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91.
Effects of dynamo magnetic fields on observational properties of accreting millisecond X-ray pulsars
In this paper,we have investigated accreting millisecond X-ray pulsars,which are rapidly rotating neutron stars in low-mass X-ray binaries.These systems exhibit coherent X-ray pulsations that arise when the accretion flow is magnetically channeled to the stellar surface.Here,we have developed the fundamental equations for an accretion disk around accreting millisecond X-ray pulsars in the presence of a dynamo generated magnetic field in the inner part of the disk.We have also formulated the numerical method for the structure equations in the inner region of the disk and the highest accretion rate is enough to form the inner region of the disk,which is overpowered by radiation pressure and electron scattering.Finally,we have examined our results with the effects of dynamo magnetic fields on accreting millisecond X-ray pulsars. 相似文献
92.
采用甘肃省CORS网和中国大陆构造环境监测网络中共48个台站的GPS观测数据,解算得到观测台站的垂直位移,并与GRACE时变重力场Mascon模型解CSR RL05M数据计算得到的垂直形变进行比较,分析区域地表垂直形变特征。结果表明,研究区内台站垂直形变存在局部特征,甘肃庆阳和平凉地区垂直形变与其他地区存在明显差异,相关系数、均方根减少量和周年信号减少量均高于其他地区;扣除趋势项后,观测台站GPS垂直位移与GRACE垂直形变时间序列相关系数均值为0.72,GPS和GRACE周年信号振幅均值分别为6.00 mm和3.70 mm,周年信号减少量和均方根误差减少量均值分别为0.51和0.29;研究区内GPS垂直位移和GRACE垂直形变时间序列一致性较强,GRACE垂直形变能有效解释50%以上的GPS垂直位移周年信号,GPS垂直位移时间序列包含的非构造形变中平均约29%来源于环境负载变化所引起的负荷形变。 相似文献
94.
Li brines are the primary resources for Li salt industries. Evaporation is necessary to concentrate Li due to its low level of concentration in raw brines. The salt sequences during the evaporation of Li brines,especially the behavior of Li salts,represent key data for solar technologies. However,chemists cannot use any phase diagram to estimate Li salt sequences during evaporation at 25℃ . The thermodynamic model proposed by us in2003 represents the only tool for the prediction of equilibrium conditions during the evaporation of solutions containing Li~+,Na~+,K~+,Mg~(2+)/Cl~-,SO_4~(2-),and-H_2 O components at 25℃ . In this paper,the predicted salt sequences of 20 brines are reported. The results indicate that( 1) the first crystallized Li salt during evaporation of Li brine varies in brine composition;( 2) lithium sulfate is crystallized in many cases initially for brines of magnesium sulfate subtype,while Db4( Li_2 SO_4·K_2 SO_4) or Db3( 2 Li_2 SO_4·Na_2 SO_4·K_2 SO_4) appears first for sodium sulfate and magnesium sulfatesubtypes with lower Mg/Li composition,and the final eutectic point is H ~+ LiC ~+ Lc ~+ Ls ~+ Car;( 3) the final eutectic point is H ~+ LiC ~+ Lc ~+ Car for brines of chloride type; and( 4) Li content corresponding to the first crystallized Li salt is in the range of 0. 43%-1%. These findings enhance our knowledge of Li chemistry and provide insights into solar pond technology of the Li-brine process. 相似文献
95.
Robert G.Strom Renu Malhotra Zhi-Yong Xiao Takashi Ito Fumi Yoshida Lillian R Ostrach 《天文和天体物理学研究(英文版)》2015,(3):407-434
We review previously published and newly obtained crater size-frequency distributions in the inner solar system. These data indicate that the Moon and the terrestrial planets have been bombarded by two populations of objects. Population 1,dominating at early times, had nearly the same size distribution as the present-day asteroid belt, and produced heavily cratered surfaces with a complex, multi-sloped crater size-frequency distribution. Population 2, dominating since about 3.8–3.7 Gyr,had the same size distribution as near-Earth objects(NEOs) and a much lower impact flux, and produced a crater size distribution characterized by a differential –3single-slope power law in the crater diameter range 0.02 km to 100 km. Taken together with the results from a large body of work on age-dating of lunar and meteorite samples and theoretical work in solar system dynamics, a plausible interpretation of these data is as follows. The NEO population is the source of Population 2 and it has been in near-steady state over the past ~ 3.7–3.8 Gyr; these objects are derived from the main asteroid belt by size-dependent non-gravitational effects that favor the ejection of smaller asteroids. However, Population 1 was composed of main belt asteroids ejected from their source region in a size-independent manner, possibly by means of gravitational resonance sweeping during orbit migration of giant planets;this caused the so-called Late Heavy Bombardment(LHB). The LHB began some time before ~3.9 Gyr, peaked and declined rapidly over the next ~ 100 to 300 Myr,and possibly more slowly from about 3.8–3.7 Gyr to ~2 Gyr. A third crater population(Population S) consisted of secondary impact craters that can dominate the cratering record at small diameters. 相似文献
96.
97.
98.
本文从地质背景、样品分析方法、气液包体特征、包一显微测温和温度气压计等几个方面扼要介绍了布阿泽尔地区不同矿床内矿前、矿后石英以及矿后方解石中卤水包体的特征,提出布阿泽尔钴矿和Cobalt银矿代表了同一类型的Co-Ag-As矿化中Ag-Co含量的差异。 相似文献
99.
基于制造业企业网络视角的城市网络核心—边缘结构的研究将加深对城市网络演化规律的理解。利用2020年中国制造业500强企业网络数据和隶属联系模型构建城市网络,研究了中国城市网络核心—边缘结构的演化特征,定量测度了核心—边缘结构的影响因素,并根据国际生产折衷理论解析了城市网络地位分异的动力机制。研究发现: 2005—2020年,核心区块的城市数量逐渐增加,主要由直辖市、经济特区以及东、中部地区的省会城市组成,这些城市通过互惠性的链接关系形成了凝聚子群,网络权力较为集中;边缘区块的城市则主要位于中、西部地区,城市间经济联系相对稀疏,整体网络结构并不稳定,城市的发展受到了网络资本的约束。关键资源、基础设施和区位优势是影响中国城市网络地位的决定性因素,择优选择、网络邻近和路径依赖构成了中国城市网络核心—边缘结构演化的动力机制,这将进一步增强核心城市的网络地位。在网络环境下,城市间的差距趋于扩大,城市网络地位的提升取决于城市在网络中的影响力,中国城市化政策需要做出相应调整。 相似文献