共查询到20条相似文献,搜索用时 15 毫秒
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The simplest type of dune is the transverse one, which propagates with invariant profile orthogonally to a fixed wind direction. Here we show, by means of numerical simulations, that transverse dunes are unstable with respect to along-axis perturbations in their profile and decay on the bedrock into barchan dunes. Any forcing modulation amplifies exponentially with growth rate determined by the dune turnover time. We estimate the distance covered by a transverse dune before fully decaying into barchans and identify the patterns produced by different types of perturbation. 相似文献
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利用corner transport upwind和constrained transport算法求解非理想磁流体动力学方程组,对匀强平行磁场作用下,黏性各向异性等离子体自由剪切层中的Kelvin-Helmholtz不稳定性进行了数值模拟.从流动结构、涡结构演化、磁场分布、横向磁压力、抗弯磁张力等角度对各向同性和各向异性黏性算例结果进行了讨论,分析了黏性各向异性对Kelvin-Helmholtz不稳定性的影响.结果表明,黏性各向异性比黏性各向同性更利于流动的稳定.其稳定性作用是由于磁感线方向上剪切速率降低导致界面卷起程度和圈数的降低,并使卷起结构中小涡产生增殖、合并,破坏了涡的常规增长,从而导致流动的稳定.黏性各向异性对横向磁压力的影响比对抗弯磁张力更大. 相似文献
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A drift-kinetic theory for ion phase-space vortices in magnetized plasmas is developed, taking into account the effects of the ion polarization and anisotropic heating by ion beams. It provides a theoretical explanation for the bipolar electrostatic structures in the auroral zone of the Earth's magnetosphere and their spatial and temporal scales, as observed by S3-3, Viking, FREJA, Polar, and FAST spacecrafts. Several types of quasi-three-dimensional ion holes are obtained analytically, in the form of either cylinders or ellipsoids. Although topologically different, they produce similar signals on the spacecraft and cannot be distinguished on the basis of the existing satellite data. 相似文献
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A regime in which a uniformly magnetized plasma does not maximize the entropy and possibly becomes unstable to a spatial perturbation in the magnetic field is explored. The physical implication is considered in the context of current generation, magnetic field reconnection, and the dynamo effect. 相似文献
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The possibility of cyclotron maser cooling of the transverse motion of electrons in a beam with the oblate velocity distribution characteristic of the setups with electron cooling has been analyzed. 相似文献
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V. V. Skobelev 《Journal of Experimental and Theoretical Physics》2011,113(5):791-797
The Fermi energy, pressure, internal energy, entropy, and heat capacity of completely degenerate relativistic electron gas
are calculated by numerical methods. It is shown that the maximum admissible magnetic field on the order of 109 G in white dwarfs increases the pressure by a factor of 1.06 in the central region, where the electron concentration is ∼1033 cm−3, while the equilibrium radius increases by approximately a factor of 1.03, which obviously cannot be observed experimentally.
A magnetic field of ∼108 G or lower has no effect on the pressure and other thermodynamic functions. It is also shown that the contribution of degenerate
electron gas to the total pressure in neutron stars is negligible compared to that of neutron gas even in magnetic fields
with a maximum induction ∼1017 G possible in neutron stars. The neutron beta-decay forbiddeness conditions in a superstrong magnetic field are formulated.
It is assumed that small neutron stars have such magnetic fields and that pulsars with small periods are the most probable
objects that can have super-strong magnetic fields. 相似文献
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采用洛伦兹变换推导出左旋椭圆偏振强激光在磁化等离子体中的非线性色散关系,根据Karpman方法推导出激光场包络的非线性控制方程,分析了在磁化等离子体中左旋椭圆偏振激光的调制不稳定性,得到了调制不稳定的时间增长率。分析结果表明,磁化等离子体中自调制不稳定的极大增长率较非磁化情况明显减小,且在激光等离子体临界面附近处调制不稳定性的时间增长率显著增大。 相似文献
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采用洛伦兹变换推导出左旋椭圆偏振强激光在磁化等离子体中的非线性色散关系,根据Karpman方法推导出激光场包络的非线性控制方程,分析了在磁化等离子体中左旋椭圆偏振激光的调制不稳定性,得到了调制不稳定的时间增长率。分析结果表明,磁化等离子体中自调制不稳定的极大增长率较非磁化情况明显减小,且在激光等离子体临界面附近处调制不稳定性的时间增长率显著增大。 相似文献
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Using the quantum hydrodynamic (QHD) equations with magnetic field on the Wigner-Maxwell system, the general dielectric tensor and dispersion equation for quantum plasmas were derived. Dispersion relations of one-, two-stream and beam-plasma instabilities in uniform quantum magnetized plasmas are investigated through the new dielectric tensor. The magnetic field which is parallel to the fluid velocity does not work on stream instabilities. The quantum and thermal effects have remarkable impact on two-stream instability. The critical wave number for beam-plasma instability with quantum effects correction is given too. 相似文献
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Modulation instability of an intense right-hand elliptically polarized laser beam propagating through magnetized plasma is investigated by a new method. The nonlinear dispersion relation, in which the relativistic and ponderomotive nonlinearities are taken into account, is obtained for the laser radiation in magnetized plasma by the Lorentz transformation. The Karpman equation is firstly generalized to the case of three dimensions with three field components. When the nonlinear frequency shift of the electromagnetic field in plasma is involved, the nonlinear evolution equation for the slowly varying envelope of the laser field is obtained. Thus, modulation instability of the intense laser beam in magnetized plasma is studied and the temporal growth rate of the instability is derived. The analysis shows that the peak growth rate of self-modulation instability is increased due to the axial magnetization of plasma. It is also shown that the growth rate of modulation instability is increased significantly near the critical surface in a laser-plasma. 相似文献
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The spin effects on electromagnetic waves in a strongly magnetized plasma with rare collisions are considered with the help of relativistic kinetic equations, which take into account the electron spin dynamics in self-consistent electric and magnetic fields. The growth rate of the electromagnetic spin waves in the presence of intense quasi-monoenergetic fluxes of neutrinos is determined. 相似文献
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《Physics letters. A》1987,121(4):178-181
A simulation of electron beam interaction with a magnetized plasma is presented. Fast relaxation to a plateau state takes place. The parameters of the plateau are estimated. 相似文献
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G. A. Shul’man 《Russian Physics Journal》1997,40(2):129-133
For a nondegenerate nonrelativistic electron system, taking account of the minimum of its total energy, the population of
the Landau electron levels by electrons with intrinsic magnetic moments parallel and antiparallel to the external magnetic
field is determined, as a function of the external magnetic field strength H. The results are then compared with analogous
data obtained by other authors without taking the minimum of the system’s total energy into account.
Brestsk State University. Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 2, pp. 14–19, February, 1997. 相似文献
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The reflection coefficient for normal incidence electrons may be deduced by using the technique of transverse electron focussing. It is shown how results from such experiments may be interpreted, using Soffer's surface scattering model, to deduce surface roughness for tungsten, cooper and silver. 相似文献
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The nonlinear interaction of electron beam with inhomogeneous semi-bounded collisional magnetized warm plasma under external static magnetic field has been studied. The second-harmonic generation at the beam entrance into the plasma is considered. This process leads to an increase in the amplitude of the electric field in the inhomogeneous region and, in turn, to higher absorption. 相似文献
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《Physics letters. A》1997,234(2):122-126
It is shown that an electrostatic electron plasma beat wave is efficiently unstable for a low-frequency and short-wave-length purely growing perturbation (ω, k), i.e. an oscillating two-stream instability in a transversely magnetized hot plasma. The nonlinear response of electrons and ions with strong finite Larmor radius effects has been obtained by solving the Vlasov equation expressed in the guiding-center coordinates. The effect of ion dynamics has been found to play a vital role around ω ∼ ωci, where ωci is the ion-cyclotron frequency. For typical plasma parameters, it is found that the maximum growth rate of the instability is about two orders higher when ion motion is taken into account in addition to the electron dynamics. 相似文献