排序方式: 共有78条查询结果,搜索用时 15 毫秒
71.
J. Bolmont A. Jacholkowska 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
Lorentz Invariance Violation (LIV) may be a good observational window on Quantum Gravity physics. Within last few years, all major gamma-ray experiments have published results from the search for LIV with variable astrophysical sources: gamma-ray bursts with detectors on-board satellites and Active Galactic Nuclei with ground-based experiments. In this paper, the recent time-of-flight studies with unpolarized photons published from the space and ground based observations are reviewed. Various methods used in the time delay searches are described, and their performance discussed. Since no significant time-lag value was found within experimental precision of the measurements, the present results consist of 95% confidence level limits on the Quantum Gravity scale on the linear and quadratic terms in the standard photon dispersion relations. 相似文献
72.
钛铝金属间化合物基合金中的孪生与孪生交互作用 总被引:1,自引:1,他引:0
因其具有的低对称正方点阵结构,孪生在钛铝金属间化合物基合金塑性变形中的重要性愈来愈引起广泛注意,被认为对塑性、加工硬化和断裂过程有重要影响。因此,对钛铝基合金中孪生和孪生交互作用机理的研究是近几年来的一个热点。综述了该研究领域取得的一些进展和目前对孪生和孪生交互作用机理的认识水平及未来的研究方向 相似文献
73.
A. Mujiber Rahman S. Umapathy A. Shanmugaraju Y.-J. Moon 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
We have analyzed 101 CMEs, and their associated ICMEs and interplanetary (IP) shocks observed during the period 1997–2005. The main aim of the present work is to study the interplanetary characteristics of metric and DH type II associated CMEs such as, shock strength, IP shock speed, ICME speed, stand off distance and transit time. Among these 101 CMEs, 38 events show both metric and DH type II bursts characteristics. There are no metric and DH type II association for 52 events. While DH type II alone is found in 7 cases, metric type II alone is found in 4 events. It is found that the mean speeds of CMEs increase progressively from CMEs without type II events to CMEs associated with metric and DH type IIs as suggested by Gopalswamy et al. (2005). In addition, we found that the speeds of ICMEs and IP shocks progressively increase in the following order: events without metric and DH type IIs, events with metric alone, events with DH alone and events with both metric and DH type IIs. Similarly the Mach number is found to increase in the same order. While there is not much change in the stand-off distance among these cases, it is minimum (∼18 R⊙) for CMEs with speed greater than 2200 km/s. The above results confirm that more energetic CMEs can produce both metric and DH type IIs for which the interplanetary parameters such as mean values of ICME speed and IP shock speed and Mach number are found to be higher. 相似文献
74.
Igor G. Mitrofanov 《Space Science Reviews》1995,74(3-4):417-426
The paper is devoted to the present crisis in the field of cosmic gamma-ray bursts. There are two different paradigms of the phenomenon, which have practically equal numbers of supporters. The cosmological one associates bursts with collisions of compact objects at distances up to those with red-shifts of about 1–2. The galactic paradigm assumes that bursts are generated by neutron stars in the extended galactic halo. The present situation is shown to be very close to the ultimate establishment of the paradigm of the origin of cosmic gamma-ray bursts. 相似文献
75.
R.I. Hayles C. Barat K. Hurley M. Niel G. Vedrenne I.V. Estulin V.G. Kurt A.V. Kuznetsov V.M. Zenchenko 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
A study of the morphology of 14 short ( 1 s) gamma ray bursts observed by the Franco Soviet SIGNE detectors onboard the VENERA spacecraft between 1978 and 1982 is presented. We find two major groups of short bursts characterised not only by their different durations ( 1 s and 100 ms respectively), but also by different e-folding rise and decay times. A study of the time history of the impulsive portion of the 1979 March 5 event at 2 ms resolution shows evidence for a previously undiscovered 23ms quasi periodicity. These results are discussed in the context of neutron star models for gamma ray bursters. 相似文献
76.
We have searched for interrelations of spikes emitted simultaneously at different frequencies during the impulsive phase of flare events (Fig.1). As the spikes are related to the flare energy release and are interpreted as emissions that originate at different sites having different magnetic field strengths, any relation in frequency is interpretated as a relation in space. Quantities of symbolic dynamics, such as mutual information, Shannon information and algorithmic complexity are appropriate to characterize such spatiotemporal patterns, whereas the popular estimate of fractal dimensions can be applied to low-dimensional systems only.The goal is to decide between two possible types of fragmentation depending on the energy release and emission processes, which we callglobal andlocal organization. In the global organization the whole region becomes supercritical, and the energy is released in independent, small regions. The alternative local scenario requires a trigger that spreads from initial localized events and ignites nearby regions.Mutual information which is a generalization of correlation indicates a relation in frequency beyond the bandwidth of individual spikes. The scans in the spectrograms with large mutual information also show a low level of Shannon information and algorithmic complexity, indicating that the simultaneous appearance of spikes at other frequencies is not a completely stochastic phenomenon (white noise). It may be caused by a nonlinear deterministic system or by a Markov process. By means of mutual information we find a memory over frequency intervals up to 60 MHz (Fig. 2). Shannon information and algorithmic complexity, however, describe spike events as a whole, i.e. a global source region. A global organization is also apparent in quasi-periodic changes of the Shannon information and algorithmic complexity in the range of 2–8 seconds (Fig. 3).This findings is compatible with a scenario of local organization in which the information of one spike event spreads spatially and hence triggers further spike events at different places. The region is not an ensemble of independently flashing sources, each representing a system that cascades in energy after an initial trigger. On the contrary, there is a causal connection between the sources at any time.The analysis of four spike events suggests that the simultaneous appearance of spikes is not stochastically independent but a process in which spikes at nearby locations are simultaneously triggered by a common exciter.We have shown in the case in the case of spikes that quantities from nonlinear dynamics used in this paper are helpful in detecting structural properties of complex spatio-temporal patterns. This approach seems to be promising also for several other astrophysical applications. 相似文献
77.
涡轮叶片是航空发动机及地面燃气轮机的重要热端部件,研究其损伤行为对涡轮叶片的制造及修复工作均有重要的意义。本文研究了长时与短时服役涡轮叶片的蠕变损伤行为,发现二者在蠕变空洞的形成机理上大致相同,而γ′相与碳化物的退化反应则有所差异,长时服役涡轮叶片的γ′相形貌更加粗大且不规则。对于碳化物,长时服役叶片的碳化物发生了由一次MC型向二次M23C6型的分解,而短时服役叶片的碳化物发生了由MC(1)型向MC(2)型的转化。此外,针对两种不同的叶片材料(K002和GTD-111高温合金),研究了不同的固溶处理制度对γ′相溶解行为的影响,发现提高固溶温度和增加固溶保温时间可以促进两种材料γ′相的溶解行为;而随着固溶时间的增加,两种材料的溶解激活能均逐渐增大,K002合金在不同固溶保温时间中的溶解激活能均大于GTD-111合金。 相似文献
78.
应用MonteCarlo方法对太阳X射线暴(1-8Å及0.5-4Å)与地球大气相互作用过程进行跟踪模拟,得到了X射线暴在电离层D层产生的电子产生率,并计算了由此产生的宇宙噪声吸收值。结果与作者在南极观测得到的X射线暴期间宇宙噪声吸收值符合较好. 相似文献