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31.
H. Lesch 《Space Science Reviews》1994,68(1-4):321-327
A model for the emission processes causing rapid variability (less than one day) in active galactic nuclei is developed. Relativistic electron beams escape from reconnection sheets in coronae of accretion disks and excite plasma turbulence with a typical frequency
, which depends on the electron number densityn (see also the contribution by R. van Oss). The finite lengths of different beams emerging from different reconnection sheets allows that the waves arecoherently scattered to frequencies 2pe. For Lorentz factors 103 and densities typical for disk coronaen106
cm
–3 (derived from iron line observations) one easily reaches the optical, frequency range. The time scale of the variability is then caused by the relaxation of the electron beams. Likewise, this model explains the very rapid variability in the X-ray (less than 10 minutes) by changing the parameters slightly. According to this scenario the higher the variable frequency is, the closer to the central black hole it should originate. 相似文献
32.
F.B. Rizzato A.C.-L. Chian M.V. Alves R. Erichsen S.R. Lopes G.I. de Oliveira R. Pakter E.L. Rempel 《Space Science Reviews》2003,107(1-2):507-514
Langmuir waves and turbulence resulting from an electron beam-plasma instability play a fundamental role in the generation
of solar radio bursts. We report recent theoretical advances in nonlinear dynamics of Langmuir waves. First, starting from
the generalized Zakharov equations, we study the parametric excitation of solar radio bursts at the fundamental plasma frequency
driven by a pair of oppositely propagating Langmuir waves with different wave amplitudes. Next, we briefly discuss the emergence
of chaos in the Zakharov equations. We point out that chaos can lead to turbulence in the source regions of solar radio emissions.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
33.
空间环境下的有机热控涂层 总被引:6,自引:3,他引:6
本文综述了国外在空间有机热控涂层领域中的研究工作和试验,着重分析了空间极端环境中紫外光辐照和原子氧侵蚀这两大因素对有机热控涂层的影响。 相似文献
34.
C. De Jager 《Space Science Reviews》2005,120(3-4):197-241
35.
Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for
interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of
electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions
as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory
is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are
bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
36.
Several examples of the radio emission of eruptive solar flares with high-frequency slowly drifting structures and type II
bursts are presented. Relationships of these radio bursts with eruptive phenomena such as soft X-ray plasmoid ejection and
shock formation are shown. Possible underlying physical processes are discussed in the framework of the plasmoid ejection
model of eruptive solar flares. On the other hand, it is shown that these radio bursts can be considered as radio signatures
of eruptive solar flares and thus used for the prediction of heliospheric effects.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
37.
38.
39.
典型几何和流动参数对高超声速进气道性能的影响 总被引:12,自引:0,他引:12
用N-S方程模拟了一系列典型二元高超声速进气道内压缩通道及隔离段模型,模拟发现内压缩通道及隔离段增压比、温升比和总压恢复系数等性能参数主要受面积收缩比、内压缩通道收缩角、隔离段长高比等几何参数以及内压缩通道进口马赫数、密度、附面层厚度等流动参数的影响。内收缩比和内收缩通道收缩角的增大都会使压缩增强;隔离段内沿程平均温升比、马赫数和总压恢复系数曲线则均接近平行直线。内压缩通道进口马赫数的增大也会使压缩增强,但较小的进口马赫数可能引起分离,进而增大增压比;而进口密度增大使附面层变薄,对气流的压缩减弱;进口附面层厚度对沿程平均温升比、增压比以及马赫数的影响近似线性。 相似文献
40.
金属载体上线天线阻抗与辐射特性的矩量法研究 总被引:2,自引:0,他引:2
用线网格模拟金属载体表面,应用矩量法求出天线及载体网格上的电流分布,据此研究在该金属载体影响下的天线特性,在计算阻抗矩阵元素时,利用了非对称正弦偶极子辐射场的精确表达式,并采用了直接复数积分,简化了计算公式,本文给出了几种金属载体上线天线的阻抗与辐射特性的计算结果,它们与有关文献上的数据或实验结果一致,最后计算了一种舰船简单模型上两根线天线的远区辐射场及它们的自阻抗与互阻抗。 相似文献