Pulsar magnetic field for an infinitely conductive accretion disk     

N. R. Sibgatullin  T. A. Doroshenko 《Astronomy Letters》2002,28(11):769-772

The magnetic-field distribution outside a flat, infinitely conductive unbounded disk in the field of a point magnetic dipole is determined. A relationship is established between the problem of magnetic-field determination and the problem of the flow of an ideal incompressible fluid around an infinitely thin disk.  相似文献   

The SFR and IMF of the galactic disk     

Andreas Just 《Astrophysics and Space Science》2003,284(2):727-730

There is a long term dynamical heating of stellar populations with age observed in the age – velocity dispersion – relation (AVR). This effect allows a determination of the star formation history SFR(t) from local kinematical data of main sequence stars. Using a self-consistent disk model for the vertical structure of the disk, we find from the kinematics of the stars in the solar neighbourhood that the SFR shows a moderate star burst about 10 Gyr ago followed by a continuous decline to the present day value consistent with the observed number of OB stars. The gravitational potential of the gas component and of the Dark Matter Halo is included and the effect of chemical enrichment, finite lifetime of the stars and mass loss of the stellar component are taken into account. The scale heights for main sequence stars together with the SFR is then used to determine constistently the IMF from the observed local luminosity function. The main new result is that the power law break in the present day mass function (PDMF) around 1 M _⊙ is entirely due to evolutionary effects of the disk and does not appear in the IMF. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

圆盘固相萃取富集-气相色谱法测定地表水中有机氯和有机磷农药   总被引：4，自引：2，他引：2  

何淼  饶竹 《岩矿测试》2008,27(1):12-16

采用环境友好的圆盘固相萃取新技术富集水体中有机氯农药和有机磷农药,分别用微池电子捕获检测器(μECD)和火焰光度检测器(FPD)气相色谱法检测,实现了水中有机氯和有机磷农药残留物的测定。结果表明,16种有机氯农药的平均回收率为64.7%~102%,精密度(RSD,n=6)为2.9%~15%;13种有机磷农药的平均回收率为65.9%~104%,精密度(RSD,n=6)为1.7%~17%。方法快速、灵敏、低污染,可用于水体中多种有机氯农药和有机磷农药的残留分析。  相似文献   

陕西气象信息数据库应用平台综合设计     

刘贵华  董文乾 《山西气象》2003,(4):28-30

硬盘一旦出现故障，对每一个使用电脑的人来说简直就是一场灾难，因为硬盘里的数据比硬盘本身的价值更大，如何将其损失降到最低限度，这是非常值得研究的。  相似文献   

碟形弹簧竖向减震体系的分析与研究   总被引：1，自引：0，他引：1  

刘天适  赵强  王兴国  苏幼坡  苏经宇 《世界地震工程》2004,20(2):1-5

对碟形弹簧竖向减震体系利用时程分析方法对其进行动力分析，并输入不同场地、不同频谱的地震波考察其减震效果，验证了碟形弹簧在合理控制其刚度的前提下可以起到有效减小竖向地震的作用。  相似文献   

An efficient and robust approach to predict ship self-propulsion coefficients     

《Applied Ocean Research》2019

Achieving a reliable and accurate numerical prediction of the self-propulsion performance of a ship is still an open problem that poses some relevant issues. Several CFD methods, ranging from boundary element methods (BEM) to higher-fidelity viscous Reynolds averaged Navier–Stokes (RANS) based solvers, can be used to accurately analyze the separate problems, i.e. the open water propeller and the hull calm water resistance. However, when the fully-coupled self-propulsion problem is considered, i.e. the hull advancing at uniform speed propelled by its own propulsion system, several complexities rise up. Typical flow simplifications adopted to speed-up the simulations of the single analysis (hull and propeller separately) lose their validity requiring a more complex solver to tackle the fully-coupled problem. The complexity rises up further when considering a maneuver condition. This aspect increases the computational burden and, consequently, the required time which becomes prohibitive in a preliminary ship design stage.The majority of the simplified methods proposed in literature to include propeller effects, without directly solve the propeller flow, in a high-fidelity viscous solver are not able to provide all the commonly required self-propulsion coefficients. In this work, a new method to enrich the results from a body force based approach is proposed and investigated, with the aim to reduce as much as possible the computational burden without losing any useful result. This procedure is tested for validation on the KCS hull form in self-propulsion and maneuver conditions.  相似文献   

基于TM影像的水体透明度反演模型——以鄱阳湖国家自然保护区为例   总被引：2，自引：2，他引：0  

邬国锋  刘耀林  纪伟涛 《湖泊科学》2007,19(3):235-240

以江西鄱阳湖国家自然保护区为例,研究基于Landsat TM 5影像的水体透明度反演模型.结合6个时期的影像与对应的13个实测塞氏盘深度(SDD)数据建立了SDD的自然对数变换值与蓝、红波段的自然对数变换值的线性组合之间的回归模型,即ln(SDD)=-4.016-0.722ln(blue)-0.587ln(red).此模型能够解释88%的水体透明度变化.利用另外12个样点进行模型的检验.检验结果显示实际量测值与模型反演值之间的相关系数为0.93,误差标准差等于0.22 m.因此我们认为此模型获得了可以接受的结果.  相似文献   

慧眼-HXMT观测到的黑洞双星系统中的W-K 关系          下载免费PDF全文

马宾远  杨孜旭  廖进元  屈进禄 《天文学报》2024,65(3):25

通过几十年的观测研究, 黑洞X射线双星(X-Ray Binary, XRB)部分特征被揭示. 然而, 吸积盘结构尚不确定. 黑洞XRB功率密度谱的截断频率与准周期振荡(Quasi Periodic Oscillation, QPO)的相关性质(W-K关系)可以限制吸积盘结构. 利用慧眼-HXMT (Hard X-ray Modulation Telescope)观测到的5个黑洞XRB的数据, 对黑洞XRB的W-K关系进行了研究, 结果表明在慧眼-HXMT观测的3个探测器能段中W-K关系成立. 此外在MAXI J1535-571之中存在截断频率和吸积盘内半径的相关关系, 这和截断的吸积盘结构一致. 如果观测到的功率密度谱来自质量吸积率的扰动传播, 可以推测吸积盘内半径接近最内圆形稳定轨道, 此黑洞可能是高自旋系统.  相似文献   

激变变星中的快速光变   总被引：2，自引：0，他引：2  

李宗云  丁月蓉 《天文学进展》1996,14(2):139-148

文中综述了激变变星中快速光变的研究进展，讨论了闪变，相干振荡和准周期振荡的观测特征和可能的产生机制。  相似文献   

黑洞候选体MAXI J1535-571爆发期间的时变现象          下载免费PDF全文

李超  王鹏举  李小波  杨雪娟  肖化平 《天文学报》2022,63(2):13-12

利用“慧眼”(Hard X-ray Modulation Telescope, Insight-HXMT)卫星在2017年9月对黑洞候选体MAXI J1535-571的观测数据,研究了该源在爆发期内的时变现象.当源处于不同的爆发谱态时,功率密度谱的谱型存在明显差异.在硬中间态,有明显的限带噪声(band-limited noise)成分和QPO (Quasi-Periodic Oscillation)成分.分析结果表明:低频限带噪声的特征频率随能量的变化呈现正相关,即软能段光子的特征频率小于硬能段光子的特征频率. 0.1–0.5 Hz频率区间的限带噪声RMS (Root Mean Square)谱在硬中间态和软中间态均出现峰值,且在高能端存在差异,可能是主导噪声RMS的能谱成分占比不同.当谱态由硬中间态过渡到软中间态时, C型QPO的RMS谱保持相似趋势,但限带噪声RMS谱存在谱态依赖现象,暗示着噪声和QPO有不同的起源机制.  相似文献