单/双涵道模式转换动态过程的数值研究

为研究变循环发动机单/双涵道模式转换动态过程中流场参数的变化规律,基于本项目组设计的模拟模式转换过程的试验台,利用动网格技术对该试验台进行了二维数值模拟。结果表明:在模式转换动态过程中,内外涵流量和总压的变化滞后于阀门缓慢关闭的状态;并且阀门变化速率越快,其内涵总压和流量的动态响应越滞后;而静压的变化规律则相反。此外,还研究了在阀门关闭过程中,不同初始涵道比对这种流场参数变化滞后性的影响。发现初始涵道比越小,滞后性越强;并且这种滞后性在阀门关闭至22°位置时达到最大。     

稀薄大气下机械展开式再入飞行器气动特性研究

以机械展开式再入飞行器为研究对象,采用DSMC(直接蒙特卡洛模拟)方法计算分析了其在稀薄大气环境下的气动特性.讨论了飞行器在不同高度下的流场特性和升阻及配平特性,结果表明飞行器流场及受力特性对大气稀薄程度显示出较强的敏感性;进一步分析了连续流过渡至稀薄大气下飞行器的阻力系数,得出了随着来流Knudsen数增加,大气稀薄效应逐渐显现,传统的CFD方法已不再适用于描述流动特征的结论,同时给出了依据来流Knudsen数大小采取CFD和DSMC方法分别进行计算分析的建议.     

航空发动机过失速及退喘模型研究

针对涡喷和涡扇发动机,通过求解带源项的2维欧拉方程组,发展了模拟发动机整机过失速及退喘动态过程的理论模型,实现了2种发动机稳定状态-喘振/旋转失速-退喘动态过程的模拟。分析了某单轴涡喷发动机算例,模拟结果展现出喘振和旋转失速相应的基本特征;对某小涵道比双轴混排涡扇发动机进、退喘模拟结果进行分析,发现风扇与压气机均发生了喘振,且喘振频率相等,并最终都恢复至稳定状态。     

压气机稳定边界的数值预测研究

为研究不同压气机稳定性预测方法的准确性,采用最大静压升系数法与商用CFD软件,对某4级低速压气机的稳定边界进行了数值模拟,并与试验结果对比。计算结果表明:最大静压升系数法在预测压气机稳定边界上有一定的准确性。使用商用CFD软件NUMECA对某4级压气机进行模拟计算,考虑了不同的网格划分方案、使用不同的湍流模型和差分格式等因素,以出现数值发散作为压气机失稳的标准,结果表明:主流区的网格对计算结果影响较大。不同差分格式的结果显示,中心差分格式的结果最好。     

利用机载GNSS-R的有效波高反演技术

采用自主研发的多源多宿GNSS-R(Global Navigation Satellite System-Reflections,全球导航卫星系统反射信号)海洋环境遥感探测系统,在天津渤海湾特定区域进行了3次机载校飞试验,获得了大量有效GNSS-R信号数据,对自然条件下的海面有效波高进行了反演处理。该系统通过对接收的GNSS直达信号和海面反射信号进行相关运算处理,可以获得DDM(Delay-Doppler Mapping,时延—多普勒映射)图谱,再利用DCF(Derivative of the Correlation Function,相关函数的导数)在DDM图谱基础上进行相关功率波形的计算,进而通过计算DCF的函数波形宽度得到海面有效波高,验证了该方法的可行性。该方法具有全天时、全天候、高分辨率、低成本等优点,对全球范围内中小尺度海洋状态和物理现象的监测具有重要意义。     

1 000 MW超超临界锅炉结渣特性预测模型

根据1 000 MW超超临界锅炉的实际运行数据,对其结渣特性进行研究和分析。建立了基于煤灰特性的锅炉结渣特性预测模型,包括单一指标和综合指标的各预测模型,这些预测模型能简单、快速地预测锅炉的结渣特性。但对于锅炉燃用煤质不均匀或采用混煤燃烧等情况,这类预测模型的准确性和可靠性将下降。同时根据锅炉运行时的实时监测数据,建立了基于炉膛清洁因子的炉膛结渣特性在线监测模型,通过炉膛出口后各受热面进出口蒸汽温度、流量,以及省煤器出口烟气温度等有关参数,利用反平衡法计算求得此时的炉膛出口烟气温度,然后求出炉膛的平均热有效性系数和炉膛清洁因子,最后根据清洁因子的大小来判断锅炉的结渣特性。该模型不仅能根据锅炉运行实时数据的采集,实现锅炉结渣特性的在线实时监测,而且能对煤质不均匀或采用混煤燃烧等情况的锅炉结渣特性做出较准确的判别。     

Observation of Terrestrial gamma-ray flashes in the RELEC space experiment on the <Emphasis Type="Italic">Vernov</Emphasis> satellite

The RELEС scientific payload of the Vernov satellite launched on July 8, 2014 includes the DRGE spectrometer of gamma-rays and electrons. This instrument comprises a set of scintillator phoswich-detectors, including four identical X-ray and gamma-ray detector with an energy range of 10 kev to 3 MeV with a total area of ~500 cm² directed to the atmosphere, as well as an electron spectrometer containing three mutually orthogonal detector units with a geometric factor of ~2 cm² sr. The aim of a space experiment with the DRGE instrument is the study of fast phenomena, in particular Terrestrial gamma-ray flashes (TGF) and magnetospheric electron precipitation. In this regard, the instrument provides the transmission of both monitoring data with a time resolution of 1 s, and data in the event-by-event mode, with a recording of the time of detection of each gamma quantum or electron to an accuracy of ~15 μs. This makes it possible to not only conduct a detailed analysis of the variability in the gamma-ray range, but also compare the time profiles with the results of measurements with other RELEC instruments (the detector of optical and ultraviolet flares, radio-frequency and low-frequency analyzers of electromagnetic field parameters), as well as with the data of ground-based facility for thunderstorm activity. This paper presents the first catalog of Terrestrial gamma-ray flashes. The criterion for selecting flashes required in order to detect no less than 5 hard quanta in 1 ms by at least two independent detectors. The TGFs included in the catalog have a typical duration of ~400 μs, during which 10–40 gamma-ray quanta were detected. The time profiles, spectral parameters, and geographic position, as well as a result of a comparison with the output data of other Vernov instruments, are presented for each of candidates. The candidate for Terrestrial gamma-ray flashes detected in the near-polar region over Antarctica is discussed.     

Designing corrections for the trajectory of the <Emphasis Type="Italic">Spektr-R</Emphasis> spacecraft in the event of immersions into the Moon’s sphere of influence

The results of updating the parameters of motion of the Spektr-R spacecraft at the end of 2016 have shown that, in January 2018, with a probability close to unity, the condition that a spacecraft stay in the Earth’s shadow is violated; however, in May of the same year, the ballistic life of the spacecraft will be terminated. Thus, in 2017, the question arose of how to design the correction of flight of this spacecraft using its onboard propulsion system. The correction was designed with allowance for the fact that, for the first time since it was launched, the spacecraft in the course of several years, beginning with 2017, repeatedly approaches the Moon, deeply immersing into its sphere of influence. This paper presents the technologically and organizationally convenient, allowable versions of upcoming correction of the Spektr-R spacecraft trajectory and justifies the particular scheme of its implementation.     

Estimating the accuracy of the technique of reconstructing the rotational motion of a satellite based on the measurements of its angular velocity and the magnetic field of the Earth

The paper has studied the accuracy of the technique that allows the rotational motion of the Earth artificial satellites (AES) to be reconstructed based on the data of onboard measurements of angular velocity vectors and the strength of the Earth magnetic field (EMF). The technique is based on kinematic equations of the rotational motion of a rigid body. Both types of measurement data collected over some time interval have been processed jointly. The angular velocity measurements have been approximated using convenient formulas, which are substituted into the kinematic differential equations for the quaternion that specifies the transition from the body-fixed coordinate system of a satellite to the inertial coordinate system. Thus obtained equations represent a kinematic model of the rotational motion of a satellite. The solution of these equations, which approximate real motion, has been found by the least-square method from the condition of best fitting between the data of measurements of the EMF strength vector and its calculated values. The accuracy of the technique has been estimated by processing the data obtained from the board of the service module of the International Space Station (ISS). The reconstruction of station motion using the aforementioned technique has been compared with the telemetry data on the actual motion of the station. The technique has allowed us to reconstruct the station motion in the orbital orientation mode with a maximum error less than 0.6° and the turns with a maximal error of less than 1.2°.