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61.
周文松 《海军航空工程学院学报》2014,29(3):247-251
建立完善的螺旋桨绕流理论异常困难,这一方面是由于螺旋桨流场整体旋转性、非定常非线性、三维效应、气流粘性、涡桨干扰等原因;另一方面是螺旋桨流场的流场结构有待于进一步认知。文章采用CFD方法对螺旋桨的瞬态流场结构进行了重点研究,详细绘制了自启动瞬间直至充分发展的螺旋桨瞬态流场结构图及所受气动力的变化图,分析了流场变化特性及其对升力的影响。 相似文献
62.
S.A. Pulinets 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The concept of the Global Electric Circuit (GEC) provides an explanation of the existence of a vertical atmospheric electric field and coupling between the ground and ionosphere. Presently, ionospheric physics pays more attention to electric fields and coupling processes in the polar and auroral regions, whereas in other areas the potential difference between the ground and ionosphere usually is not taken into account. Regional processes exist, however, that are able to significantly affect the GEC parameters and through modification of the ionospheric potential to create plasma density irregularities of different scales within the ionosphere. One such source of ionosphere modification is air ionization in the vicinity of active tectonic faults, which takes place due to increased radon emanation. This paper considers the process of local modification of the GEC and corresponding ionospheric variability due to tectonic activity. 相似文献
63.
The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field. 相似文献
64.
T. Hirayama 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):914-925
In this paper we present a new mechanism of the main energy conversion of the solar flare. Since a flare inducing prominence (flux tube) rises Vz ? 300 km s−1, the plasmas below it cannot continuously eject with Alfvén speeds of VA = 3000 km s−1 but probably with Vz ≈ ±100 km s−1. Plasma up and downflows with VA will within a short duration be blocked between the chromosphere where reconnected flux tubes are piling up, and the slowly rising flux rope. Hence the Petschek slow shock mechanism is difficult to be realized as a major energy converting mechanism. 相似文献
65.
在铁路无线列调通信中存在弱场区和盲区,通信质量难以控制。设计了完整的方案,提高了原无线列调中存在的弱场区的场强,并增大场强覆盖率,使通话距离得到扩展,改善了话音质量。 相似文献
66.
José Luis Ballester 《Space Science Reviews》2005,121(1-4):105-113
Prominence seismology is a rapidly developing topic which seeks to infer the internal structure and properties of solar prominences
from the study of its oscillations. An extensive observational background about oscillations in quiescent solar prominences
has been gathered during the last 70 years. These observations point out the existence of two different types of oscillations:
Flare-induced oscillations (winking filaments) which affect the whole prominence and are of large amplitude and small amplitude
oscillations which seem to be of local nature. From the theoretical point of view, few models have been set up to explain
the phenomenon of winking filaments while, on the contrary, for small amplitude oscillations a large number of models trying
to explain the observed features have been proposed. 相似文献
67.
Nat Gopalswamy 《Space Science Reviews》2006,124(1-4):145-168
Interplanetary coronal mass ejections (ICMEs) originating from closed field regions on the Sun are the most energetic phenomenon
in the heliosphere. They cause intense geomagnetic storms and drive fast mode shocks that accelerate charged particles. ICMEs
are the interplanetary manifestations of CMEs typically remote-sensed by coronagraphs. This paper summarizes the observational
properties of ICMEs with reference to the ordinary solar wind and the progenitor CMEs. 相似文献
68.
V.M. Lipunov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The general aproach is considered which describs the evolution of neutron stars in terms of their interaction with surrounding matter. All possible states of neutron stars are classified from this point of view. Classification and evolution of binaries contaning neutron stars are also considered. 相似文献
69.
杨继松 《中国空间科学技术》1997,17(4):1-8
通过对几个具体实例的计算,证实了在电磁场边值问题的矩量法求解过程中,选用不同的基函数其解的数值稳定性会有很大的差别。从而有可能选择一种数值稳定性比较好的基函数来进行矩量法求解。另一方面,提出了选用多尺度子域基函数,并通过多次迭代来提高矩量法解的精度的算法。实例计算表明,该算法不仅可以有效地降低系数矩阵的条件数,而且还降低了对计算机内存容量的要求,是一种有效的、稳定的算法 相似文献
70.
无电极高密度等离子体电磁推进技术已成为未来深空探测、载人航天和货运、太阳能电站以及航天器在轨服务与维护等空间任务中极具竞争力的核心推进技术之一。在梳理不同无电极等离子体电磁加速机制基础上,开展大功率无电极高密度等离子体电磁推进技术性能对比,给出新概念无电极场反构型电磁推进技术向未来超大功率拓展的优势和发展潜力,同步分析了该技术亟需解决的关键基础问题,旨在为中国新概念场反构型电磁推进技术的研发提供理论基础。 相似文献