A complete relativistic ionized accretion disc in Cygnus X-1

The galactic black hole candidate Cygnus X-1 is observed to be in one of two X-ray spectral states: either the low/hard (low soft X-ray flux and a flat power-law tail) or high/soft (high blackbody-like soft X-ray flux and a steep power-law tail) state. The physical origin of these two states is unclear. We present here a model of an ionized accretion disc, the spectrum of which is blurred by relativistic effects, and fit it to the ASCA , Ginga and EXOSAT data of Cygnus X-1 in both spectral states. We confirm that relativistic blurring provides a much better fit to the low/hard state data and, contrary to some previous results, find the data of both states to be consistent with an ionized thin accretion disc with a reflected fraction of unity extending to the innermost stable circular orbit around the black hole. Our model is an alternative to those that, in the low/hard state, require the accretion disc to be truncated at a few tens of Schwarzschild radii, within which there is a Thomson-thin, hot accretion flow. We suggest a mechanism that may cause the changes in spectral state.     

不同反应参数下纤蛇纹石纳米管的水热合成研究

以活性MgO和纳米SiO2为原料,在仿地质作用的碱性水热环境下控制不同反应参数合成了多个系列的纤蛇纹石样品。利用XRD和IR分析系统地研究了不同反应参数对纤蛇纹石特征的影响。结果表明,活性MgO和纳米SiO2在水热环境中很容易转变成纤蛇纹石相,但形成完善纳米管结构须严格控制水热反应条件;pH值、反应温度和反应时间的提高均有利于水热合成结晶度及管状结构更加完善的纤蛇纹石,最佳水热反应条件为pH=13.8,200℃,反应60h,此条件下无其它杂质产物生成,合成温度较前人采用的300℃有所降低。利用SEM和AFM对最佳反应条件下合成的纤蛇纹石纳米管的形貌进行了观察,发现其为短柱状,准直性较高,表面光洁无杂质,直径均一,约50nm,长度多为400～500nm。     

基于剪切波速的深层砂土地震液化研究

阐述了剪切波速法判别饱和砂土液化的原理,结合武汉地区某工程实例,对场地内埋深超越"规范法"适用范围的砂层进行液化判别,确定场地的临界液化深度。通过与室内动三轴试验的对比得出,2种方法的液化判别结果及确定的临界液化深度均吻合较好,验证了以剪切波速为指标的液化评估方法的可行性。     

埋深对恐龙化石的影响效果研究

已发现的恐龙化石大多数埋藏在不同深度的地层中,不同埋深化石所受风化破坏程度不尽相同。为深入研究恐龙化石的风化机理,探究恐龙化石的保护措施和方法,重点分析埋深产生的侧向压力对恐龙化石强度和破坏特性的影响。通过有限差分软件FLAC3D进行数值模拟,揭示埋深因素对恐龙化石保存的影响程度。试验结果表明:围岩对恐龙化石施加的侧向压力是影响恐龙化石变形和强度特性的一个重要因素。在弹性变形阶段,恐龙化石的初始强度、峰值强度随侧向压力的增大而不断增大。当应力超过了恐龙化石极限强度后进入塑性变形,其初始强度、峰值强度逐渐减小,最终达到残余强度。     

关于山东省地热尾水回灌试验的应用研究

为解决地热水开采利用过程中造成诸如水位下降、热流体排放引起的热污染和化学污染等问题,通过开展地热尾水回灌试验研究,认为在开采深层的地下热水资源的同时,必须进行人工的回灌补源,山东省通过在德州、东营、济南等地开展地热尾水回灌试验工作,效果显著。     

常顶瓦斯油吸附法脱除微量氯的实验研究

炼油厂将常压塔顶油和减一线油作为重整原料,但由于氯含量过高(30×10-6)无法利用,传统方法是将其中的有机氯转化为无机氯化氢后脱除,但其对加氢催化剂有毒害,采用常顶瓦斯油吸附法可直接脱除微量氯。     

基于STC单片机的实验开发平台的设计

介绍了基于STC89C516RD＋单片机的实验开发平台的硬件电路设计、ISP编程、软件开发实例及系统的抗干扰措施.为帮助学生学习单片机技术,同时也为有经验者开发和调试产品打下基础.     

Effects of Kerr space–time on spectral features from X-ray illuminated accretion discs

We performed detailed calculations of the relativistic effects acting on both the reflection continuum and the iron line from accretion discs around rotating black holes. Fully relativistic transfer of both illuminating and reprocessed photons has been considered in Kerr space–time. We calculated overall spectra, line profiles and integral quantities, and present their dependences on the black hole angular momentum. We show that the observed EW of the lines is substantially enlarged when the black hole rotates rapidly and/or the source of illumination is near above the hole. Therefore, such calculations provide a way to distinguish between different models of the central source.     

The 'off' state of GX 339–4

We report BeppoSAX and optical observations of the black hole candidate GX 339–4 during its X-ray 'off' state in 1999. The broad-band (0.8–50 keV) X-ray emission can be fitted by a single power law with spectral index, α ∼1.6. The observed luminosity is 6.6×10³³ erg s⁻¹ in the 0.5–10 keV band, which is at the higher end of the flux distribution of black hole soft X-ray transients in quiescence, comparable to that seen in GS 2023+338 and 4U 1630–47. An optical observation just before the BeppoSAX observation shows the source to be very faint at these wavelengths as well ( B =20.1, V =19.2). By comparing with previously reported 'off' and low states (LS), we conclude that the 'off' state is actually an extension of the LS, i.e. an LS at lower intensities. We propose that accretion models such as the advection-dominated accretion flows are able to explain the observed properties in such a state.