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排序方式: 共有1854条查询结果,搜索用时 31 毫秒
51.
R. J. Murphy 《Space Science Reviews》2007,130(1-4):127-138
Interactions of ions accelerated in solar flares produce gamma-ray lines and continuum and neutrons. These emissions contain
a rich set of observables that provides information about both the accelerated ions and the environment where the ions are
transported and interact. Ion interactions with the various nuclei present in the ambient medium produce gamma-ray lines at
unique energies. How abundance information is extracted from the measurements is discussed and results from analyses of a
number of solar flares are presented. The analyses indicate that the composition of the ambient gas where the ions interact
(typically at chromospheric densities) is different from that of the photosphere and more like the composition of the corona,
exhibiting low-FIP elemental enhancements that may vary from flare to flare. Evidence for increased Ne/O and the photospheric
3He abundance is also discussed. 相似文献
52.
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
53.
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
54.
We present up-to-date evolutionary models of low-mass stars, from M0.6 M down to the hydrogen burning minimum mass, using recent equation of state and synthetic spectra calculations. Comparison is made with observed luminosity function for these objects. We also present implications for the dark-matter distribution in the galactic halo. 相似文献
55.
C. De Jager 《Space Science Reviews》2005,120(3-4):197-241
56.
探讨了用钨极氩弧焊焊接铝合金LY12CZ及LY12M薄板时其热裂纹的变化规律,并分析了焊接工艺参数及填充材料对热裂纹的影响。试验结果表明,选择合适的工艺参数和填充材料可以明显提高该类合金的抗裂性能。 相似文献
57.
混浊液内部的流动,由于微粒子之间的相互作用以及因浊度高不易进行内部观察,所以无论是分析还是可视化实验都相当困难,存在着许多未弄清的问题。通过采用折射率匹配(Refractive-IndexMatching)技术,使透明的微粒子与透明的溶媒的折射率近乎相同,做成一种透明的“混浊液”,从而使混入其中的示踪粒子的运动轨迹能被摄像机捕捉到,并以微粒子的沉降和温度的干涉所引起的流动现象为焦点,利用图像速度测量法来处理分析所拍摄到的可视化图像,成功地获得了定量的混浊液内部的速度场,为进一步揭示混浊液内部自然对流的流动机理提供了实验依据。 相似文献
58.
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
59.
航天材料热物理性能测试技术的发展现状 总被引:1,自引:0,他引:1
根据航天材料热物理性能测试技术的特点 ,系统介绍了国内航天材料热物理性能测试技术的发展状况和发展趋势 ,并详细介绍了目前我国航天材料热物理性能测试领域中所具备的测试技术和测试装置、航天热物理性能所涉及的研究领域和内容以及目前正在开展的研究工作。 相似文献
60.