Observational evidence for non-equilibrium ionization in the solar corona

We investigate whether temperature sensitive EUV line ratios can be used as observational signatures for the presence of non-equilibrium ionization in transition region plasma. We compute the total intensity of some EUV lines of carbon and oxygen expected from coronal loop models with a steady-state flow and which are known to have significant departures from ionization equilibrium, selecting lines whose intensity ratios are useful for deducing the electron temperature in the coronal plasma. We calculate the intensity ratios with and without the approximation of ionization equilibrium, in order to determine the effects of any deviations from equilibrium on the numerical values of the line ratios examined.     

Manifestation of magnetic reconnection in coronal streamer current sheets

We investigate the possibility of observing the effects of magnetic reconnection inside a current sheet forming in a coronal streamer in the extended corona. In particular we study the possibility to observe with the UVCS of SOHO the excitation of the tearing instability in the current sheet.     

The Burst Alert Telescope (BAT) on the SWIFT Midex Mission

he burst alert telescope (BAT) is one of three instruments on the Swift MIDEX spacecraft to study gamma-ray bursts (GRBs). The BAT first detects the GRB and localizes the burst direction to an accuracy of 1–4 arcmin within 20 s after the start of the event. The GRB trigger initiates an autonomous spacecraft slew to point the two narrow field-of-view (FOV) instruments at the burst location within 20–70 s so to make follow-up X-ray and optical observations. The BAT is a wide-FOV, coded-aperture instrument with a CdZnTe detector plane. The detector plane is composed of 32,768 pieces of CdZnTe (4×4×2 mm), and the coded-aperture mask is composed of ∼52,000 pieces of lead (5×5×1 mm) with a 1-m separation between mask and detector plane. The BAT operates over the 15–150 keV energy range with ∼7 keV resolution, a sensitivity of ∼10⁻⁸ erg s⁻¹ cm⁻², and a 1.4 sr (half-coded) FOV. We expect to detect > 100 GRBs/year for a 2-year mission. The BAT also performs an all-sky hard X-ray survey with a sensitivity of ∼2 m Crab (systematic limit) and it serves as a hard X-ray transient monitor.     

高效气动优化设计方法

基于CFD方法开展气动外形优化设计通常计算量较大,采用离散共轭方法计算目标函数梯度,建立了高效的飞机气动优化设计系统。采用NURBS方法对翼剖面几何外形的扰动量进行参数化,避免了对原始外形的拟合,建立了基于NURBS方法的机翼剖面参数化方法。在复杂外形的优化设计中,动网格方法是关键技术之一,采用无限插值方法生成变形后的网格,并提出采用无限插值方法处理部件之间相贯线发生变化的情况。最后开展了翼身组合体+吊舱+挂架等复杂外形的优化设计,成功地减小了阻力,证明了方法的有效性。     

一种新型宽频带单脉冲天馈系统

提出了一种新近研制成功的结构紧凑的S~C波段新型的宽频带单脉冲天馈系统.其关键部件包括天线单元、宽频带魔T及宽频带功分器.通过对渐变槽线天线单元的分析和计算、天线阵列的分布及阵因子的计算、微带-槽线双重接头及其构成的魔T的研究,而获得了高增益的宽频带单脉冲天馈系统.天馈系统的实测结果与理论设计相吻合.      

Reverberation time lags in the high luminosity quasar PG 1247+267

Virial estimates of the black hole mass in the center of AGNs, derived from single-epoch observations of luminosity and emission line widths, are now available for several thousands of objects at all redshifts and luminosities, so that studies of the cosmological evolution of the AGN mass function are becoming possible. These estimates are based on the empirical luminosity-size relation measured through reverberation mapping at low redshifts and luminosities. For this reason the spectrophotometric monitoring of 4 luminous quasars was started in 2003, with the 1.8 m telescope of the Asiago Observatory. To measure the reverberation time lag we adopt a method, recently introduced by Zu et al. (2011), which takes advantage of the available statistical information on variability autocorrelation and makes simple assumptions on the continuum-emission line transfer function. We present the estimate of the broad line region size for the quasar PG 1247+267, which is the most luminous object with reverberation measures to date. Virial products computed for C iv and C iii] emission lines provide consistent results. A possible flattening of the size-luminosity relation for C iv at high luminosity is suggested.     

一种复杂形体消隐的新方法

本文首先提出了一种视线交点法消隐原理。然后针对复杂形体投影特点,给出了一种消除复杂形体隐藏线的新方法。该方法的特点是将复杂形体分解成若干个若干凸体,并将凸体的外围线框找出,同时将待消隐线段与外围线框求交,并用交点将待消隐线段分解成若干段,每一段采用视线交点法消隐原理测试其可见性,从而达到对待消隐线段消隐的目的。     

航空工业推行清洁生产优先生产线及清洁技术

本文在分析航空工业现状、特点,主要污染源及主要污染物的基础上,对现有清洁技术进行了选择性研究,提出了推行清洁生产的优先生产线及清洁技术。     

飞机中机身壁板预定位柔性工装技术研究

经过对数字化柔性装配工装技术内涵及柔性工装定位方式深入研究,结合某型飞机中机身壁板装配需求,设计了一套壁板组件预定位柔性工装,开发了基于现场总线的多轴控制系统,通过仿真完善了工装设计。工装能与现有自动钻铆机相配合,形成数字化柔性预定位、钻铆生产线,为提高中机身装配质量及效率,缩短生产准备周期,构建飞机数字化柔性装配生产线提供了一个良好范例。     

Fast spectroscopy of the 4 November 1978 gamma-ray burst

The Franco-Soviet Signe experiments on Venera 11 and Venera 12 allow a spectral analysis of gamma-ray bursts with a time resolution of 250 ms. Evidence is presented for i) short annihilation flashes of up to 20 photons cm⁻²s⁻¹ and ii) rapid variations of the continuum, from a study of the intense 4 November 1978 event.