Results of solar observations by the CORONAS-F payload

The CORONAS-F mission experiments and results have been reviewed. The observations with the DIFOS multi-channel photometer in a broad spectral range from 350 to 1500 nm have revealed the dependence of the relative amplitudes of p-modes of the global solar oscillations on the wavelength that agrees perfectly well with the earlier data obtained in a narrower spectral ranges. The SPIRIT EUV observations have enabled the study of various manifestations of solar activity and high-temperature events on the Sun. The data from the X-ray spectrometer RESIK, gamma spectrometer HELICON, flare spectrometer IRIS, amplitude–temporal spectrometer AVS-F, and X-ray spectrometer RPS-1 have been used to analyze the X- and gamma-ray emission from solar flares and for diagnostics of the flaring plasma. The absolute and relative content of various elements (such as potassium, argon, and sulfur) of solar plasma in flares has been determined for the first time with the X-ray spectrometer RESIK. The Solar Cosmic Ray Complex monitored the solar flare effects in the Earth’s environment. The UV emission variations recorded during solar flares in the vicinity of the 120-nm wavelength have been analyzed and the amplitude of relative variations has been determined.     

地球同步轨道薄膜太阳帆的姿态轨道控制方法

薄膜太阳帆（FSS）是集推进、发电和姿轨控功能于一体化的超大型挠性太阳帆式航天器，通过调整薄膜反射率产生可变推力和力矩，实现其姿态和轨道运动控制。结合薄膜太阳帆在地球同步轨道运行时的受力特性进行了轨道漂移分析。通过建立薄膜太阳帆动力学模型及受力模型，提出了调整帆面角度轨道修正方法以及基于薄膜光压力矩角动量卸载的长期在轨对日定向面内双轴动量轮稳定控制方法。通过系统仿真验证表明所提的轨道修正和对日定向控制方法是合理有效的，可使薄膜太阳帆长期在定点位置维持对日定向。     

Sunspot activity and cosmic ray modulation at 1 a.u. for 1900–2013

The descent of sunspot cycle 23 to an unprecedented minimum of long duration in 2006–2009 led to a prolonged galactic cosmic ray (GCR) recovery to the highest level observed in the instrumental era for a variety of energetic charged particle species on Earth, over a wide range of rigidities. The remarkable GCR increase measured by several ground-based, balloon-borne, and detectors on a satellite is described and discussed. It is accompanied by a decrease in solar wind velocity and interplanetary magnetic field at 1 a.u., reaching the lowest values since measurements of the solar wind began in October 1963; the solar polar field strength (μT) measured at the Wilcox Solar Observatory (WSO) is also significantly reduced compared to prior cycles since the start of the program in 1976, the polar field in the northern hemisphere reversed in June 2012 and again in February 2014, that in the southern hemisphere reversed in July 2013. If updates of WSO data confirm the second reversal in northern solar hemisphere, it would pose a serious challenge to the Dynamo Theory. The long-term change in solar behavior may have begun in 1992, perhaps earlier. The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified. The study discusses the recent phenomena in the context of GCR modulation since 1900. These happenings affected our empirical predictions for the key parameters for the next two sunspot cycles (they may be progressively less active than sunspot cycle 24) but it enhanced support for our prediction that solar activity is descending into a Dalton-like grand minimum in the middle of the twentyfirst century, reducing the frequency of the coronal mass ejections; they determine the space weather affecting the quality of life on Earth, radiation dose for hardware and human activities in space as well as the frequency of large Forbush decreases at 1 a.u.     

Sunspot cycle 23 descent to an unusual minimum and forecasts for cycle 24 activity

The decay phase of the sunspot cycle 23 exhibited two unusual features. First, it lasted too long. Second, the interplanetary magnetic field intensity at earth orbit reached the lowest value since in situ measurements in space began in October 1963. These physical anomalies significantly altered the early forecasts for the sunspot activity parameters for cycle 24, made by several colleagues. We note that there was a significant change in the solar behavior during cycle 22. We discuss the observed trends and their effect on our empirical solar activity forecast technique, leading to our prediction for cycle 24 parameters; cycle 24 will be only half as active as cycle 23, reaching its peak in May 2013. We speculate on the possible implications of this outcome on future earth climate change and the ensuing socio-economic consequences.     

飞机高温高压空气导管的振动特性研究

在分析某大型客机环境控制系统的配平子系统的基础上,基于有限元软件Patran和Nastran建立了配平系统的空气导管有限元分析模型,选用Lanczos算法,对管系进行动力学模态分析,获得了系统前五阶的频率和振型.同时,考察了气体热力学参数和球形接头作动力学参数对空气导管动力学模态特性的影响.结果表明:从频率上看,配平系统Part1在45Hz以下谐振模态分布密集.从振型上看,球形接头和滑动接头处的振型变化幅度较大;从动力学特性的影响因素来看,配平系统空气导管管系的固有频率随管内温度的增加而递减,随管内压力的增加而增加;球形接头起动力矩和刚度增大会增加各阶的固有频率.研究工作对于我国大型客机空气导管系统的可靠性设计具有参考价值.     

军航活动下扇区动态容量评估研究

民航业迅速发展,空域资源的稀缺性日益凸显。科学合理地评估空域容量是解决空中交通流量瓶颈的关键,同时也为制定流量管理策略提供科学的依据。由于我国体制的特殊性,军航活动一直是我国空域资源限制的重要因素。研究并详细分析军航活动对扇区容量损失作用的机理,定量地评估军航活动对扇区容量的影响,建立军航活动影响下的扇区动态容量评估模型,结论表明模型有一定的参考意义。     

A100钢外螺纹椭圆超声滚压强化试验研究

A100钢有较高的疲劳抗力和显著的减重效果.在航空工业中,飞机起落架主要承力件正逐步采用A100钢,且主要承力件多采用螺纹联接.为了提高螺纹疲劳寿命,提出了超声振动滚压强化工艺方法,设计了外螺纹超声滚压强化装置,进行了螺纹超声滚压强化前后性能对比试验.利用X射线分析仪、维式硬度计、粗糙度仪和疲劳试验机,分别测量了螺纹超声滚压强化前后的残余应力、维氏硬度、表面粗糙度以及疲劳寿命.结果表明,超声滚压强化后牙底残余应力提高了70％,显微硬度提高了14％,粗糙度降低了51％,600MPa应力条件下寿命提高了5倍.     

大阻尼高刚度复合材料仪表板的设计结构与工艺研究

设计了一种五层夹芯多层阻尼薄膜嵌入的复合材料仪表板结构,并采用多次热压罐固化成型工艺来制作该大阻尼高刚度复合材料仪表板.它们分别是:上、下蒙皮和中心层的制作,上、下蒙皮和中心层与泡沫塑料的粘接与紧固件的预埋,孔的修正及仪表板的包边加工.通过成形质量检验和加载试验,验证了成形工艺的可行性和合理性.     

先进材料与工艺在机载导弹上的研究与应用

先进材料和工艺在机载导弹中的应用是实现机载导弹优异性能的基础和前提.主要讨论了用于机载导弹的复合材料、高温钛合金、铝锂合金、金属间化合物等先进材料和近无余量成形、超精密加工等先进工艺的特点以及国内外的发展概况.     

冷坩埚定向凝固TiAl基合金高温持久性能研究

采用电磁冷坩埚定向凝固技术制备了成分为Ti-47A1-2Cr-2Nb的合金铸锭,定向凝固后的显微组织为α2+γ全片层结构.在0.4～1.2mm/min的抽拉速率范围内,随着抽拉速率的增加,片层间距减小,柱状晶与生长方向的夹角增大.随着温度升高,合金的拉伸强度有所下降,但由于细化片层界面对切变应力变形的阻碍作用,合金的高温拉伸强度会随着抽拉速率的增加而提高.通过对抽拉速率为1.0mm/min试样的拉伸强度与温度的拟合,得到了拉伸强度和温度之间的函数关系.随着抽拉速率的增加,Ti-47A1-2Cr-2Nb合金的持久寿命明显升高,对于抽拉速率为1.2mm/min试样的持久性能测试表明,其持久寿命最长,达到了48h.持久试样的断口形貌表明,其断裂的主要方式是伴随着少量延性断裂的脆性解理断裂.最后根据时间-温度模型,分别采用Larson-Miller和Manson-Haferd参数法建立了定向凝固Ti-47Al-2Cr-2Nb合金的持久强度预测函数模型,预测的理论值与试验结果吻合度较高.