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661.
Madeeha Talha Ghulam Murtaza Jean L. Rasson Nabeel Ahmed Mahrukh Peerzada 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2021,67(1):66-74
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. 相似文献
662.
Chenwei Nie Jingjuan Liao Guozhuang Shen Wentao Duan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(2):826-839
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. 相似文献
663.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):379-391
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. 相似文献
664.
665.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(1):663-676
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. 相似文献
666.
667.
一种新的速率陀螺测试方法 总被引:3,自引:2,他引:1
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。 相似文献
668.
669.
高温低周应变疲劳的三参数幂函数能量方法研究 总被引:10,自引:0,他引:10
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。 相似文献
670.
涡轮叶片榫齿部位疲劳/蠕变试验的新特点 总被引:2,自引:1,他引:1
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. 相似文献