共查询到20条相似文献，搜索用时 46 毫秒
1.
陈有君 《内蒙古农业大学学报(自然科学版)》2003,24(1):79-86
对运动电磁场的电场强度变量和磁感应强度变量做旋度及散度运算分析，表明除电位移变量项与经典Mexwell方程组的正负号不同外，大多数时变电磁场理论下的Maxwell方程都可以在一定条件下从运动电磁场的Maxweel方程组中导出。但在有些条件下运动电磁场的Maxwell创方程组仍然可以应用，并能得到正确的结果，而经典Maxwell方程组无法应用。这说明用“运动电场具有磁场特性；运动磁场具有电场特性”来描述电场与磁场之间的关系要比时变电磁场理论更符合自然规律。时变电磁场理论的Maxwell方程组是运动电磁场在特殊条件下的特殊形式。所谓时变电磁场可能是运动电磁场在特殊条件下的特殊表现，时变电场与时变磁场之间的相互转化可能是运动电磁场在特殊条件下所表现出的假象，并非电磁场的真正规律。时变电磁场理论的Maxwell方程组作为数学工具在一些领域中可以应用，但作为原理表达式，它们不是每个都正确的，也不是总对的。 相似文献
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陈有君 《内蒙古农业大学学报(自然科学版)》2001,22(4):105-111
综合经典电磁学中关于电与磁联系的基本实验定律及理论,经推导和分析得出电场与磁场的联系是运动磁场具有或表现出电场的特性,当一个具有磁感应强度为B的场,以速度V运动时,这个场的电场强度为E=B×VB.磁场的时变必然是由于磁场的运动所至,而运动的磁场具有电场的性质,因此所谓时变磁场产生电场只不过是运动磁场具有电场特性这一自然规律在特定条件下的一种表现.经典电磁学中把磁场分为静磁场和时变磁场是不合理的.因为与静止相应的是运动而不是时变.磁场的时变和磁场的电特性是伴生关系,而非因果关系,它们都是磁场运动的结果.所以时变磁场产生电场或者Faraday-Lenz定律不是一个普适的自然规律.但在有些条件下,运动磁场和其电场特性之间在数量上确实满足Faraday-Lenz定律,因此,作为一个从实验中总结出的规律,并有一定的理论根据,它可以在一些领域中作为数学工具用. 相似文献
3.
Fluctuations are important near phase transitions, where they can be difficult to describe quantitatively. Superconductivity in mesoscopic rings is particularly intriguing because the critical temperature is an oscillatory function of magnetic field. There is an exact theory for thermal fluctuations in one-dimensional superconducting rings, which are therefore expected to be an excellent model system. We measured the susceptibility of many rings, one ring at a time, by using a scanning superconducting quantum interference device that can isolate magnetic signals that are seven orders of magnitude smaller than applied flux. We find that the fluctuation theory describes the results and that a single parameter characterizes the ways in which the fluctuations are especially important at magnetic fields where the critical temperature is suppressed. 相似文献
4.
陈有君 《内蒙古农业大学学报(自然科学版)》2002,23(1):91-97
Biot-Savart定律是经典电磁学中关于电流的磁场的基本定律,以它为基础,并结合分析经典电磁学中关于磁与电关系的理论,推导出了磁场与电场联系的规律,即运动电场具有磁场特性.磁感应强度与电场强度之间具有如下关系B=(1)/(C2)(VE×E)电流的磁场是电流周围运动电场的特性,在传导电流的周围,由于正负电荷的电场强度相等,方向相反而抵消,所以没有明显的电场,但是随电荷运动的电场潜流,相反方向的电场的运动方向相反,因此向量VE×E却是不平衡的,这个向量就是传导电流的磁场.即电流只是磁场的表面的源,磁场的源是运动的电场或运动的电荷.磁场与电场及运动速度之间是互相垂直的三维向量.电场的时变也是由于运动造成的,所以时变电场引起的磁场也是由电场的运动造成的.时变电场产生磁场不是电磁现象的一般规律. 相似文献
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Hey AJ Merlin JH Ricketts MW Vaughn MT Williams DC 《Science (New York, N.Y.)》1988,240(4856):1163-1168
A diverse range of physical phenomena, both observed and hypothetical, are described by topological solutions to nonlinear gauge field theories. Computer-generated color graphic displays can provide a clear and detailed representation of some of these solutions, which might otherwise be physically unintelligible because of their mathematical complexity. Graphical representations are presented here for two topological solutions: (i) the solutions of a model that represents the filaments of quantized magnetic flux in a superconductor, and (ii) the solutions of an SO(3) gauge theory corresponding to a pair of separated magnetic monopoles. An introduction is provided to the gauge field theories giving rise to these solutions. 相似文献
8.
磁处理对原油结蜡影响的机理分析 总被引：2，自引：0，他引：2
分析了磁处理对原油结蜡的影响因素,用石油胶体分散体系理论分析了原油结蜡过程,应用胶体化学中的"DLVO理论"解释了磁处理对原油结蜡的影响.分析认为,磁场通过对蜡晶分子间色散力的影响作用,致使蜡晶胶粒之间的范德华引力势能增大,从而促进了原油中蜡晶胶粒的聚结,这就是磁处理对原油凝胶结构产生影响从而降粘的基本原因. 相似文献
9.
为了探求磁处理技术防垢的机理，应用电学与统计力学的理论和数学分析的方法。对电解质内胶态粒子周围的电荷分布进行了研究，计算了磁场对这种电荷分布的影响，给出了在温度较高及稀溶液情况下磁场对胶态粒子周围电荷分布影响的公式。认为电解质内的胶态粒子周围带有一层离子电荷，其厚度取决于温度与离子的浓度。当离子浓度离子大时，离子层变薄，促使胶粒之间发生凝聚；当温度增高时，离子层变厚，阻碍胶粒之间发生凝聚。当电解质 相似文献
10.
Heyner D Wicht J Gómez-Pérez N Schmitt D Auster HU Glassmeier KH 《Science (New York, N.Y.)》2011,334(6063):1690-1693
The observed weakness of Mercury's magnetic field poses a long-standing puzzle to dynamo theory. Using numerical dynamo simulations, we show that it could be explained by a negative feedback between the magnetospheric and the internal magnetic fields. Without feedback, a small internal field was amplified by the dynamo process up to Earth-like values. With feedback, the field strength saturated at a much lower level, compatible with the observations at Mercury. The classical saturation mechanism via the Lorentz force was replaced by the external field impact. The resulting surface field was dominated by uneven harmonic components. This will allow the feedback model to be distinguished from other models once a more accurate field model is constructed from MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) and BepiColombo data. 相似文献
11.
利用等效介质理论，在考虑磁性层表面动力学退磁场影响的前提下，首先给出了动力学磁化率，然后求出了色散方程。当坐标系的，轴垂直于层间界面，饱和磁化和外场均沿z轴方向时，数值计算结果表明：表面静磁波可以在任意磁性层的相对厚度时存在，同时表面波的传播方向处在x-z平面的第三和第四象限中。这两结论与以往的结果不同。体静磁模频率的连续区在表面模频率的上方。 相似文献
12.
过渡金属配合物的配位场理论克服了价键理论的某些局限性 ,阐明了配位体对中心离子的 d轨道影响。能定性的和定量的说明配合物的空间模型、稳定性、磁性及其能量变化 ,得到了广泛的应用 相似文献
13.
Gaensler BM Haverkorn M Staveley-Smith L Dickey JM McClure-Griffiths NM Dickel JR Wolleben M 《Science (New York, N.Y.)》2005,307(5715):1610-1612
We have measured the Faraday rotation toward a large sample of polarized radio sources behind the Large Magellanic Cloud (LMC) to determine the structure of this galaxy's magnetic field. The magnetic field of the LMC consists of a coherent axisymmetric spiral of field strength approximately 1 microgauss. Strong fluctuations in the magnetic field are also seen on small (<0.5 parsec) and large (approximately 100 parsecs) scales. The large bursts of recent star formation and supernova activity in the LMC argue against standard dynamo theory, adding to the growing evidence for rapid field amplification in galaxies. 相似文献
14.
Kivelson MG Bargatze LF Khurana KK Southwood DJ Walker RJ Coleman PJ 《Science (New York, N.Y.)》1993,261(5119):331-334
Two large magnetic field rotations were recorded by the spacecraft Galileo 1 minute before and 2 minutes after its closest approach to the asteroid Gaspra. The timing and the geometry of the field changes suggest a connection with Gaspra, and the events can be interpreted as the result of the draping of the solar wind field around a magnetospheric obstacle. Gaspra's surface field is inferred to be within an order of magnitude of Earth's surface field, and its magnetic moment per unit mass is in the range observed for iron meteorites and highly magnetized chondrites. The location of the magnetic signatures suggests that perturbations are carried by waves in the magnetosonic-whistler mode with wavelengths between electron and ion gyro radii. 相似文献
15.
The ocean is an electrically conducting fluid that generates secondary magnetic fields as it flows through Earth's main magnetic field. Extracting ocean flow signals from remote observations has become possible with the current generation of satellites measuring Earth's magnetic field. Here, we consider the magnetic fields generated by the ocean lunar semidiurnal (M2) tide and demonstrate that magnetic fields of oceanic origin can be clearly identified in satellite observations. 相似文献
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Mars' crustal magnetic field was most likely generated by dynamo action in the planet's early history. Unexplained characteristics of the field include its strength, concentration in the southern hemisphere, and lack of correlation with any surface features except for the hemispheric crustal dichotomy. We used numerical dynamo modeling to demonstrate that the mechanisms proposed to explain crustal dichotomy formation can result in a single-hemisphere dynamo. This dynamo produces strong magnetic fields in only the southern hemisphere. This magnetic field morphology can explain why Mars' crustal magnetic field intensities are substantially stronger in the southern hemisphere without relying on any postdynamo mechanisms. 相似文献
17.
Lunar-modulated geomagnetic orientation by a marine mollusk 总被引：4，自引：0，他引：4
Behavioral experiments indicated that the marine opisthobranch mollusk Tritonia diomedea can derive directional cues from the magnetic field of the earth. The magnetic direction toward which nudibranchs spontaneously oriented in the geomagnetic field showed recurring patterns of variation correlated with lunar phase, suggesting that the behavioral response to magnetism is modulated by a circa-lunar rhythm. The discovery of a magnetic sense in a mollusk with giant, reidentifiable neurons provides a unique opportunity to study the cellular mechanisms underlying magnetic field detection. 相似文献
18.
对3种不同的水在搅拌状态下磁化,结果表明:水的表面张力系数和粘度随磁感应强度和磁化时间均呈现多极值增减变化关系。原因是水分子在磁场作用下获得能量的同时,电子云的空间分布及其磁矩的取向均发生变化,磁感应强度和磁化时间取不同的值可以满足水中氢键形成和断裂的条件,从而导致水的物理性质变化。分析实验结果,得出了减小水的表面张力和粘度的最佳磁化条件。 相似文献
19.
Buffett BA 《Science (New York, N.Y.)》2000,288(5473):2007-2012
Earth's magnetic field is generated by fluid motion in the liquid iron core. Details of how this occurs are now emerging from numerical simulations that achieve a self-sustaining magnetic field. Early results predict a dominant dipole field outside the core, and some models even reproduce magnetic reversals. The simulations also show how different patterns of flow can produce similar external fields. Efforts to distinguish between the various possibilities appeal to observations of the time-dependent behavior of the field. Important constraints will come from geological records of the magnetic field in the past. 相似文献
20.
The Moon possesses strong magnetic anomalies that are enigmatic given the weak magnetism of lunar rocks. We show that the most prominent grouping of anomalies can be explained by highly magnetic extralunar materials from the projectile that formed the largest and oldest impact crater on the Moon: the South Pole-Aitken basin. The distribution of projectile materials from a model oblique impact coincides with the distribution of magnetic anomalies surrounding this basin, and the magnetic properties of these materials can account for the intensity of the observed anomalies if they were magnetized in a core dynamo field. Distal ejecta from this event can explain the origin of isolated magnetic anomalies far from this basin. 相似文献