A study of acoustic halos in active region NOAA 11330 using multi-height SDO observations

We analyze data from the Helioseismic Magnetic Imager (HMI) and the Atmospheric Imaging Assembly (AIA) instruments on board the Solar Dynamics Observatory (SDO) to characterize the spatio-temporal acoustic power distribution in active regions as a function of the height in the solar atmosphere. For this, we use Doppler velocity and continuum intensity observed using the magnetically sensitive line at 6173?Å as well as intensity at 1600?Å and 1700?Å. We focus on the power enhancements seen around AR 11330 as a function of wave frequency, magnetic field strength, field inclination and observation height. We find that acoustic halos occur above the acoustic cutoff frequency and extends up to 10?mHz in HMI Doppler and AIA 1700?Å observations. Halos are also found to be strong functions of magnetic field and their inclination angle. We further calculate and examine the spatially averaged relative phases and cross-coherence spectra and find different wave characteristics at different heights.     

Solar atmosphere wave dynamics generated by solar global oscillating eigenmodes

The solar atmosphere exhibits a diverse range of wave phenomena, where one of the earliest discovered was the five-minute global acoustic oscillation, also referred to as the p-mode. The analysis of wave propagation in the solar atmosphere may be used as a diagnostic tool to estimate accurately the physical characteristics of the Sun’s atmospheric layers.In this paper, we investigate the dynamics and upward propagation of waves which are generated by the solar global eigenmodes. We report on a series of hydrodynamic simulations of a realistically stratified model of the solar atmosphere representing its lower region from the photosphere to low corona. With the objective of modelling atmospheric perturbations, propagating from the photosphere into the chromosphere, transition region and low corona, generated by the photospheric global oscillations the simulations use photospheric drivers mimicking the solar p-modes. The drivers are spatially structured harmonics across the computational box parallel to the solar surface. The drivers perturb the atmosphere at 0.5?Mm above the bottom boundary of the model and are placed coincident with the location of the temperature minimum. A combination of the VALIIIC and McWhirter solar atmospheres are used as the background equilibrium model.We report how synthetic photospheric oscillations may manifest in a magnetic field free model of the quiet Sun. To carry out the simulations, we employed the magnetohydrodynamics code, SMAUG (Sheffield MHD Accelerated Using GPUs).Our results show that the amount of energy propagating into the solar atmosphere is consistent with a model of solar global oscillations described by Taroyan and Erdélyi (2008) using the Klein-Gordon equation. The computed results indicate a power law which is compared to observations reported by Ireland et al. (2015) using data from the Solar Dynamics Observatory/Atmospheric Imaging Assembly.     

Successes and challenges in non-destructive testing of aircraft composite structures

Composite materials are increasingly used in the aerospace industry. To fully realise the weight saving potential along with superior mechanical properties that composites offer in safety critical applications, reliable Non-Destructive Testing (NDT) methods are required to prevent catastrophic failures. This paper will review the state of the art in the field and point to highlight the success and challenges that different NDT methods are faced to evaluate the integrity of critical aerospace composites. The focus will be on advanced certificated NDT methods for damage detection and characterization in composite laminates for use in the aircraft primary and secondary structures.     

声重波激发的ESF的波长效应

通过对赤道地区声重波激发的Ｓｐｒｅａｄ－Ｔ扰动的非线性制约方程的拓扑特性,在不同扰动波长和扰动振幅的条件一进行数值计算,以及对原始非线性方程组在不同参数范围内进行数值模拟,显示了声重波的垂直扰动分量对ＥＳＦ演化的影响,为赤道地区Ｓｐｒｅａｄ－Ｆ形态的多样性提供了一种非线性的解释。     

通讯用K波段20W空间行波管设计

文章介绍了K波段20W空间行波管的设计和测试情况.该行波管整管采用金属陶瓷封接结构、周期永磁聚焦、传导冷却、四级降压收集极、B J220标准波导输入输出,其主要参数为输出功率24W、增益≥45dB、总效率≥53％、相移＜40°.     

液氧煤油气液同轴直流离心式喷嘴的声学模拟实验研究

气液同轴直流离心式喷嘴对补燃发动机燃烧室高频燃烧稳定性有显著影响。为研究气液同轴直流离心式喷嘴的声学特性,在大气环境条件下进行了单喷嘴声学模拟实验。通过安装在模拟燃烧室外侧的扬声器激发声学振荡,利用声学探针测量燃烧室内的声压,获得了喷嘴长度、节流嘴直径对燃烧室声学特性的影响规律,确定了喷嘴长度与节流嘴直径的选取原则。     

碳/环氧复合材料层板基体裂纹的检测与分析

本工作从实验和计算两方面测算碳/环氧复合村料在拉伸载荷下,[0/90]s、[±45]_(s),]11=11]碳布三种层板基体裂纹发生的形式和应变水平,以期能预测不同裂纹产生的载荷门槛值。结果表明:采用声发射技术跟踪配合显微观测碳/环氧层板初始损伤(基体裂纹、脱层等)的应力水平,并采用能量判据有限无计算裂纹扩展的临界应变能释放率,计算和实验结果比较,符合较好。     

CFRP在钻削加工中的声发射特性

文摘根据CFRP钻削过程中缺陷的产生机理,用声发射传感器采集钻削过程中的声发射信号有效值电压(RMS)。分析了在不同钻削参数下的RMS,对孔的入口处撕裂与出口处撕裂对应的RMS进行识别。结果表明:在钻削过程中,入口处和出口处撕裂会引起RMS的突变,能够有效的进行识别;主轴转速一定时,RMS随着进给量的增大而增大;进给量一定时,RMS随着主轴转速的增大而增大。     

Design and optimization of supersonic turbines for detonation combustors

Detonation-based engines offer a potential surge in efficiency for compact thermal power systems. However, these cycles require ad-hoc components adapted to the high outlet velocity from the detonation combustors. This paper presents the design methodology of turbine stages suitable for supersonic inlet conditions and provides a detailed analysis of optimized turbine geometries. A reduced-order solver examines the supersonic blade rows’ functional design space, quantifies the turbine’s non-isent...     

Location of layered structures in the ionosphere and atmosphere by use of GPS occultation data

A method is introduced to locate the layered structures in the atmosphere and ionosphere based on simultaneous observations of radio wave intensity and phase variations in trans-ionospheric satellite-to-satellite links. The method determines location of a tangent point on the trans-ionospheric ray trajectory where gradient of refractivity is perpendicular to the ray trajectory and influence of a layered structure on radio wave parameters is maximal. An estimate of the location of a layer can be obtained from a combination of the phase and intensity variations. This new technique was applied to measurements provided during FORMOSAT-3 and CHAMP radio occultation (RO) missions. For the considered RO events the location of the inclined plasma layer in the lower ionosphere is found and the electron density distribution is retrieved. The method is checked by measuring the location of the tangent point on the ray trajectory in the neutral gas in the atmosphere. The results showed a fairly good agreement.