83 resultados para TILTED MAGNETIC-FIELDS
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A numerical analysis of an electron waveguide coupler based on two quantum wires coupled by a magnetically defined barrier is presented with the use of the scattering-matrix method. For different geometry parameters and magnetic fields, tunneling transmission spectrum is obtained as a function of the electron energy. Different from that of conventional electron waveguide couplers, the transmission spectrum of the magnetically coupled quantum wires does not have the symmetry with regard to those geometrically symmetrical ports, It was found that the magnetic field in the coupling region drastically enhances the coupling between the two quantum wires for one specific input port while it weakens the coupling for the other input port. The results can be well understood by the formation of the edge states in the magnetically defined barrier region. Thus, whether these edge states couple or decouple to the electronic propagation modes in the two quantum wires, strongly depend on the relative moving directions of electrons in the propagating mode in the input port and the edge states in the magnetic region. This leads to a big difference in transmission coefficients between two quantum wires when injecting electrons via different input ports. Two important coupler specifications, the directivity and uniformity, are calculated which show that the system we considered behaves as a good quantum directional coupler. (C) 1997 American Institute of Physics.
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The magnetocapacitive response of a double-barrier structure (DBS), biased beyond resonances, has been employed to determine the density of states (DOS) of the two-dimensional electron gas residing in the accumulation layer on the incident side of the DBS. An adequate procedure is developed to compare the model calculation of the magnetocapacitance with the experimental C vs B curves measured at different temperatures and biases. The results show that the fitting is not only self-consistent but also remarkably good even in well-defined quantum Hall regimes. As a result, information about the DOS in strong magnetic fields could reliably be extracted.
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We report on high magnetic fields (up to 40 T) cyclotron resonance, quantum Hall effect and Shubnikov-de-Hass measurements in high frequency transistors based on Si-doped GaN-AlGaN heterojunctions. A simple way of precise modelling of the cyclotron absorption in these heterojunctions is presented, We clearly establish two-dimensional electrons to be the dominant conducting carriers and determine precisely their in-plane effective mass to be 0.230 +/- 0.005 of the free electron effective mass. The increase of the effective mass with an increase of two-dimensional carrier density is observed and explained by the nonparabolicity effect. (C) 1997 American Institute of Physics.
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The magnetotransport properties of the two-dimensional (2D) electron gas confined in a modulation-doped Zn0.80Cd0.20Se/ZnS0.06Se0.94 single quantum well structure were studied at temperatures down to 0.35 K in magnetic fields up to 7.5 T. Well resolved 2D Shubnikovde Haas (SdH) oscillations were observed, although the conductivity of the sample in the as grown state was dominated by a bulk parallel conduction layer. After removing most of the parallel conduction layer by wet chemical etching the amplitude and number of SdH oscillations increased. From the temperature dependence of the amplitude the effective mass of the electrons was estimated as 0.17 m(0). Copyright (C) 1996 Published by Elsevier Science Ltd
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The cyclotron resonance (CR) of electrons in GaAs/AlGaAs quantum wells is investigated theoretically to explain a recent CR experiment, where two CR peaks were observed at high magnetic fields when both spin-up and spin-down states of the lowest Landau level are occupied. Our theoretical model takes into account the conduction band non-parabolicity, the electron bulk longitude-optic-phonon coupling, and the self-consistent subband structure. A good agreement is found.
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A systematic study of electron cyclotron resonance (CR) in two sets of GaAs/Al0.3Ga0.7As modulation-doped quantum-well samples (well widths between 12 and 24 nm) has been carried out in magnetic fields up to 30 T. Polaron CR is the dominant transition in the region of GaAs optical phonons for the set of lightly doped samples, and the results are in good agreement with calculations that include the interaction with interface optical phonons. The results from the heavily doped set are markedly different. At low magnetic fields (below the GaAs reststrahlen region), all three samples exhibit almost identical CR which shows little effect of the polaron interaction due to screening and Pauli-principle effects. Above the GaAs LO-phonon region (B > similar to 23 T), the three samples behave very differently. For the most lightly doped sample (3 x 10(11) cm(-2)) only one transition minimum is observed, which can be explained as screened polaron CR. A sample of intermediate density (6 x 10(11) cm(-2)) shows two lines above 23 T; the higher frequency branch is indistinguishable from the positions of the single line of the low density sample. For the most heavily, doped sample (1.2 x 10(12) cm(-2)) there is no evidence of high frequency resonance, and the strong, single line observed is indistinguishable from the lower branch observed from sample with intermediate doping density. We suggest that the low frequency branch in our experiment is a magnetoplasmon resonance red-shifted by disorder, and the upper branch is single-particle-like screened polaron CR. (C) 1998 Elsevier Science B.V. All rights reserved.
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Electron transport in heavily-doped GaAs/AlAs superlattices in parallel electric and magnetic fields is reported. The current-voltage (I-V) characteristic exhibited the feature of negative differential velocity (NDV) and high electric field domain effect at different biases. Under strong magnetic fields, sequential resonant tunnelling through Landau levels in the negative differential velocity regime is observed, which are manifested as oscillations in the conductance-voltage characteristics. (C) 1998 Elsevier Science B.V. All rights reserved.
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In 0.15T and 0.35T(Tesla) magnetic fields, soil breathing intensity, activities of invertase and phosphatase were improved, but activity of urease was inhibited. After applying magnetized coal ash to red soil, the rate of germination of Sudan grass was increased, growth of seedlings was speeded up, and activity of polyphenol oxidase was decreased.
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1 初级视觉皮层功能,GABA系统功能在衰老过程中的变化 本章首先对衰老过程中神经形态学和神经电生理学上的研究进行了综述,然后报道了作者的博士学位论文研究工作。实验采用神经电生理的手段,探讨初级视觉皮层(primary visual cortex;V1)功能,以及GABA(gamma-aminobutyric acid)系统功能在衰老过程中的变化。 实验1和2均采用单细胞记录技术,检测了中年猴V1细胞的方位选择性、方向选择性、自发放和最大反应,并与年轻和老年猴进行对比;比较了年轻和老年猴V1细胞的感受野外周抑制能力。在实验3中,我们记录了年轻和中年大鼠在给予GABA直接或间接的激动剂,戊巴比妥钠或氯胺酮{通过拮抗NMDA(N-methyl-D-aspartate)受体}后,其皮层的EEG(electroencephalogram)活动,并分析与年龄相关的差异。结果如下: 实验1:中年猴V1细胞的方向选择性和自发放介于年轻猴和老年猴之间,而方位选择性和最大反应与年龄之间没有相关性。 实验2:感受野外周区的最优刺激明显降低了年轻和老年猴具有高方位选择性细胞的比例。同时,年轻猴所有细胞,以及老年猴高方位选择性细胞具有较高的最大抑制比,与它们相比,老年猴无明显方位偏好细胞的最大抑制比显著降低; 实验3:戊巴比妥钠注射后,在年轻和中年大鼠上,alpha (8-12 Hz) 和beta (12-20 Hz) 频段EEG功率增加,theta (4-8 Hz) 功率减少,这些变化在中年大鼠上较为明显。氯胺酮注射后,中年大鼠theta功率比年轻大鼠具有更大幅度的降低。 我们的结果表明,视觉皮层功能的下调在衰老早期就已发生,其机制可能与抑制系统功能普遍降低有关. 2 奖赏机制,极低频磁场的生物学效应研究 本章首先对自然奖赏和药物成瘾机制、极低频磁场生物学效应,以及极低频磁场对奖赏系统的影响进行了综述,然后报道了作者的博士论文研究工作。实验目的是探讨大鼠眶额叶皮质(orbitofrontal cortex;OFC)活动与食物奖赏刺激的相关性,以及极低频磁场对小鼠空间认知能力的影响。 实验1采用EEG记录技术,检测了大鼠OFC在食物奖赏和渴求过程中EEG各频段的功率变化。在实验2中,使用了一种探索型Y-迷宫实验范式,它仅依赖于啮齿类动物天生的探索欲望,避免了奖赏效应的干扰,利用此新型迷宫,我们检测了25和50 Hz磁场对小鼠空间识别记忆能力的影响。其结果如下: 实验1:大鼠OFC的delta频段(2-4 Hz)EEG活动与食物刺激显著相关,其相对功率在食物渴求时下降,在食物奖赏时升高。 实验2:与短时照射相比,长时的50 Hz磁场照射降低了小鼠对新异臂的探索能力,而25和50 Hz磁场暴露都不影响小鼠的活动力。 本研究表明,食物奖赏与OFC的delta频段EEG活动密切相关,而我们以前发现,大鼠和猴OFC的gamma(20-100 Hz)活动与吗啡成瘾相关,提示了OFC在自然奖赏和药物成瘾中具有不同的作用;另外,本实验首次证明,极低频磁场损害了小鼠不依赖于奖赏系统的空间认知能力,而我们先前发现,极低频磁场可以强化吗啡诱导的条件化位置偏好,从而说明极低频磁场对吗啡成瘾具有独特的生物学效应。
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1.老年猴视皮层神经元对图形对比度的反应及潜伏期特征: 在正常衰老过程中人类的视觉功能受到严重影响,例如空间和时间对比度敏感性下降以及信息处理时间的延长。虽然部分视觉功能的退化与眼睛的光学系统老化有关,但是它并不能解释所有视觉功能的下降。此外,我们以前的研究和别人的研究结果都表明衰老过程中视觉中枢系统功能的改变可能是视觉功能下降的主要原因。因此,利用单位放电记录技术(single-unit recording technique),我们比较了年轻猕猴和老年猕猴的初级视觉皮层(primary visual cortex,又称V1)神经元对比度反应之间的差异,以及V1和内侧颞叶(medial temporal cortex,MT)视觉区神经元反应潜伏期及其变异性之间的差异。结果显示,与年轻猴相比,老年猴V1区神经元对比度敏感性降低,同时伴随着神经元活动信噪比下降;老年猴V1区和MT区神经元反应潜伏期及其变异性显著增加。然而,两个年龄组MT区神经元平均潜伏期之间差异小于V1区神经元平均潜伏期之间的差异,说明MT区神经元能够自我调整老化带来的影响。另外,两个年龄组V1区神经元潜伏期和变异性都具有正相关关系,但是MT区神经元则没有这种相关性。这些结果表明,在老化过程中皮层神经元的对比度和潜伏期反应特性发生了改变。我们推测这种改变可能与视觉皮层内抑制系统功能的降低有关,但是具体的分子机制和神经环路还不清楚。总之,本实验的研究结果为更好的理解老年人在视觉信息处理中时间和空间对比度敏感性及处理速度下降提供了新线索。2.极低频磁场对脑功能的影响及眶额叶认知功能的研究: 实验目的:(1)研究极低频磁场(20 Hz, 14 mT)照射对长期吗啡处理引起的大鼠背侧海马神经元多巴胺D2密度降低的影响;(2)小鼠青春期长期极低频磁场(50 Hz, 2 mT)照射对空间学习记忆的影响;(3)初步探讨了眶额叶在大鼠新异性探索行为中的作用。实验1,我们用免疫组化的方法检测了大鼠背侧海马神经元多巴胺D2受体密度的变化。结果显示,在长期吗啡处理后戒断早期背侧海马神经元多巴胺D2受体密度相对于对照组减少,磁场和吗啡共同作用会强化这种适应,但是这种变化很快恢复正常。这些结果表明长期吗啡处理会引起海马多巴胺系统产生适应;磁场强化了长期吗啡处理对背侧海马多巴胺系统的影响,这为我们先前发现磁场照射延缓了大鼠条件位置偏好消退的研究结果提供了一个内在神经基础。实验2,我们分别用Y-迷宫(two-trial Y-maze)和Morris水迷宫两种行为装置研究了青春期早期磁场暴露对小鼠短时空间识别记忆和长时空间参考记忆的影响。结果显示,磁场暴露并没有影响小鼠Y-迷宫作业,但是提高了水迷宫任务的学习以及记忆保持。这些结果表明磁场对空间记忆的影响是任务依赖性的。实验3,我们用旷场和Y-迷宫两种行为装置研究了眶额叶电损伤对大鼠新异性探索行为的影响。结果显示,眶额叶受损并没有影响大鼠的神经运动能力,但是降低了大鼠在旷场中的行走距离和直立次数以及降低了在Y-迷宫新异臂中的探索时间和穿梭次数。这些结果表明,眶额叶的完整性对大鼠探索新异环境行为是必要的,这可能与眶额叶参与记忆或行为决策功能有关。
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C-13 and H-1 relaxation times were measured as a function of temperature in two magnetic fields for dilute solutions of phenolphthalein poly(ether sulfone) (PES-C) in deuterated chloroform. The spin-lattice relaxation times were interpreted in terms of segmental motion characterized by the sharp cutoff model of Jones and Stockmayer (J. S. model). The phenyl group rotation is treated as a stochastic diffusion by the J. S. model. The restricted butterfly motion of the phenyl group attached to the cardo ring in PES-C is mentioned but is not discussed in detail in this work. Correlation times for the segmental motion are in the picosecond range which indicates the high flexibility of PES-C chains. The correlation time for the phenyl group internal rotation is similar to that of the segmental motion. The temperature dependence of these motions is weak. The apparent activation energy of the motions considered is less than 10 kJ/mol. The simulating results for PES are also reasonable considering the differences in structure compared with PES-C. The correlation times and the apparent activation energy obtained using the J. S. model for the main chain motion of PES-C are the same as those obtained using the damped orientational diffusion model and the conformational jump model.
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Magnetic storm is a kind of severe disturbances in the whole solar-earth electromagnetic space. It has significant effects on communication, electric power, oil transport pipe and human activities in space. Therefore, magnetic storms are worth for applications systems, not only being a favorable issue for scientists. In this paper, the spatial and temporal distributions of the magnetic fields produced by the magnetosphere-ionosphere current systems during storms are studied. Four parts are included in this paper decomposion of different disturbances with different origins, topological structure of the ring current, the asymmetric characteristics of the ring current, and the statistic peculiarities of the day-to-day variability (DTD) of Sq. 1 The decomposition of magnetic disturbances at mid-low latitudes and its evolutions during storms Transient variations in the geomagnetic field recorded at mid-low latitudes mainly include the storm-time variation (Dst), solar quiet daily variation (Sq) and disturbance daily variation (SD). With the data of the geomagnetic meridian chain observatories in China, 25 storms during the period of 1997 to 1999 have been analyzed. According to the features of different variations, a method of “three-steps decomposition” is developed by using the method of Natural Orthogonal Components (NOC), Correlation Analysis and Fourier Analysis to separate those three components in turn. The results show that, the first eigenmode by the MNOC clearly describing the special distribution and temporal evolution of storm-time variation, in addition, Correlation Analysis and Fourier Analysis offer a useful method to extract the Sq and SD variations. The latitudinal shift of the Sq current focus seems to be the principal reason of the day-to-day variaitons in the daily range of Sq. The magnitude of SD reaches a maximum during the main phase, and then gradually decreases. 2 The topology structure of the ring current during storms Both the mechanism of the ring current and the geomagnetic data suggest that the central plane of the ring current is declining to the geomagnetic equator plane with a tilt angle δ. Using the H and Z component data at two stations in a meridian chain, we deduce a new parameter describing the invariable peculiarity of different storms. Then the δ angle is calculated by using the data from a meridian chain and tested with the ERC model. Finally the deduced tilt angles are used to modify Dst index. 3 The asymmetric characteristics of the ring current during storms The variations of the geomagnetic field at mid-low latitudes show a significant dawn-dusk asymmetry, resulting from the superposition of the fields from the symmetric ring current and the partial ring current. On the basis of the data from the 20°E, 30°E meridian chains and 30°N latitudinal chain, the dawn-dusk asymmetry is investigated by using three methods, namely, statistic analysis, ring current model calculation and typical event analysis. This characteristic implies the asymmetry of the spatial distribution of the ring current. In addition, during the main phase after the sudden commencement (SC), H field increases and reaches maximum around noontime, implying the effect of the Chapman-Ferraro current. 4 The statistic characteristics of the day-to-day variability and its mechanism The day-to-day variability of the geomagnetic Sq field is studied by using the magnetic data from a meridian chain of magnetometers along 120° E longitude. The method of NOC is applied to separate the Sq variation from complicated disturbances. The first eigenmode with the largest eigenvalue represents fairly well the Sq variation with a conspicuous day-to-day variability in the daily range. For the stations on the same north- or south-side of the Sq current system focus, the day-to-day variations show a positive correlation. In contrast, for the stations on the different sides of the Sq focus, they show a negative correlation, suggesting an important role of latitudinal shift of the Sq current system focus to the day-to-day variability of the Sq daily range. The Sq daily range is correlated with the magnetic indices Ap and Dst in a peculiar way: on some severe disturbed days, noticeably enhancements of the Sq are observed, implying increases of the ionospheric conductivities and/or tidal wind velocities; on other severe disturbed days, however, dramatically reduced Sq variations occur, suggesting dominant effects of the ‘disturbance dynamo’ process.
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A frequency domain electromagnetic (conductivity) method for near surface soundings at low frequencies is discussed in this thesis. Its elementary principle is to detect the conductivity of the earth by the secondary magnetic fields induced by a current dipole on the earth. According to the EM induction theory, a coil with alternating current on the earth will generate a magnetic field in whole space which is referred to as the primary field Hp. The primary field would induce secondary currents in the earth which go down to depth like a batch of smoking rings. These currents further produce secondary magnetic field Hs .The primary and secondary magnetic fields are collected together by a receiver coil. Generally speaking,the secondary magnetic field is a complicated function of coil spacing, transmitting frequency and earth conductivity. But at low induction numbers, the secondary field is deduced to as a simple function of frequency, spacing and conductivity. Especially the ratio of secondary to primary field shares a linear proportion to the apparent conductivity. The earth conductivity can be interpreted by proper inversions with the apparent conductivity. The method is discussed at three steps: (1)Derivation of primary and secondary magnetic fields arising from vertical and horizontal magnetic dipoles on the earth based on the basic EM induction theory. (2)Field techniques and equipment developed for the method. (3)An interpretation technique was introduced using a cumulative and relative response function. Finally a test example is presented for examining the effectiveness of the method.
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Using the approach of local expansion, we analyze the magnetostatic relations in the case of conventional turbulence. The turbulent relations are obtained consisten tly for themomentum equation and induction equation of both the average and fluctuation relations.In comparison with the magnetostatic relations as discussed usually, turbulent fluctuationfields produce forces, one of which 1/(4π)(α1×B0)×B0 may have parallel and perpendicular components in the direction of magnetic field, the other of which 1/(4π)K×B0 is introduced by the boundary value of turbulence and is perpendicular to the magnetic field. In the case of 2-dimensional configuration of magnetic field, the basic equation will be reduced into a second-order elliptic equation, which includes some linear and nonlinear terms introduced by turbulent fluctuation fields. Turbulent fields may change the configuration of magnetic field and even shear it non-uniformly. The study on the influence of turbulent fields is significant since they are observed in many astrophysical environments.
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As an improvement of resolution of observations, more and more radio galaxies with radiojets have been identified and many fine structures in the radio jets yielded. In the presentpaper, the two-dimensional magnetohydrodynamical theory is applied to the analysis of themagnetic field configurations in the radio jefs. Two-dimensional results not only are con-sistent theoretically, but also explain the fine structures of observations. One of the theo-retical models is discussed in detail, and is in good agreement as compared with the observedradio jets of NGC6251. The results of the present paper also show that the magneticfields in the radio jets are mainly longitudinal ones and associate with the double sources ofQSOs if the magnetic field of the central object is stronger; the fields in the radio jets aremainly transverse ones and associate with the double sources of radio galaxies if the fieldof the central object is weaker. The magnetic field has great influence on the morphol-ogy and dynamic process.