Structure of the Program of Short-term Prediction of Powerful Solar Flares

Input data of the system are two-dimensional images and one-dimensional distributions of total and polarized solar emission at 5.2 cm wavelength obtained with SSRT. Together with photoheliograms, magnetograms, Hα-filtergrams and characteristics of active regions received from other sources, they form the initial database. The first stage includes superimposing the images, identifying microwave sources with active regions, assigning NOAA numbers to the sources, and determining for each active region the heliolatitude, extent, and inclination angle of the group's axis to the equator. These data are used to calculate the boundaries of longitude zones for each active region. A next stage involves determining the brightness temperatures of microwave sources less than the polarization distribution, the degree of polarization, and microwave emission flux, as well as calculating the parameters of microwave sources. Each parameter is assigned its own value of the weight factor, and the sum of values is used to draw the conclusion about the flare occurrence probability in each active region and on the Sun in general.      

Experimental Study on Emission Performance of an LPP/TVC

A key issue in the commercial aircraft engine design is environmental acceptability, and designers are continually challenged to reduce emissions. In this paper, an experimental investigation is performed to evaluate the emission performance of a liquid-fueled trapped vortex combustor (TVC) under lean premixed prevaporized (LPP) mode. When operating as an LPP system, a TVC is fueled both in the cavities and in the main stream. The correlations between the emission performance and the total excess air ratio, the positions (4 positions) of the fuel injectors in the main stream, and the inlet temperature are obtained. Experi- mental results show that both the volume concentrations of unburnt hydrocarbon (UHC) and NOx (NO, NO2 usually grouped together as NOx) increase with the increase of total excess air ratio from 1.5 to 3.0; the emission performance relies heavily on the position of the main stream injector, and the best performance is achieved at Position 4 in the experiments; the increase of the inlet temperature impacts on the emission performance positively; the smallest volume concentrations of UHC and NOx obtained in the experiment are 94×10 6 and 2.3×10 6 respectively. This paper validates the feasibility of low emissions for an LPP/TVC and provides a reference for further optimization of TVCs.     

高空环境下喷嘴参数对航空活塞发动机燃烧与性能的影响

以一台四缸四冲程压燃式航空煤油活塞发动机为研究机型,运用工程系统高级建模和仿真平台软件(AMESim)仿真软件建立了发动机的整机模型,并使用台架实验的采集数据对该仿真模型进行了验证。在高空环境中,仿真分析了飞行器起飞工况、最大巡航工况下发动机喷油器的不同喷孔数、孔径对发动机燃烧过程、性能和NOx排放特性的影响。计算结果表明:稳态工况下,随着喷孔数的增加,最高燃烧压力和温度增加,瞬时放热率增长速度快且峰值上升;同时,缸内预混燃烧得到强化,燃烧始点提前,滞燃期和燃烧持续期缩短,燃烧重心前移,循环热效率增高,但同时会提高NOx的生成量;在飞行器瞬态变海拔的起飞工况下,多喷孔数、小孔径的喷油嘴有利于航空活塞发动机在高空环境下恢复发动机功率,提升飞行器的动力性和续航性能。      

Homologous flare–CME events and their metric type II radio burst association

Active region NOAA 11158 produced many flares during its disk passage. At least two of these flares can be considered as homologous: the C6.6 flare at 06:51 UT and C9.4 flare at 12:41 UT on February 14, 2011. Both flares occurred at the same location (eastern edge of the active region) and have a similar decay of the GOES soft X-ray light curve. The associated coronal mass ejections (CMEs) were slow (334 and 337 km/s) and of similar apparent widths (43° and 44°), but they had different radio signatures. The second event was associated with a metric type II burst while the first one was not. The COR1 coronagraphs on board the STEREO spacecraft clearly show that the second CME propagated into the preceding CME that occurred 50 min before. These observations suggest that CME–CME interaction might be a key process in exciting the type II radio emission by slow CMEs.     

高超声速流场对自由流扰动波响应及边界层扰动波演化

采用高阶精度有限差分方法直接数值模拟了来流慢声波作用下的钝锥高超声速绕流瞬态流场,分析了自由流扰动波与流场的相互干扰,并应用Fourier频谱分析了边界层扰动波时域和空域演化.结果显示:弓形激波出现连续的“∽”变形,初始扰动被显著放大,边界层内外扰动模态存在明显差别.从空域(沿流线)演化来看,在球头附近低频扰动为主导模态,出了球头区,总扰动模态中的低频和高频成分比例迅速转变,高频模态成分显著地增大.至流场下游,大部分低频分量衰减,或者不再增长,边界层内仅存在特殊频率的不稳定波快速增长.从时域演化来看,比起其他模态,主导模态的发展对上游激励的依赖更大.无论时域还是空域演化,都存在模态竞争现象.      

基于声发射的单层铝板高速撞击损伤类型识别

针对基于声发射技术的在轨航天器遭受空间碎片撞击损伤的评估问题,采用AUTODYN软件进行了弹丸超高速正撞击铝板所产生声发射波动信号的数值模拟,给出了二维模拟结果;对所得到的声发射信号进行小波重构,得到低频和高频部分的信号。通过研究低频和高频信号的峰值变化,发现第一和第二峰值幅度与撞击速度的变化具有一定的规律性,通过低频第二峰值幅度与第一峰值幅度比值将高速撞击损伤模式分为成坑、锥形穿孔和圆柱形穿孔三种类型。
     

Gyrosynchrotron Radiation of Interplanetary CMEs

CMEs (Coronal Mass Ejections) are an important means of energy release in the solar corona. Solar Polar Orbit Radio Telescope (SPORT) is a mission being proposed for observing the propagation of interplanetary CMEs from solar polar orbit. The main payload onboard SPORT is a synthetic aperture interferometric radiometer, which receives radio emission of interplanetary CMEs. It is identified that there are mainly three radio emission mechanisms of CMEs, i.e., bremsstrahlung, gyrosynchrotron emission and plasma emission. Among these emission types, bremsstrahlung emission is the main emission mechanism of the high-density plasma clouds of interplanetary CMEs. Gyrosynchrotron emission is the continuous emission generated by high-energy electrons from CMEs, while plasma emission is the main mechanism of transient radio bursts from CMEs. In this paper, the gyrosynchrotron emission of interplanetary CMEs is focused on. Firstly, the mechanism of gyrosynchrotron emission is reviewed. Secondly, a review of the physical parameter models of background solar wind and interplanetary CMEs is presented. After these, the brightness temperature and polarization of gyrosynchrotron emission of interplanetary CMEs are calculated and analyzed. Finally, the detectability of gyrosynchrotron emission of interplanetary CMEs by radio meters is discussed briefly.      

直升机气动噪声研究进展

对直升机气动噪声的研究进展进行了综述,内容包括试验技术、理论分析方法和噪声抑制技术。声学风洞试验是直升机气动噪声研究的基本手段,其中非定常载荷测试、流场显示和声源定位等先进测试技术已实现应用;飞行试验在直升机噪声适航标准完善和噪声控制技术研究等方面已成为必不可少的研究和验证手段。直升机气动噪声的理论体系不断完善,包括声类比法、Kirchhoff/CFD 混合法等旋翼气动噪声分析方法都已形成分析程序,成为直升机研发的有效工具。直升机气动噪声的抑制仍然以旋翼桨尖设计为主,飞行轨迹优化、旋翼噪声主动控制等新技术已实现飞行验证,但尚未进行型号应用。在用户和市场需求的推动下,在新型直升机的研发中,引入气动噪声的抑制技术将是必然的发展趋势。     

航天器声试验ISO国际标准制定过程及启示

标准国际化是助推中国航天国际化发展战略转型重要途径。针对航天器声试验技术成果,通过积极推动其向国际标准转化,最终使其立项并成为ISO 19924《空间系统——声试验》的国际标准。该标准是在航天器环境试验领域首个由中国发起、起草和主导的国际标准。文章将介绍声试验技术成果向国际标准转化的过程和方法,以分享经验,为我国积极参与国际标准化活动,提高标准国际化水平提供借鉴。