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81.
82.
C. Gontikakis A. Anastasiadis C. Efthymiopoulos 《Monthly notices of the Royal Astronomical Society》2007,378(3):1019-1030
The acceleration of charged particles in a site of magnetic reconnection is analysed by detailed numerical simulations. Single or multiple encounters of the particles with Harris-type reconnecting current sheets (RCSs) are modelled as an overall stochastic process taking place within an active region. RCS physical parameters are selected in a parameter space relevant to solar flares. Initially, the charged particles form a thermal (Maxwellian) distribution corresponding to coronal temperature ≃2 × 106 K . Our main goal is to investigate how the acceleration process changes the shape of the particles' kinetic energy distribution. The evolution of the kinetic energy distribution, calculated numerically after one encounter of the particles with a single RCS, is found to be in good agreement with our previously published analytical formulae. In the case of consecutive encounters, we find that the kinetic distribution tends to converge to a practically invariant form after a relatively small number of encounters. We construct a discrete stochastic process that reproduces the numerical distributions and we provide a theoretical interpretation of the asymptotic convergence of the energy distribution. We finally compute the theoretical X-ray spectra that would be emitted by the simulated particles in a thick target model of radiation. 相似文献
83.
84.
Edison Liang 《Astrophysics and Space Science》2007,307(1-3):309-313
We review recent PIC simulation results which show that double-sided irradiation of a thin over-dense plasma slab with ultra-intense
laser pulses from both sides can lead to sustained comoving Poynting flux acceleration of electrons to energies much higher
than the conventional ponderomotive limit. The result is a robust power-law electron momentum spectrum similar to astrophysical
sources. We discuss future ultra-intense laser experiments that may be used to simulate astrophysical particle acceleration. 相似文献
85.
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
86.
87.
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
88.
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
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
89.
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
90.
?????????????????????????ο??????????????????????????????????????????????????????????NGA?????????????????????????飬??????????????????????о?????????????????????????????????????????2012?????4.7??????????е?????????????????????????????????????PGA??????S??a??T???????б????о?????????????????????????????????????????????????????????????????????????????????????????????? 相似文献