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161.
W.Q. Gan Y.P. Li L.I. Miroshnichenko 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(6):908-913
The footpoint motions of flare hard X-ray (HXR) sources are directly related to the reconnection scenario of a solar flare. In this work, we tried to extract the information of footpoint motions for a number of flares observed with RHESSI. We found that the RHESSI flare results of the footpoint motions strongly support the classification proposed from the observations of YOHKOH/HXT. Furthermore, it is found that a flare can consist of two types of footpoint motions. We discussed the connections of the footpoint motions with the two-dimensional reconnection models. 相似文献
162.
纤维缠绕壳体设计的网格分析方法 总被引:12,自引:5,他引:12
讨论了用于纤维缠绕薄壁结构设计的网格理论的意义。基于网格理论,得到了固体火箭发动机纤维缠绕壳体圆筒壁厚和爆破压强的计算方法,给出了用模拟实验压力容器确定纤维发挥强度的方法。算例表明,计算值与实测结果符合良好。 相似文献
163.
164.
介绍了纤维缠绕金属内衬压力容器的工艺特点、性能优势和爆破前先泄漏(LBB)的安全失效模式,以及一般设计原则、构形、材料和工艺要求。分析了金属内衬的厚度、过渡区、焊接区和纤维缠绕层。以及输入输出极孔的设计技术。阐明了用于静力分析的解析法和数值法,以及用于循环寿命预测的断裂力学分析法。最后概述了一些新技术、新材料的应用情况,并指出了压力容器设计的发展趋势。 相似文献
165.
Hong Li Xiangyun Long Hua Feng Qiong Wu Jiahui Huang Weichun Jiang Massimo Minuti Dongxin Yang Saverio Citraro Hikmat Nasimi Jiandong Yu Ge Jin Ming Zeng Peng An Luca Baldini Ronaldo Bellazzini Alessandro Brez Luca Latronico Enrico Costa 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):708-714
PolarLight is a compact soft X-ray polarimeter onboard a CubeSat, which was launched into a low-Earth orbit on October 29, 2018. In March 2019, PolarLight started full operation, and since then, regular observations with the Crab nebula, Sco X-1, and background regions have been conducted. Here we report the operation, calibration, and performance of PolarLight in the orbit. Based on these, we discuss how one can run a low-cost, shared CubeSat for space astronomy, and how CubeSats can play a role in modern space astronomy for technical demonstration, science observations, and student training. 相似文献
166.
P. Jovanović V. Borka Jovanović D. Borka T. Bogdanović 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
We used a model of a relativistic accretion disk around a supermassive black hole (SMBH), based on ray-tracing method in the Kerr metric, to study the variations of the composite Fe Kα line emitted from two accretion disks around SMBHs in a binary system. We assumed that the orbit of such a binary is approximately Keplerian, and simulated the composite line shapes for different orbital elements, accretion disk parameters and mass ratios of the components. The obtained results show that, if observed in the spectra of some SMBH binaries during their different orbital phases, such composite Fe Kα line profiles could be used to constrain the orbits and several properties of such SMBH binaries. 相似文献
167.
Yoshitomo Maeda Hideyuki Mori Tadayasu Dotani 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
We detected hard X-ray emission from the unidentified Galactic bulge source 1RXS J175721.2-304405 with ASCA. The observed absorption column, flux and power-law index led us to consider that 1RXS J175721.2-304405 may be a new low-mass X-ray binary located near the Galactic center. Furthermore, the X-ray light-curve shows a step-function-like time variability, which is likely due to the occultation of a companion star. Future follow-up observations by missions such as ASTROSAT may reveal a periodic eclipse from 1RXS J175721.2-304405 if it is covered long enough. Since the long orbital period suggests a giant companion, follow-up observations will give firm evidence that 1RXS J175721.2-304405 is a new and rare eclipsing low-mass X-ray binary with a giant companion. 相似文献
168.
M.T. Menna A. Papitto L. Burderi T. Di Salvo F. DAntona N.R. Robba 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2704-2706
We analyze the three outbursts of the X-ray millisecond pulsar SAX J1808.4-3658 that occurred in 1998, 2000, and 2002 observed with RXTE. With a technique based on epoch folding search we find an unique orbital solution valid over the five years of high temporal resolution data available. We revise the estimate of the orbital period, Porb = 7249.1569(1) s and of its error, which we decrease by one order of magnitude. We also give the first constraint on the orbital period derivative, . We find that in 2002 the pulse profile shape is clearly asymmetric, showing a secondary peak at about 145° from the main pulse, which is different from the sinusoidal shape reported at the beginning of the 1998 outburst. 相似文献
169.
Dipankar Bhattacharya 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2999-3001
The Scanning Sky Monitor aboard the Indian Multiwavelength Astronomy Satellite ASTROSAT will employ coded mask X-ray cameras, rotating continuously to scan the sky. This paper discusses a method of image reconstruction for such continuously moving coded mask cameras. 相似文献
170.
Brian D. Ramsey 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2985-2988
Grazing-incidence optics has revolutionized soft-X-ray astronomy yet the scientifically important hard-X-ray region has gone relatively unexplored at high sensitivity and fine angular scales. This situation is now changing with several flight-ready balloon-borne focusing telescopes and planned satellite-borne observatories. This review discusses some of the developments in mirror and focal plane technologies that are making these payloads possible. 相似文献