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31.
Chang Tom Tam Sunny W.Y. Wu Cheng-Chin Consolini Giuseppe 《Space Science Reviews》2003,107(1-2):425-445
The first definitive observation that provided convincing evidence indicating certain turbulent space plasma processes are
in states of ‘complexity’ was the discovery of the apparent power-law probability distribution of solar flare intensities.
Recent statistical studies of complexity in space plasmas came from the AE index, UVI auroral imagery, and in-situ measurements
related to the dynamics of the plasma sheet in the Earth's magnetotail and the auroral zone.
In this review, we describe a theory of dynamical ‘complexity’ for space plasma systems far from equilibrium. We demonstrate
that the sporadic and localized interactions of magnetic coherent structures are the origin of ‘complexity’ in space plasmas.
Such interactions generate the anomalous diffusion, transport, acceleration, and evolution of the macroscopic states of the
overall dynamical systems.
Several illustrative examples are considered. These include: the dynamical multi- and cross-scale interactions of the macro-and
kinetic coherent structures in a sheared magnetic field geometry, the preferential acceleration of the bursty bulk flows in
the plasma sheet, and the onset of ‘fluctuation induced nonlinear instabilities’ that can lead to magnetic reconfigurations.
The technique of dynamical renormalization group is introduced and applied to the study of two-dimensional intermittent MHD
fluctuations and an analogous modified forest-fire model exhibiting forced and/or self-organized criticality [FSOC] and other
types of topological phase transitions.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
32.
33.
Asit Saha Jharna Tamang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1596-1606
Nonlinear and supernonlinear ion-acoustic periodic waves are investigated in a three-component unmagnetized plasma which consists of mobile fluid cold ions, Maxwellian cold electrons and q-nonextensive hot electrons employing phase plane analysis. Using the traveling wave transformation, the plasma system is reduced to a planar autonomous dynamical system. Utilizing phase plane analysis of planar dynamical systems, all possible phase portraits including nonlinear homoclinic orbit, nonlinear periodic orbit, supernonlinear homoclinic orbit and supernonlinear periodic orbit are presented depending on physical parameters and V. Using numerical simulations, nonlinear and supernonlinear ion-acoustic periodic waves are shown for different conditions. It is found that the nonextensive parameter q plays a crucial role in the bifurcations of nonlinear and supernonlinear ion-acoustic periodic waves. Our study may be applicable to understand the nonlinear and supernonlinear periodic features in auroral plasma. 相似文献
34.
电磁帆是一类利用太阳风驱动的无工质或少工质新型推进技术,在需要推力器长时间工作的深空探测任务中具有非常广阔的应用前景。首先介绍了电磁帆的基本概念和主要分类,其次分别介绍了电帆、纯磁帆和磁等离子体帆三类推进方式的系统组成和工作原理,重点介绍了各自的研究现状,并梳理出了相关关键技术,同时介绍了等离子体磁罩技术。最后对电磁帆推进技术研究进展进行了总结,为国内开展此方面研究提供了研究方向和发展思路。 相似文献
35.
Valentin A. Shuvalov Dmitry N. Lazuchenkov Nikolai B. Gorev Galina S. Kochubei 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):355-366
Using a cylindrical Langmuir probe and the authors’ proprietary two-channel pressure transducer, ionospheric plasma parameter distributions along the orbit of the Sich-2 satellite (Ukraine, 2011–2012) were measured. This paper is concerned with identifying the space–time location of ionospheric plasma disturbance sources, including the epicenters of actual earthquakes (before or during the satellite flyover) and incipient earthquakes on the subsatellite track, from the measured distributions of the electron density and temperature and the neutral particle temperature along the satellite orbit. To do this, the measured ionospheric plasma parameter distributions are connected to the coordinates on the subsatellite track.It is shown that local disturbances in the electron density and temperature and neutral particle temperature distributions in the satellite orbit in the ionosphere may serve as indicators of seismic activity on the subsatellite track. The epicenters of incipient earthquakes may be set off from other plasma parameter disturbance sources associated with seismic activity using information provided by special monitoring and survey centers that monitor the current seismic situation. 相似文献
36.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(5):1619-1633
The behaviour of the equatorial/low-latitude ionosphere and the transport processes during magnetic disturbed and quiet periods of a high solar activity year, 2014, in the American sector are investigated. Parameters used include vertical drift (Vz), transport term (W), NmF2, hmF2 and scale-height (H). The F2 plasma variations followed the diurnal local solar pattern, being higher at daytime. The sunset maximum and sunrise minimum peaks of hmF2 were directly opposite to the scale height (H) pattern. The plasma distribution was basically controlled by combined actions of the electrodynamic convection/thermospheric composition, which is geomagnetic activity dependent. The annual, semi-annual and winter-anomalies of the F2 parameters were higher at the dip equator in comparison with the low-latitude. The Vz pre-reversal peak magnitude coincided with hmF2 peak and the effects are more pronounced during geomagnetic disturbed conditions. The transport term pattern was similar to that of the scale height and it is suggested as a proxy parameter for quantifying low-latitude plasma irregularities and distribution of thermospheric composition. 相似文献
37.
Vladimir N. Gubenko A.G. Pavelyev I.A. Kirillovich Y.-A. Liou 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(7):1702-1716
We have used the radio occultation (RO) satellite data CHAMP/GPS (Challenging Minisatellite Payload/Global Positioning System) for studying the ionosphere of the Earth. A method for deriving the parameters of ionospheric structures is based upon an analysis of the RO signal variations in the phase path and intensity. This method allows one to estimate the spatial displacement of a plasma layer with respect to the ray perigee, and to determine the layer inclination and height correction values. In this paper, we focus on the case study of inclined sporadic E (Es) layers in the high-latitude ionosphere based on available CHAMP RO data. Assuming that the internal gravity waves (IGWs) with the phase-fronts parallel to the ionization layer surfaces are responsible for the tilt angles of sporadic plasma layers, we have developed a new technique for determining the parameters of IGWs linked with the inclined Es structures. A small-scale internal wave may be modulating initially horizontal Es layer in height and causing a direction of the plasma density gradient to be rotated and aligned with that of the wave propagation vector k. The results of determination of the intrinsic wave frequency and period, vertical and horizontal wavelengths, intrinsic vertical and horizontal phase speeds, and other characteristics of IGWs under study are presented and discussed. 相似文献
38.
采用雷诺平均N-S方程对碳氢燃料甲烷(CH4) 在超声速流动中混合燃烧过程进行了数值研究, 提出了简化的甲烷燃烧的反应机理及反应动力学模型, 建立了Baldw in-Lom ax 代数涡粘性湍流模型, 采用了高精度的TVD隐式格式和化学源项隐式解法, 计算结果和氢气/空气超燃的计算结果进行了比较, 表明所采用的反应机理及计算模型合理, 算法可行, 就算例结果而言,碳氢化合物作为一种超燃燃料有其独特的优势, 值得进一步深入研究 相似文献
39.
40.
通过对JL8飞机航炝吊舱供弹系统及弹带结构的分析,结合弹带在供弹道内的运动特性,找出了航炮吊舱卡停射故障产笺原因,并通过计算,提出了改进措施。 相似文献