The Landau level-superfluid modified factor and the overal soft X/<Emphasis Type="Italic">γ</Emphasis>-ray efficiency coefficient of a magnetar     

Z. F. Gao  Q. H. Peng  N. Wang  C. K. Chou  W. S. Huo 《Astrophysics and Space Science》2011,336(2):427-439

As soon as the energies of electrons near the Fermi surface exceed Q, the threshold energy of inverse β-decay, electron capture (EC) dominates inside a neutron star. The high-energy neutrons released by EC will destroy anisotropic ³ P ₂ neutron Cooper pairs in the degenerate superfluid. By colliding with the neutrons produced in the process n+(n↑n↓)→n+n+n, the kinetic energies of the neutrons released by EC will be transformed into thermal energy. A portion of this thermal energy will be transported from the star interior to the star surface by conduction, then converted to a thermal spectrum of soft X-rays and γ-rays. By introducing two important parameters: the Landau level-superfluid modified factor and the overal soft X/γ-ray efficiency coefficient, we compute the theoretical luminosity L _X of a magnetar under our model and plot a diagram of L _X as a function of magnetic field strength B. Numerical calculations based on our model agree well with the observed properties of magnetar candidates.  相似文献   

低高度角大气静力学延迟修正的改进     

刘艳  郭鹏  刘敏 《天文学报》2010,51(3)

进行低高度角观测是GPS(Global Positioning System)气象学的发展趋势,其中发展高精度的低高度角的大气静力学延迟修正是主要的关键技术.比较了3种计算无线电波从空间到地面接收机的大气静力学延迟修正方法:(1)在大气球对称假设下用探空气球资料路径积分得到大气静力学延迟;(2)在大气球对称假设下用NCEP(National Centers for Environmental Prediction)再分析资料得到大气静力学延迟;(3)用Niell的大气静力学映射函数得到大气静力学延迟.与2001年中国地区89个探空气球站资料计算得到的大气静力学映射函数比较结果显示:NCEP再分析资料路径积分的方法在低高度角(5°以下)的精度好于Niell映射函数模型约5倍.  相似文献   

The evolution of the z distribution of normal neutron stars in the Galaxy     

Y.‐C. Wei  C.‐M. Zhang  Y.‐H. Zhao  Q.‐H. Peng  X.‐J. Wu  J. Wang  Y.‐Y. Pan  H.‐X. Yin  Y. Yan  T.‐S. Yan  H.‐J. Tian  A. Esamdin  A.L. Luo  Y. Cai  A. Taani 《Astronomische Nachrichten》2010,331(8):817-831

Under the two initial 1‐D one parameter velocity distribution forms (one is normal, the other is exponential), the z direction scale height evolution of normal neutron stars in the Galaxy is studied by numerical simulation. We do statistics for the cases at different time segments, also do statistics for the cumulative cases made of each time segment. The results show in the cumulative cases the evolution curves of the scale heights are smoother than in the each time segment, i.e., the cumulation improve the signal‐to‐noise ratio. Certainly the evolution cases are different at different Galactic disk locations, which also have very large difference from the average cases in the whole disk. In the initial stages of z evolution of normal neutron stars, after the beginning transient states, the cumulative scale heights increase linearly with time, and the cumulative scale height increasing rates have linear relationship with the initial velocity distribution parameters, which have larger fluctuation in the vicinity of the Sun than in the whole disk. We utilize the linear relationship of the cumulative scale height increasing rates vs. the initial velocity distribution parameters in the vicinity of the Sun to make comparison with the observation near the Sun. The results show if there is no magnetic decay, then the deserved initial velocity parameters are obvious lower than the present well known results from some authors; whereas if introducing magnetic decay, for the 1‐D normal case we can make consistence among concerning results using magnetic decay time values which are supported by some authors, while for the 1‐D exponential case the results show the lackness of young pulsar samples in the larger z in the vicinity of the Sun (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Dependence of the holmberg effect on separations between paired galaxies     

Xin-Fa Deng  Yong Xin  Jiang Peng  Ping Wu 《Astrophysics》2010,53(3):342-350

To investigate the dependence of the Holmberg effect of paired galaxies on three-dimensional separations, we have constructed four subsamples characterized by three-dimensional separations s ≤ 50 kpc, 50 kpc < s ≤ 100 kpc , 100kpc < s ≤150kpc , and 150 kpc < s ≤ 200 kpc , respectively. In this study, linear correlation coefficients and surplus standard deviations of color indices, luminosity, and size between two components of paired galaxies are calculated. It is found that there is a weak tendency for correlation coefficients of color indices to increase with decreasing three-dimensional separations, but such a tendency does not exist for ones of luminosity and size. We also note that there is no tendency for surplus standard deviations to decrease with decreasing three-dimensional separations. This suggests that it is still very difficult to clearly affirm the dependence of the Holmberg Effect of paired galaxies on three-dimensional separations.  相似文献   

升级改造后的BPL时频监控系统     

车爱霞  段建文  魏孝峰  万江红  万亚红  乔建武  高飞 《时间频率学报》2010,33(2)

为更好地完成授时任务,对BPL长波授时系统(由中国科学院国家授时中心承建)进行了升级改造。介绍了升级改造后的BPL长波授时系统组成、时频控制与监测方法。改造前、后系统时频控制指标的统计结果表明,改造后时号控制精度大幅提高。  相似文献   

Zn²⁺对日本沼虾(Macrobrachium nipponensis)的急性致毒效应   总被引：1，自引：0，他引：1  

王志铮  任夙艺  赵晶  付英杰  杨鹏 《海洋与湖沼》2013,44(1):235-240

在水温(27.4±1.3)℃条件下,以体长(33.23±1.66)mm、体质量(0.7893±0.1518)g的日本沼虾为实验动物,采用静水停食法开展了Zn2+对日本沼虾的急性毒性实验,并以此为基础,测定了Zn2+不同质量浓度水平下日本沼虾的耗氧率与窒息点.结果表明:(1)Zn2+对日本沼虾的急性致死效应与其呼吸生理代谢受阻密切相关;(2) Zn2+对日本沼虾24h、48h、72h、96h的半致死质量浓度依次为1.493、0.844、0.643和0.464mg/L; (3) Zn2+对日本沼虾昼均、夜均和日均耗氧率均无显著影响的阈值为0.046mg/L,该值为Zn2+对日本沼虾急性毒性的安全质量浓度;(4) Zn2+对日本沼虾产生轻度胁迫和中度胁迫的质量浓度范围分别为0.046-0.064mg/L和0.064-0.082mg/L.  相似文献   

末次盛冰期末期以来南海北部陆坡的陆源物质输入及其控制因素     

黄杰  李安春  万世明  徐方建  孟庆勇 《海洋与湖沼》2013,44(4):882-889

通过对南海北部陆坡KNG5孔沉积物粒度、粘土矿物和14C年龄的综合分析, 探讨了南海北部陆坡的沉积物来源及其控制因素。物源分析表明, KNG5孔17.5-12.5ka BP的沉积物主要来源于珠江, 12.5ka BP 时粘土矿物组合突然发生改变, 并且自12.5ka BP以后, 高岭石含量总体稳定, 说明12.5ka BP时海平面已上升到相当的高度, 并且可能当时南海的现代环流系统已开始形成, 西行的广东沿岸流导致向外扩散的珠江物质减少, 由于受北太平洋深层水(NPDW)和黑潮(KC)南海分支的作用, 台湾成为此时沉积物的主要贡献者。KNG5孔17.5-11ka BP时期的粘土矿物和粒度变化主要受控于海平面和洋流系统的变化。全新世早期(11.0-8ka BP)平均粒径达到最细和1-2.2m 粒级含量达到最高值可能是强盛的夏季风作用的结果。全新世中晚期(8—0ka BP) 1-2.2?m组分含量的减少是8ka BP以来东亚夏季风减弱的具体体现, 1-2.2m 粒级含量指示的东亚夏季风变化能和北半球其它季风指标能很好地对应起来, 说明这次季风减弱是北半球各个季风系统的共同现象。  相似文献   

青海天峻新关角隧道涌排水水源识别与量化分析     

彭红明  袁有靖  李铜邦  董高峰  刘毅  巴瑞寿 《地质科技情报》2022,41(1):60-70

涌排水严重影响隧道施工与运行安全,查明隧道涌排水的来源,是隧道防水止水重要科学依据.青海天峻新关角隧道南北洞口处的地下水排水量分别为10021,60877 m3/d,两者存在近50000 m3/d的差异,涌排水量大,且来源不明.基于水文地质条件分析,分别采集了新关角隧道隧址区内大气降水、不同类型地下水和隧道出口涌排水水...  相似文献   

东北非与中国胶东造山型金矿对比及对非洲找矿勘查的启示     

曾国平  向文帅  吴发富  李福林  王建雄  胡鹏 《地质通报》2022,(1):48-59

东北非是一个快速兴起的世界级金矿省,发育大量造山型金矿床.选择东北非努比亚地盾代表性造山型矿床进行总结梳理,认为区内金矿成矿可能受控于努比亚地盾地块拼帖后挤压/压扭向张扭剪切转换的过程,绿片岩相-角闪岩相变质基性火山岩是主要赋矿围岩,剪切带(断层)为主要控矿构造.通过对比,发现努比亚地盾矿集区与胶东矿集区类似,在大规模...  相似文献   

气象卫星观测资料全球交换的基础——FM94 BUFR码原理及实现   总被引：1，自引：1，他引：0  

王素娟  崔鹏 《气象科技》2007,35(3):414-417

针对风云二号(02)批应用系统项目建设中气象卫星观测资料全球交换的需求,介绍了FM94 BUFR码的压缩原理、BUFR编码软件的信息结构和软件结构,并以风云二号C星云导风产品BUFR编码为例,给出了报文段3的详细内容和段4的数据宽度。编码结果表明BUFR编码有较高的数据压缩率,非常适合数据传输。  相似文献