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41.
P. C. Frisch 《Space Science Reviews》2007,130(1-4):355-365
The properties of interstellar matter at the Sun are regulated by our location with respect to a void in the local matter
distribution, known as the Local Bubble. The Local Bubble (LB) is bounded by associations of massive stars and fossil supernovae
that have disrupted dense interstellar matter (ISM), driving low density intermediate velocity ISM into the void. The Sun
appears to be located in one of these flows of low density material. This nearby interstellar matter, dubbed the Local Fluff,
has a bulk velocity of ∼19 km s−1 in the local standard of rest. The flow is coming from the direction of the gas and dust ring formed where the Loop I supernova
remnant merges into the LB. Optical polarization data suggest that the local interstellar magnetic field lines are draped
over the heliosphere. A longstanding discrepancy between the high thermal pressure of plasma filling the LB and low thermal
pressures in the embedded Local Fluff cloudlets is partially mitigated when the ram pressure component parallel to the cloudlet
flow direction is included. 相似文献
42.
T. S. Bastian 《Space Science Reviews》1994,68(1-4):261-274
Radio and X-ray observations of stellar flares provide the most direct probes of energy relaase particle acceleration, and energy transport on stars other than the Sun. In this review, the observational basis for our understanding of the flare phenomenon on other stars is briefly described and outstanding interpretive and theoretical issues are discussed. I shall confine my attention to objects which are solar-like, to the extent that they possess deep convective envelopes and display activity which is presumed to be magnetic in origin. These include pre-main sequence objects, classical flare stars, and close binaries. Future directions are briefly discussed. 相似文献
43.
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
44.
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
45.
C. De Jager 《Space Science Reviews》2005,120(3-4):197-241
46.
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
47.
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
48.
超声爬波无损检测方法的研究 总被引:2,自引:0,他引:2
本文介绍了超声无损检测中一种具有较好应用前景的波型──超声爬波。试验研究了爬波检测时缺陷定位、定性评定的方法,并给出了主要结论。 相似文献
49.
显式有限差分方法用于求解小钝锥高超声速化学非平衡尾流的轴对称边界层方程。该方法既适用于层流也适用于湍流。应用 Goldburg 转捩准则确定转捩初始位置。详细地计算了小钝锥尺寸、飞行速度、高度对尾流转捩和光电特性的影响。从计算中得到转捩和光电特性变化的一些有用规律。对湍流亚密部分的雷达散射截面进行了规律性分析。计算结果具有实用参考价值。 相似文献
50.