＨＥＸＡＧＯＮＡＬＺＩＲＣＡＬＯＹ－４￥ＸｉａｏＬｉｎ（ＩｎｓｔｉｔｕｔｅｏｆＥｎｇｉｎｅｅｒｉｎｇＭｅｃｈ．，Ｘｉ＇ａｎＪｉａｏｔｏｎｇＵｎｉｖｅｒｓｉｔｙ，Ｘｉ＇ａｎ，Ｃｈｉｎａ...     

EXPERIMENTAL RESEARCH OF THE CONFIGURATION OF WING－TIP DRAG REDUCTION FOR LIGHT AIRCRAFT

ＥＸＰＥＲＩＭＥＮＴＡＬＲＥＳＥＡＲＣＨＯＦＴＨＥＣＯＮＦＩＧＵＲＡＴＩＯＮＯＦＷＩＮＧ－ＴＩＰＤＲＡＧＲＥＤＵＣＴＩＯＮＦＯＲＬＩＧＨＴＡＩＲＣＲＡＦＴＤｅｎｇＹａｎｍｉｎ，ＨｕＪｉｚｈｏｎｇ（ＦａｃｕｌｔｙｏｆＬｉｇｈｔＡｉｒｃｒａｆｔＤｅｓｉｇ...     

Abstracts of Acta Aeronauticaet Astronautica Sinica

ＢＳＴＲＡＣＴＳＣｏｎｆｌｉｃｔＰｒｏｂｌｅｍｏｆＤｅｍｐｓｔｅｒ ＳｈａｆｅｒＥｖｉｄｅｎｃｅＴｈｅｏｒｙ .ＺＨＡＮＧＳｈａｎ ｙｉｎｇ ,ＰＡＮＱｕａｎ ,ＺＨＡＮＧＨｏｎｇ ｃａｉ(Ｄｅｐａｒｔ ｍｅｎｔｏｆＡｕｔｏｍａｔｉｃＣｏｎｔｒｏｌ,ＮｏｒｔｈｗｅｓｔｅｒｎＰｏｌｙｔｅｃｈｎｉｃＵｎｉ ｖｅｒｓｉｔｙ ,Ｘｉ′ａｎ　 710 0 72 ,Ｃｈｉｎａ) .ＡｃｔａＡｅｒｏｎａｕｔｉｃａｅｔＡｓ ｔｒｏｎａｕｔｉｃａＳｉｎｉｃａ (ＩＳＳＮ 10 0 0 6 893) ,Ｖｏｌ.2 2 ,ｎｏ .4 ,Ｊｕｌｙ2 0 0 1,Ｐ36 9 372 .13ｒｅｆｓ…     

CUTTING TEMPERATURE OF CBN TOOLS WHEN MACHINING STEEL OF MEDIUM HARDNESS

ＣＵＴＴＩＮＧＴＥＭＰＥＲＡＴＵＲＥＯＦＣＢＮＴＯＯＬＳＷＨＥＮＭＡＣＨＩＮＩＮＧＳＴＥＥＬＯＦＭＥＤＩＵＭＨＡＲＤＮＥＳＳＣｈｅｎＷｕｙｉ１（陈五一），ＤａｖｉｄＫ．Ａｓｐｉｎｗａｌ２，ＨａｎＳｈｕｗｅｎ３（韩书文）１ＢｅｉｊｉｎｇＵｎｉｖｅｒｓｉ...     

SPECIAL HIGH-ORDER BENDING CRACK TIP FINITE ELEMENT FOR THE REISSNER PLATE

ＳＰＥＣＩＡＬＨＩＧＨ┐ＯＲＤＥＲＢＥＮＤＩＮＧＣＲＡＣＫＴＩＰＦＩＮＩＴＥＥＬＥＭＥＮＴＦＯＲＴＨＥＲＥＩＳＳＮＥＲＰＬＡＴＥＪｉａｎｇＣｈｉｐｉｎｇ（ＤｅｐａｒｔｍｅｎｔｏｆＦｌｉｇｈｔＶｅｈｉｃｌｅＤｅｓｉｇｎａｎｄＡｐｐｌｉｅｄＭｅｃｈａｎｉ...     

ANALYSIS OF COUPLING SENSITIVITY OF UN－CONVENTIONAL RESPONSES FOR DIRECTFORCE CONTROL AIRCRAFT

ＡＮＡＬＹＳＩＳＯＦＣＯＵＰＬＩＮＧＳＥＮＳＩＴＩＶＩＴＹＯＦＵＮ－ＣＯＮＶＥＮＴＩＯＮＡＬＲＥＳＰＯＮＳＥＳＦＯＲＤＩＲＥＣＴＦＯＲＣＥＣＯＮＴＲＯＬＡＩＲＣＲＡＦＴＸｕＲｕｉｊｕａｎ（Ｆａｃｕｌｔｙ５０３，ＮｏｒｔｈｗｅｓｔｅｒｎＰｏｌｙｔｅｃｈ...     

砷化镓异质外延薄膜的近红外光致发光研究

本文通过在硅衬底上用ＭＯＣＶＤ方法生长的砷化镓外延薄膜的变激发强度的近红外光致发光，研究了在液氮温度下峰值为１．１３与１．０４ｅＶ两个发光带的发光特性。     

Neutrino pair emission from the inner crust of a neutron star

It is shown that spin-orbital interaction of neutrons with clusters (nuclei or bubbles) immersed in the neutron sea of the inner crust of a neutron star can intensify substantially the neutrino pair emission (with respect to the neutrino emission in the uniform nuclear matter) at temperatures typical for the neutrino cooling epoch of the star. The neutrino pair emissivity of sub-nuclear matter is calculated both for the case when clusters are at random positions and for the case when clusters are ordered in a lattice.     

Damping of Ni-Mn-Ga epoxy resin composites

By combining the advantages of effcient damping and high mechanical properties,Ni-Mn-Ga particle composites have a very good prospect for applications in damping structure design.In this paper,a ferromagnetic shape memory alloy Ni-Mn-Ga composite is prepared.Ni-Mn-Ga particle/bisphenol-A epoxy composite cantilever beam vibration tests under a magnetic feld and without the magnetic feld are conducted to analyze the structural damping ratios n.Meanwhile,the damping characteristics of the Ni-Mn-Ga composite are studied through the axial loading-unloading method and the acoustic emission signals method.The damping coeffcient of the composite for different Ni-Mn-Ga volume fractions is obtained.The interface properties of the composite are discussed by micro examination and axial loading.The relationships between the damping of the composite and that of the component materials are discussed.The specifc damping capacity（SDC）and acoustic emission counts diagram of different specimens with different Ni-Mn-Ga volume fractions are analyzed.     

Some problems of pulsar physics or I'm madly in love with electricity

Some current topics in the theory of pulsar magnetospheres and their emission are reviewed. The mode of plasma supply and its consequences for structure of planetary and stellar magnetospheres is discussed. In the pulsar case, the plasma is supplied by electrical forces, in contrast to all other known examples. The resulting theories of particle acceleration along polar field lines are then reviewed, and the total energization of the charge separated plasma is summarized, when pair creation is absent. The effects of pair creation are reviewed using models of the resulting steady and unsteady flows, when the polar zones of the pulsar emit either electrons or ions. The application of these theories of acceleration and plasma supply to pulsars is discussed, with particular attention paid to the total amount of electron-positron plasma created and its momentum distribution. Qualitative agreement is shown between the spatial structure of the relativistically outflowing plasma described in one version of these models and the morphology of pulsar wave forms. Various aspects of radiation emission and transport are summarized, based on the polar current flow model with pair creation, and the phenomenon of marching subpulses is discussed. The corotation beaming and the relativistically expanding current sheet models for pulsar emission are also discussed briefly, and the paper concludes with a brief discussion of the relation between the theories of polar flow with pair plasma and the problem of the energization of the Crab Nebula.Proceedings of the NASA/JPL Workshop on the Physics of Planetary and Astrophysical Magnetospheres.     

Magnetic Fields in Galaxies

Radio synchrotron emission, its polarization and its Faraday rotation are powerful tools to study the strength and structure of magnetic fields in galaxies. Unpolarized emission traces turbulent fields which are strongest in spiral arms and bars (20–30?μG) and in central starburst regions (50–100?μG). Such fields are dynamically important, e.g. they can drive gas inflows in central regions. Polarized emission traces ordered fields which can be regular or anisotropic random, generated from isotropic random fields by compression or shear. The strongest ordered fields of 10–15?μG strength are generally found in interarm regions and follow the orientation of adjacent gas spiral arms. Ordered fields with spiral patterns exist in grand-design, barred and flocculent galaxies, and in central regions of starburst galaxies. Faraday rotation measures (RM) of the diffuse polarized radio emission from the disks of several spiral galaxies reveal large-scale patterns, which are signatures of regular fields generated by a mean-field dynamo. However, in most spiral galaxies observed so far the field structure is more complicated. Ordered fields in interacting galaxies have asymmetric distributions and are an excellent tracer of past interactions between galaxies or with the intergalactic medium. Ordered magnetic fields are also observed in radio halos around edge-on galaxies, out to large distances from the plane, with X-shaped patterns. Future observations of polarized emission at high frequencies, with the EVLA, the SKA and its precursors, will trace galactic magnetic fields in unprecedented detail. Low-frequency telescopes (e.g. LOFAR and MWA) are ideal to search for diffuse emission and small RMs from weak interstellar and intergalactic fields.     

Preparation and Photoluminescence of ZnO Nanostructures

Porous anodic alumina (PAA) hosts with ZnO nanoparticles loaded in were prepared by immersing PAA films in an aqueous solu-tion of zinc acetate and then annealing at high temperatures. Highly ordered ZnO nanodot arrays were produced using the method in combination of PAA template with RF magnetron sputtering deposition. The photoluminescence of the ZnO/PAA composite and the highly ordered ZnO nanodot arrays were investigated by means of a fluorescent spectrometer. The ZnO/PAA composite exhibits intense and broad photoluminescence spectra with the peak position at around 485 nm. The ZnO nanodot arrays have a strong UV light emissive peak at about 380 nm and a wide light emissive peak at 460 nm-610 nm at the room temperature.     

纳米CeO2粉体的制备及其发光性能研究

以氨水和硝酸铈为反应原料,采用沉淀滴定法制备了纳米CeO2粉体,通过XRD、SEM、TEM等手段对其进行了结构表征和形貌分析;考察了不同溶剂、煅烧温度等对其颗粒尺寸的影响;应用荧光光谱法测试了其发光光谱,首次探讨了纳米CeO2粉体的发光性能。结果表明,前驱体经过300～700℃煅烧后可以得到颗粒尺寸为4-30nm的立方萤石结构CeO2晶体,其形貌接近于球形。在无水乙醇溶剂中得到的纳米CeO2颗粒分散较好,其颗粒尺寸随煅烧温度的升高而增大。纳米CeO2粉体具有良好的蓝光发光性能,在276nm的激发波长作用下,其发射光谱的最大峰值为473nm。     

High energy X-ray spectrum of her X-1

Summary On May 8, 1980, we conducted a 90 minute observation on hard X-ray emission (15-200 keV) from Her X-1, using a large area ( 1500 cm²), low background balloon borne X-ray telescope. The energy resolution of the telescope was 17% FWHM at 60 keV. Her X-1 was at binary phase 0.0725 and 2.7 ± 0.5 days after turn on in the 35 day cycle.Average pulsation light curves were obtained by sorting data into 25 equal bins, according to pulse arrival time, modulo the 1.24 sec pulsation period. The width of the main pulse is energy dependent and in the 45–75 keV region about 30% smaller than in the range from 15 to 30 keV.The data have been analyzed by taking the Her X-1 pulse minus background spectrum, where the pulse count rate is defined in a pulse phase interval around the pulse maximum of the 1.24 sec period. The background spectrum was intermittently obtained by a chopping collimator system.A spectral feature is present in emission at an energy of 49.5 (+ 1.5, -3) keV and a FWHM of 18 (+ 6, -3) keV and in absorption at an energy of 29.5 (+ 1.7, -1.5) keV and a FWHM of 17.0 (+ 2.6, -2.8) keV. The intensity of this line feature in emission is (1.8 ± 0.4) photons/cm sec. The line excess in emission over the continuum (with kT = 6.75 (+ 0.2, -0.4) keV) is 7.     

GaInP_2外延薄膜的成份调制与超结构间的关联

用自制的具有极高分辨率的微机控制的三晶体x-射线衍射仪测量了用MOCVD方法生长的Ga_(0.52)In(0.48)P外延薄膜的超结构。我们发现,在Ga_(0.52)In(0.48)P外延薄膜内由In平面和Ga平面交替组成的(?)平面中,存在着交替的In丰与Ga丰平面。对此,我们定义了有序因子,并首先精确地测定了有序因子值。由此导出了成份调制的表达式。这样,我们就可用成份调制表示式来表达GaInP_2外延薄膜中存在的部分有序相的超结构特征。     

生长在Si上的GaAs外延膜中有关深能级缺陷与其形貌间的关联研究

由于在GaAs和Si单晶材料间有着很大的格子常数及线性热膨胀系数差别，所以在St上生长的GaAs异质外延薄膜（GaAs／Si）中会存在着界面失配形变与高密度的结构缺陷。我们的实验显示，GaAs／Si外延膜的无序与其生长条件有关，尤其与其［As］／［Ga］比密切相关。与GaAs／Si无序相关的失配位错、线位错及畴区的形貌已用扫描电子显微镜作了观察;与深能级相关的缺陷与其形貌间的关联也已用实验说明。对于高有序GaAs／Si外延膜来说，其与离域相关的主发光峰的强度对温度的变化服从阿兰纽斯方程，而对低有序的GaAs／Si外延膜来说，其与局域相关的主发光峰的强度对温度的变化关系则遵循对无定型半导体才成立的另一种方程。