Sq(H) field variations at Sonmiani geomagnetic observatory,Pakistan for solar cycle 24

In this study, Sq(H) field results for Sonmiani geomagnetic observatory (SON), Pakistan are presented first time for solar cycle i.e., Solar Cycle 24. Sonmiani observatory was established in 2008 and was included in the list of INTERMAGNET Magnetic Observatory (IMO) in 2012. The analysis of Sq(H) field is performed to examine diurnal, annual and seasonal behaviour of Sq(H) field at Sonmiani along with Honolulu which is used as reference observatory. Both the observatories lie at the Equatorial Ionisation Anomaly (EIA) crest. In general strong dependency of Sq(H) field on solar cycle has been observed. First peak of SC24 was visible in Sq(H) field at both observatories. However, at HON maximum Sq(H) was observed in 2015 instead of 2014, a year later than the year of solar maximum. Prominent longitudinal difference has been noted between both observatories. At HON, maximum Sq(H) was observed during equinox while at SON it was noted during equinox and summer as a consequence of shift in latitude of Sq focus. Phase shift of Sq(H) at SON followed a general trend, that is maximum Sq(H) shifted to later hours in solar maximum as compared to solar minimum. Whereas, an opposite trend was noted at HON which might be due to coastal effect. In case of seasonal phase shift, at both observatories maximum Sq(H) occurred at later hours in summer than in winter which is opposite to the results obtained by many workers. These points need further investigation and geomagnetic as well as wind, and electric field data of other observatories situated at the EIA crest region is required to interpret the Sq(H) phase shift extensively.     

Simulation of the land surface temperature from moon-based Earth observations

The land surface temperature (LST) is a key parameter for the Earth’s energy balance. As a natural satellite of the Earth, the orbital of the moon differs from that of current Earth observation satellites. It is a new way to measure the land surface temperature from the moon and has many advantages compared with artificial satellites. In this paper, we present a new method for simulating the LST measured by moon-based Earth observations. Firstly, a modified land-surface diurnal temperature cycle (DTC) method is applied to obtain the global LST at the same coordinated universal time (UTC) using the Moderate Resolution Imaging Spectroradiometer (MODIS) LST products. The lunar elevation angles calculated using the ephemeris data (DE405) from the Jet Propulsion Laboratory (JPL) were then applied to simulate the Earth coverage observed from the moon. At the same time, the modified DTC model was validated using in situ data, MODIS LST products, and the FengYun-2F (FY-2F) LST, respectively. The results show that the fitting accuracy (root-mean-square error, RMSE) of the modified DTC model is not greater than 0.72?°C for eight in situ stations with different land cover types, and the maximum fitting RMSE of the modified model is smaller than that of current DTC models. By the comparison of the simulated LST with MODIS and FY-2F LST products, the errors of the results were feasible and accredited, and the simulated global LST has a reasonable spatiotemporal distribution and change trend. The simulated LST data can therefore be used as base datasets to simulate the thermal infrared imagery from moon-based Earth observations in future research.     

Ascent guidance law for a horizontal take-off vehicle with a multi-combined cycle engine

This paper researches the ascent guidance law for the vehicle with a multi-combined cycle propulsion. The guidance law comprises two parts, namely, the off-line optimal trajectories generation and online guidance. With respect to the off-line part, disturbances are discretized and incorporated into the trajectory optimization problem; subsequently, a set of trajectories is calculated to constitute a database. To quickly obtain a database that comprises a large number of trajectories, a novel ascent profile is proposed with respect to height and velocity. Based on this profile, only inequity constraints exist in the optimization model, and the original optimization problem is converted to a parameter searching problem. The optimal trajectories are calculated using a hybrid optimization method that comprises a particle swarm optimization (PSO) method and the Hooke-Jeeves (HJ) method. With respect to online guidance, the profile is updated using a radial basis function neural network (RBFNN) based on the current flight states and the database. Simulation validates the efficiency of the proposed optimization method by comparing the method with the pseudospectral method; the robustness of the guidance law is also validated using Monte Carlo simulation.     

燃气发生器循环变推力发动机频率响应分析

采用分段集中参数的有限元方法建立了发动机模块化模型,以此模型搭建了燃气发生器循环液体火箭发动机仿真模型,对变推力发动机在变工况下的系统特征及频率响应进行了研究。研究表明:发动机系统在变工况后系统特征频率及其对应的阻尼系数有明显变化。通过提取变工况过程中的主要频率,发现对应能量峰值的频率为5.34 Hz。在发动机系统工况转换过程中,输入带有该频率的扰动的入口压力信号,仿真结果证明这种低频扰动使系统稳定裕度降低,应当避免该频率下扰动信号出现。     

Spectra of the two official GLEs of solar cycle 24

Based on ground-level data and on satellite data we determine in this work the observational spectrum of both, the Ground Level Enhancement of May 17, (2012) the so-called GLE71 and the Ground Level Enhancement of September 10, 2017 (GLE 72). We describe a simplified method to obtain the experimental spectrum at ground level. Data of the GLE71 and GLE72 indicate the presence of two different populations, each one with a different energy spectrum. On the other hand, we explore the kind of phenomena that take place at the source in these two particular events. In contrast with other methods based on the temporal synchronization between electromagnetic emissions of flares and coronal mass ejections (CME), here we develop an alternative option based on the study of the accelerated particles, by adjusting our theoretical spectra to the observational spectra. The main results of this work are the derivation of the source and acceleration parameters involved in the generation process. These results lead us to construct possible scenarios of particle generation in the source for each one of the two studied GLEs.     

三角翼大攻角绕流数值模拟研究

采用Harten-Yee的二阶精度隐式TVD格式对N-S方程进行数值模拟,研究了后掠角为65°和70°的三角翼绕流的流场特性。计算结果表明：TVD格式中限制器函数的选取对于三角翼绕流结构的计算结果具有较重要的影响。结合张涵信的旋涡定性分析理论对旋涡的发展过程进行研究,此外,还对二次涡破裂现象和网格分布影响等问题进行了探讨。     

一种新的速率陀螺测试方法

主要介绍了用力矩电流法对速率陀螺进行测试及其数学模型的辨识,为速率陀螺的动态测试提供了一种新的方法。试验结果表明,该方法是可行的。     

组网卫星电推进自主轨道保持方法

以某对地观测星座任务为背景,对基于电推进的组网卫星自主轨道保持控制方法进行研究.由地面进行标称轨道递推并定期上注,星上考虑地球非球形J2项摄动进行本星和标称星拟平均轨道参数递推,采用单边极限环方法进行面内相位保持控制.针对长期运行在对日定向模式的倾斜轨道且固定太阳翼卫星,考虑能源、程控任务、轨道偏心率等约束,设计了卫星...     

高温低周应变疲劳的三参数幂函数能量方法研究

 对Manson-Coffin方程、拉伸滞后能寿命模型和三参数幂函数公式进行了应用研究,提出了三参数幂函数能量方法,并用某高温合金900  ℃低周疲劳数据进行了验证研究。通过寿命预测分散带和标准差的比较发现：三参数幂函数能量方法的低周疲劳寿命预测能力较Manson-Coffin方程和三参数幂函数公式的寿命预测能力有较大的提高;用三参数幂函数能量方法确定的循环应力-应变曲线比用Manson-Coffin方程处理得到的塑性应变分量确定的循环应力-应变曲线更能反映低周疲劳过程中应力和应变之间的关系。     

涡轮叶片榫齿部位疲劳/蠕变试验的新特点

在某型航空发动机涡轮叶片的低周疲劳试验中发现, 叶片疲劳/蠕变试验寿命高于纯疲劳试验寿命, 为探究这一现象的原因, 对此展开相关的理论计算和分析.研究表明:试验条件较好地模拟了叶片的实际工作条件, 该涡轮叶片的损伤以疲劳损伤为主, 相对于真实涡轮叶片的纯疲劳试验, 在疲劳/蠕变试验条件下, 其考核部位(榫齿)出现了较大的应力松弛, 故而使得叶片疲劳/蠕变寿命高于纯疲劳寿命.研究结果对于保证发动机安全工作、提高飞行可靠性、以及发展高温构件的疲劳试验技术有重要意义.