太阳帆绕地球周期轨道研究

  地球同步和太阳同步卫星在各个领域有着广泛的应用。静止轨道是一种特殊的地球同步轨道,轨道资源有限。利用化学推进或电推进可以实现轨道高度不同的同步轨道,如悬挂轨道,但需要消耗较多的燃料,工程上无法承受。本文考虑利用太阳帆实现地球同步和太阳同步轨道。太阳光压力在轨道平面内沿拱线方向,选择光压力与平面的夹角使得轨道平面的旋转速率与太阳光同步。研究表明,设计合适的半长轴和偏心率可以使得轨道旋转速率与地球自转速率一致。假设太阳光与赤道平面平行,可以得到准静止轨道,太阳帆将在传统静止轨道的附近运动,星下点的经度将在一个固定值附近振动。实际上太阳光是与黄道面平行,黄道面与赤道面之间存在夹角。考虑黄赤交角的情况下,太阳帆将在一定纬度和经度范围内运动。适合于对某个区域进行长期观测任务。     

Changes in total electron content (TEC) during the annular solar eclipse of 15 January 2010

The solar eclipse of 15 January 2010 was an annular eclipse of the Sun with a maximum magnitude of 0.96 at 1.62°N, 69.29°E. To study the effect of this solar eclipse on the ionosphere the GPS data recorded at three different Indian stations Varanasi (Geographic latitude 25°, 16′N, longitude 82°, 59′E), Hyderabad (Geographic latitude 17°, 20′N, longitude 78°, 30′E) and Bengaluru (Geographic latitude 12°, 58′N, longitude 77°, 33′E) have been used to retrieve ionospheric total electron content (TEC). The ionospheric response to this rare event has been studied in terms of GPS-derived TEC observed at all the three Indian stations. A significant reduction in TEC reflected by all PRNs at all the three stations has been observed. The magnitude of the reduction in VTEC compared to quiet mean VTEC depends on latitude as well as longitude. The amount of reduction observed from different satellites (PRN) is different and depends on the location of the satellite from the solar eclipse path.     

某于功率反馈的涡轴发动机神经网络PID控制研究

通过对功率平衡关系进行分析,提出了利用功率反馈设计智能神经网络PIO控制器的方法。基于BP(Back Propagation)神经网络,将功率信号作为神经网络的输入层信号,并改进了网络权值的学习规则。通过在线整定PID参数,控制器能够根据功率误差信号的变化实时调整控制参数,从而使系统自主寻找到功率平衡点,具有良好的稳态和动态响应特性。仿真结果表明：该方法可以使涡轴发动机在全包线范围内具有理想的控制性能。     

LEO卫星电源系统拓扑研究

基于30个近地轨道（LEO）卫星任务及其电源系统应用情况,在系统层面上对5种电源系统拓扑进行了分析比较,包括配置方式、控制原理、效率及器件等。针对功率调节性能和器件组成规模,选择配有最大功率点跟踪（MPPT）的升一降压调节器（B2R）作为多适用的电源系统拓扑。此系统适应LEO卫星需求,属于拓扑用途广泛的电源系统,可通过合理配置热备份的功率调节模块来实现功率组合及可靠性设计,具有较高的兼容性,能够满足中国LEO卫星任务需求。     

On the variabilities of the Total Electron Content (TEC) over the Indian low latitude sector

The Total Electron Content (TEC) from four locations in the Indian sector namely, Trivandrum (8.47°N, 76.91°E, Geomag.0.63°S, 0.3° dip), Waltair (17.7° N, 83.3°E, Geomag. 6.4°N, 20° dip), Bhopal (23.28°N, 77.34°E, Geomag.14.26°N, 33.2° dip), and Delhi (28.58°N, 77.21°E, Geomag.19.2°N, 43.4° dip) during a low sunspot year of 2004 are used to study the variabilities of the TEC. The day time TEC values are higher over Waltair and Bhopal compared to those at Trivandrum and Delhi. Considerable day-to-day variations in the diurnal values of TEC are observed at the anomaly crest locations. The observed GPS-TEC has been compared with the IRI-2007 model derived TEC considering three different options (IRI-2001, IRI-2001 corrected and Ne-Quick) available in the model for the topside electron density. The TEC derived with Ne-Quick and IRI-01 corrected options show better agreement with GPS-TEC while the TEC from IRI-01 method shows larger deviations. From the correlation analysis carried out between TEC value at 1300 h LT and solar indices parameters namely sunspot number (SSN), F10.7 and EUV, it is observed that the correlation is more during equinoctial months and less during summer months. The correlation coefficients observed over the anomaly locations, Bhopal and Delhi are lower compared to those at Trivandrum and Waltair.     

Correction of B2bot for NeQuick during low solar activity at Hainan station

This work is a continuation of the previous article and it focuses on low solar activity and modeling effort. NeQuick model uses Epstein layer formalism to model each part of the profile. We study the diurnal and seasonal variations of B2_bot, ΔB2 (B2_best − B2_NeQuick2) and R (B2_best/B2_{NeQuick 2}) at Hainan station during low solar activity. The results show it is possible to improve the B2_bot parameter of the NeQuick model at that region during low solar activity. Then, we use a function ?(t) with LT in different seasons to correct the B2_bot formula of NeQuick 2. The correction shows that (1) By the correction formula, the B2_bot of NeQuick is improved. The maximum standard deviation is improved for 9 km. (2) The correction formula is more effective in summer than in equinox and winter and performs better during early morning hours than during the rest of the day.     

Near 13.5-day periodicity in Muon Detector data during late 2001 and early 2002

In this study we perform a continuous Morlet wavelet transform method in time series of secondary cosmic rays and 1 AU interplanetary medium parameters for the interval from October 2001 to October 2002. The near 13.5-day periodicity was obtained during late 2001, and it was remarkable for muon data. Even though some works have pointed out that the main activations of the 13.5 day recurrence in near-Earth solar wind are related, e.g., with the heliosheet crossings or to the occurrence at 1 AU of two high speed streams approximately 180° apart in solar longitude per solar rotation, we aim to show that the period of about half the solar rotation during the end months of 2001 present in muon time series was apparently due to the occurrence of non-recurrent interplanetary disturbances. The interconnections among successive Forbush decreases, recovery phases and gradual muon depressions (associated with corotating interaction regions) seem to play an important role in such 13.5-day periodicity.     

中国微藻航空煤油制备潜能及CO2减排

综合考虑中国各地温度变化、水资源和CO₂的供给能力等因素,分析了中国适合微拟球藻规模化养殖的地区;根据2013年沿海地区燃煤发电排放CO₂量,结合蓬莱地区微拟球藻规模化养殖的实际数据,预测了中国微藻的年产量潜力及在现有技术水平下利用这些微藻原料可制备航空煤油的潜力;并采用全生命周期模型GREET计算了微藻航空煤油相比传统石油基航空煤油在全生命周期内中可减少CO₂的排放量。结果表明:目前中国具有每年8894万t的微藻养殖潜力,这些微藻共可制备航空煤油1917万t;与传统航煤相比,制备1 t微藻航空煤油在全生命周期内相比传统航空煤油可降低CO₂排放2.28 t。     

波音737NG飞机后缘襟翼常见故障分析及解决措施

针对波音737NG系列飞机运行期间常见的后缘襟翼系统典型故障进行了分析与整理,总结并提出了一些实践中可行的改进方法和措施。     

在片功率参数校准方法研究

针对在片功率参数的校准需求,分析如何通过矢量方法修正由于微波探针和功率计引入的失配误差,并推导相关修正公式。同时对在片功率测量矢量修正中涉及的微波探针S参数提取方法做介绍,并将试验提取的S参数与微波探针的出厂数据比较。最后将在片功率参数测量的矢量修正数据分别与标量修正数据和未修正数据比较,结果表明,在40GHz内,运用矢量修正得到的在片功率参数测量结果准确度较未修正结果提高0.4dB,较标量修正结果提高0.1dB。