Effect of parallel electric field on electrostatic ion-cyclotron instability in anisotropic plasma in the presence of ion beam and general distribution function—Particle aspect analysis     

Ruchi Mishra 《Planetary and Space Science》2006,54(2):188-199

Dispersion relation, resonant energy transferred, growth rate and marginal instability criteria for the electrostatic ion-cyclotron wave with general loss-cone distribution in low-β anisotropic, homogeneous plasma in the auroral acceleration region are discussed by investigating the trajectories of the charged particles. Effects of the parallel electric field, ion beam velocity, steepness of the loss-cone distribution and temperature anisotropy on resonant energy transferred and growth rate of the instability are discussed. It is found that the effect of the parallel electric field is to stabilize the wave and enhance the transverse acceleration of ions whereas the effect of steepness of loss-cone, ion beam velocity and the temperature anisotropy is to enhance the growth rate and decrease the transverse acceleration of ions. The steepness of the loss-cone also introduces a peak in the growth rate which shifts towards the lower side of the perpendicular wave number with the increasing steepness of the loss-cone.  相似文献   

基于三轴加速度的波浪测量技术研究     

赵杰  惠力  初士博  盖志刚  朱洪海  杨俊贤  王志 《海洋技术学报》2015,34(5):66-70

以浮标为载体,以TMS320C6416型DSP处理器、三轴加速度传感器、电子罗盘为硬件电路核心,利用加速度频域二次积分的波高计算方法以及三轴加速度倾角补偿电子罗盘的波向测量方式,进行海洋波浪要素测量技术研究,获取了某一海域不同时段的波浪特征值。  相似文献   

Ion acceleration and Alfvén wave generation at the Earth’s bow shock     

E. G. Berezhko  S. N. Taneev 《Astronomy Letters》2007,33(5):346-353

The processes of ion acceleration and Alfvén wave generation by accelerated particles at the Earth’s bow shock are studied within a quasi-linear approach. Steady-state ion and wave spectra are shown to be established in a time of 0.3–4 h, depending on the background level of Alfvénic turbulence in the solar wind. The Alfvén waves produced by accelerated ions are confined within the frequency range 10^?2–1 Hz and their spectral peak with a wave amplitude βB ～ B comparable to the interplanetary magnetic field strength B corresponds to the frequency v = (2–3) × 10^?2 Hz. The high-frequency part of the wave spectrum (v > 0.2 Hz) undergoes damping by thermal ions. The calculated spectra of the accelerated ions and the Alfvén waves generated by them reproduce the main features observed in experiments.  相似文献   

Some things old, some things new: The spatial representations and politics of change of the peak oil relocalisation movement   总被引：1，自引：0，他引：1  

Ian Bailey  Rob Hopkins  Geoff Wilson 《Geoforum》2010,41(4):595-605

Despite continued uncertainty about the physical realities and political, economic and social implications of peak oil, combined concerns about oil scarcity, climate change and globalisation has spawned an energetic relocalisation movement dedicated to achieving a comprehensive reduction in oil dependency through community-scale initiatives. This paper uses a discourse approach to examine the emergence, geographical spread and practices of the Transition Network, a UK-originated relocalisation movement now involving 186 local initiatives in the UK and other countries. We trace the movement’s drawing upon, and innovation from, discourses and techniques used by other grassroots environmental movements to promote a spatial representation of peak oil as an inevitable and geographically undiscriminating problem, and its use of addiction metaphors and participatory techniques to promote personal and community-scale energy descent initiatives as a viable and necessary alternative to globalisation. We also analyse the spatial representations and techniques used in the Network’s “rhizomic” spread across multiple localities around the world and embedding in communities where relocalisation initiatives are established. We conclude by examining the future challenges these spatial constructions of peak oil pose for the relocalisation movement.  相似文献   

Oil in parallax: Scarcity, markets, and the financialization of accumulation     

Mazen Labban 《Geoforum》2010,41(4):541-552

Relations between oil scarcity, production, investment, and price have become increasingly mediated and shaped by financial markets. Yet, the mediation of finance is absent in peak oil narratives, which posit a direct relation between the availability of oil in the ground and its price on the market. The orthodox critique of peak oil deconstructs its basis in geological limits only to reproduce the argument from scarcity and reverse the relationship between the price of oil and its availability on the market. Both narratives are formulated in physical space and do not account for the degree to which the oil market has become infused by the logic of finance. Critical political economy, on the other hand, demonstrates the extent to which finance has transformed capital accumulation, only to render material production somewhat irrelevant to the accumulation of capital. This is equally problematic, given oil companies’ continuing investment in production and reserve expansion. The relation between accumulation, investment, and production under finance needs to be examined rather than discarded. I argue that finance has emancipated the circulation of oil in the world market from its circulation in physical space, fragmenting the oil market into a physical and a financial component, but reintegrating both under the dominance of financial logic without transcending their duality and their differences. I explicate this relation by examining the circulation of oil in trade and investment under the dictates of finance to open questions on current theorizations of oil scarcity in relation to prices, markets, and investment.  相似文献   

Using path analysis to identify the influence of climatic factors on spring peak flow dominated by snowmelt in an alpine watershed   总被引：5，自引：1，他引：4  

Fei-Yun Zhang  Lan-Hai Li  Sajjad Ahmad  Xue-Mei Li 《山地科学学报》2014,11(4):990-1000

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孟庆筱  王太松  韩勇  胡国新  吕健  郭宝震  李伟亮 《大地测量与地球动力学》2014,34(4):9-16

?????????????????????????ο??????????????????????????????????????????????????????????NGA?????????????????????????飬??????????????????????о?????????????????????????????????????????2012?????4.7??????????е?????????????????????????????????????PGA??????S??a??T???????б????о??????????????????????????????????????????????????????????????????????????????????????????????  相似文献   

常加速度模型的简化自协方差最小二乘法     

林旭  罗志才  姚朝龙 《测绘学报》2014,43(11):1144-1150

“当前”统计模型自适应算法并非真正意义上的自适应目标跟踪算法,其性能与其中关键参数的选择有着直接的关系。本文以常加速度模型对机动载体进行建模,顾及其状态噪声协方差矩阵满足特定结构,提出了简化的自协方差最小二乘噪声协方差估计方法,该方法通过建立新息的相关函数序列与未知噪声协方差矩阵间的函数模型,并结合最小二乘法进行噪声协方差估计。数值仿真结果表明,当载体进行阶跃加速度运动或变加速度运动时,本文所提方法的目标跟踪精度均优于“当前”统计模型自适应算法。  相似文献   

Regular and chaotic dynamics in 3D reconnecting current sheets     

C. Gontikakis  C. Efthymiopoulos  A. Anastasiadis 《Monthly notices of the Royal Astronomical Society》2006,368(1):293-304

We consider the possibility of particles being injected at the interior of a reconnecting current sheet (RCS), and study their orbits by dynamical systems methods. As an example we consider orbits in a 3D Harris type RCS. We find that, despite the presence of a strong electric field, a 'mirror' trapping effect persists, to a certain extent, for orbits with appropriate initial conditions within the sheet. The mirror effect is stronger for electrons than for protons. In summary, three types of orbits are distinguished: (i) chaotic orbits leading to escape by stochastic acceleration, (ii) regular orbits leading to escape along the field lines of the reconnecting magnetic component, and (iii) mirror-type regular orbits that are trapped in the sheet, making mirror oscillations. Dynamically, the latter orbits lie on a set of invariant KAM tori that occupy a considerable amount of the phase space of the motion of the particles. We also observe the phenomenon of 'stickiness', namely chaotic orbits that remain trapped in the sheet for a considerable time. A trapping domain, related to the boundary of mirror motions in velocity space, is calculated analytically. Analytical formulae are derived for the kinetic energy gain in regular or chaotic escaping orbits. The analytical results are compared with numerical simulations.  相似文献   

On the cosmic ray spectrum from type II supernovae expanding in their red giant presupernova wind     

《Astroparticle Physics》2015

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