X-ray bursts associated with envelope expansion

The precursor associated with a long X-ray burst is interpreted in terms of the stellar envelope expansion. The mass flow driven by the radiation pressure in excess of the local Eddington limit and the grey atmosphere model correctly describe the burst profiles in different energy ranges.     

修正平均应力法预测轮盘破裂转速的试验研究

基于修正平均应力法,分析了TC17钛合金压气机轮盘型面尺寸参数对径向和周向破裂转速的影响,并对破裂模式的转变进行预判。进而设计了针对径向破裂模式的轮盘试验件,并开展了TC17钛合金压气机轮盘的破裂试验。轮盘破裂试验结果与修正平均应力法计算结果吻合较好,计算的破裂转速储备与试验结果的误差由修正前的7.24%下降为修正后的0.72%,可为工程应用提供依据。     

减涡器破裂转速预测方法及试验验证

采用数值分析同试验相结合的方法研究了减涡器破裂转速问题。根据减涡器支撑环孔边的应力状态,设计了支撑环结构的模拟试验件,开展了单调拉伸载荷下的破坏试验,得到了体现结构应力特征的破坏参数。进而基于有限元方法,将模拟试验件的破坏参数引入减涡器支撑环破裂转速预测中,并对比了不同破裂准则对破裂转速预测结果的影响。分析表明:所设计的模拟试验件与减涡器支撑环的应力梯度吻合较好,可准确描述结构应力特征;局部塑性法和基于材料强度的方法预测破裂转速时结果更为保守,分别比平均应力法的预测值低15%和23%,对此类结构的破裂分析具有工程参考价值。      

自适应阈值突发模式光接收机的性能分析

在考虑判决阈值的衰落时间和噪声特性对光接收机性能的影响后,提出了一种分析突发模式光接收机误码性能的综合模型,并分析了与传统的交流耦合光接收机相比较时,突发模式光接收机的灵敏度损失.     

A statistical study of solar radio Type III bursts and space weather implication

Solar radio bursts (SRBs) are the signatures of various phenomenon that happen in the solar corona and interplanetary medium (IPM). In this article, we have studied occurrence of Type III bursts and their association with the Sunspot number. This study confirms that occurrence of Type III bursts correlate well with Sunspot number. Further, using the data obtained using e-CALLISTO network, we have investigated drift rates of isolated Type III bursts and duration of the group of Type III bursts. Since Type II, Type III and Type IV bursts are signatures of solar flares and/or CMEs, we can use the radio observations to predict space weather hazards. In this article, we have discussed two events that have caused near Earth radio blackouts. Since e-CALLISTO comprises more than 152 stations at different longitudes, we can use it to monitor the radio emissions from the solar corona 24 h a day. Such observations play a crucial role in monitoring and predicting space weather hazards within few minutes to hours of time.     

“Ⅳ型”激波干扰中流-热-固耦合问题一体化计算分析

针对高超声速进气道前缘"Ⅳ型"激波干扰产生的气动加热与结构传热多物理场耦合计算问题，发展了一种基于有限体积法的流-热-固一体化计算方法。该方法采用一体化控制方程组统一离散求解外部高速流场与内部结构温度场，规避了传统分区耦合算法在时间域内交替迭代的繁琐数据交换策略。另外，提出一种新的双温阻模型计算流-固交界面的物性参数以保证计算准确性，采用LU-SGS隐式时间迭代和自适应时间步长以提高计算效率。采用经典高超声速二维圆管流-热-固耦合算例对该一体化方法进行验证，计算结果与试验值和参考文献数据吻合较好，证明了该方法的可靠性和正确性。利用一体化方法对高超声速前缘"Ⅳ型"激波干扰流-热-固耦合问题进行定常/非定常计算与分析，给出了温度与热流的时变特性，计算结果表明，激波干扰作用产生的超声速"喷流"不断冲击壁面，使得壁面最大压力系数增大约9倍，壁面最大热流增大约4.7倍，给高速飞行器的热防护设计与选材带来严峻挑战。同时，也表明了一体化计算方法可以较好地用于长航时飞行条件下与复杂飞行环境下的高超声速热防护系统的热环境特性分析与综合性能评估。     

A highly-ionized absorber as a new explanation for the spectral changes during dips from X-ray binaries

We report the XMM-Newton detection of narrow Fe xxv and Fe xxvi X-ray absorption lines at 7 keV in the persistent emission of the dipping low-mass X-ray binary (LMXB) 4U 1323−62. Such features have now been reported in a growing number of LMXBs seen almost edge-on, indicating that the highly-ionized plasma probably originates in an accretion disk atmosphere or wind. During dipping intervals of 4U 1323−62, the strength of the Fe xxv feature increases while that of the Fe xxvi feature decreases, consistent with the presence of less strongly ionized material in the line-of-sight. As observed previously, the changes in the X-ray spectrum during dips are inconsistent with a simple increase in absorption by cool material. However, we show that the changes in both the narrow absorption features and the continuum can be modeled self-consistently by variations in the properties of an ionized absorber. From persistent to deep dipping the photo-ionization parameter decreases while the equivalent hydrogen column density of the ionized absorber increases. No partial covering of any component of the spectrum, and hence no extended corona, are required. Since highly-ionized absorption features are seen from many other dip sources, this mechanism may also explain the overall changes in X-ray spectrum observed during dipping intervals from these systems.     

Source investigation of impulsive He-rich particle events

We have investigated the source characteristic and coronal magnetic field structure of six impulsive solar energetic particle (SEP) events selected from Wang et al. [Wang, Y.-M., Pick, M., Mason, G.M. Coronal holes, jets, and the origin of ³He-rich particle events. ApJ 639, 495, 2006] and Pick et al. [Pick, M., Mason, G.M., Wang, Y.-M., Tan, C., Wang, L. Solar source regions for ³He-rich solar energetic particle events identified using imaging radio, optical, and energetic particle observations. ApJ 648, 1247, 2006]. Some results are obtained: first, 2 events are associated with wide (≈100°) CMEs (hereafter wide CME events), another 4 events are associated with narrow (?40°) CMEs (hereafter narrow CME events); second, the coronal magnetic field configuration of narrow CME events appear more simple than that of the wide CME events; third, the photospheric magnetic field evolutions of all these events show new emergence of fluxes, while one case also shows magnetic flux cancellation; fourth, the EUV jets usually occurred very close to the footpoint of the magnetic field loop, while meter type III bursts occurred near or at the top of the loop and higher than EUV jets. Furthermore, the heights of type III bursts are estimated from the result of the coronal magnetic field extrapolations.     

一种基于DFT的高精度载波频偏估计算法

针对无线数字通信中的载波频率同步问题,提出一种新的载波频偏估计算法。利用离散傅里叶变换（DFT）内插技术,在较大频偏范围内估计出载波频偏,并且在估计精度上相对于DFT法有了很大的提高。这种算法不需要增加DFT数据长度,适合突发通信方式。进行了Monte Carlo仿真实验,仿真结果表明新算法不仅具有宽的估计范围,还具有高的估计精度。     

指数寿命型可靠性增长试验的Bayes分析

该文论述了指数寿命型可靠性增长试验中的Bayes分析方法。文中首先给出了可靠性分析的模型，然后运用历次阶段性试验中的可靠性增长数据建立动态参数模型，在此基础上给出各阶段可靠性增长试验中失效率的Bares估计。