基于三因素模型的企业持续经营高风险预测研究

随着竞争的日趋激烈，企业持续经营不确定性显著增加，尽旱识别企业持续经营面临的风险，对于企业管理者、投资者来说都具有重要意义。现有的持续经营高风险研究依然没有摆脱“资料驱动型”的困境，文章根据三因素模型建立持续经营高风险预测模型。     

测微目镜-TV测读系统在测量金属线胀系数中的应用

鉴于光杠杆法测量金属线膨胀系数的缺点,依据金属线膨胀系数测量原理,采用测微目镜-TV测读系统测量金属线膨胀系数,并做了可行性分析,在此基础上,设计出了一整套完整的测量金属线膨胀系数的方法,进行了大量的实验,取得了较多的实验数据,并进行了数据分析,最后认为运用测微目镜-TV测读系统测量金属线胀系数,提高了被测物体微小位移的可视度,大大降低了系统误差.     

航空发动机虚拟自学习控制方法研究

随着人工智能技术的发展，智能航空发动机逐渐成为当今航空领域研究的热点。传统的航空发动机控制对发动机模型的依赖性过强，而基于发动机气热动力学公式的机理建模会引入较大的建模误差，给控制器设计带来困难。对此，提出一种基于强化学习的航空发动机控制虚拟自学习方法，首先利用航空发动机的试验数据通过LSTM 神经网络建立虚拟学习环境，然后采用深度强化学习TD3 算法，在虚拟环境中训练智能控制器，最后采用JT9D 发动机模型验证智能控制器的性能。结果表明：相比于传统PID 控制，智能控制器产生的超调量更小，调节时间更短。     

一种基于环路分类和启发式搜索的大围长QC-LDPC码构造新方法

文章通过对QC-LDPC码校验矩阵中的环路进行分类,提出一种检测所有长度小于12的环的无重无漏方法。利用该环路检测方法,提出了一种新的基于启发搜索的大围长QC-LDPC码构造法。该构造法分3步:首先,在无穷大CPM尺寸条件下根据启发策略搜索2条满足围长约束的整数序列;然后,依据设计码率从2条序列中截取若干整数对构成一个移位矩阵;最后,利用最近Zhang提出的理论下界从该移位矩阵中精确计算出使围长不减的CPM尺寸连续取值区间。与Liu-Han方法相比,新方法有2个优点:(1)既可以构造CPM尺寸连续变化的girth-10+QC-LDPC码,也可以构造CPM尺寸连续变化的girth-12 QC-LDPC码;(2)由于新环路检测方法有效提高了序列搜索速度,因此可以构造出设计码率非常高的girth-10+和girth-12 QC-LDPC码。     

Initial results from COMPTEL onboard GRO

COMPTEL is the first imaging telescope to explore the MeV gamma-ray range (0.7 to 30 MeV). At present, it is performing a complete sky survey. In later phases of the mission selected celestial objects will be studied in more detail. The data from the first year of the mission have demonstrated that COMPTEL performs very well. First sky maps of the inner part of the Galaxy clearly identify the plane as a bright MeV-source (probably due to discrete sources as well as diffuse radiation). The Crab and Vela pulsar lightcurves have been measured with unprecedented accuracy. The quasars 3C273 and 3C279 have been seen for the first time at MeV energies. Both quasars show a break in their energy spectra in the COMPTEL energy range. The 1.8 MeV line from radioactive ²⁶A1 has been detected from the central region of the Galaxy and a first sky map of the inner part of the Galaxy has been obtained in the light of this line. Upper limits to gamma-ray line emission at 847 keV and 1.238 MeV from SN 1991T have been derived. Upper limits to the interstellar gamma-ray emissivity have been determined at MeV-energies. Several cosmic gamma-ray bursts within the field-of-view have been located with an accuracy of about 1°. On 1991 June 9, 11 and 15, COMPTEL observed gamma-ray emission (continuum and line) from three solar flares. Also neutrons were detected from the June 9 and June 15 flares.     

Pulsar studies with GRO-COMPTEL

Pulsar measurements performed by the experiment COMPTEL, aboard the Compton Gamma Ray Observatory, are described. The main results refer to the Crab and Vela pulsars whose pulse shape characteristics are given in some detail and light curves are compared with those above 50 MeV, as observed by the COS-B satellite. No other gamma-ray pulsars have been detected to date by COMPTEL, the upper limit on the pulsed signal from Geminga being compatible with indications by other experiments.     

The gravity-darkening of the main-sequence components of spectral types A, F and G in detached close binary systems

From analysis of the photometric ellipticity effect in seven well-understood detached close binary systems, empirical values of the exponent of gravity-darkening have been practically deduced for eleven main-sequence components of spectral types A, F and G which should cover the range of structural change (from radiative to convective) in stellar atmospheres. The result indicate that values of the exponent diminish gradually with decreasing effective temperatures from 1.0 for radiative atmospheres with T > 8500 K to = 0.2 0.3 for convective atmospheres with T < 6500 K, in spite of some uncertainty in the reflection correction process.     

一种非接触光外差轮廓仪

介绍了一种纳米级非接触超高精度光外差轮廓仪。该量仪是基于普通光路的外差干涉仪,两束具有微小频差的激光束照射到制件表面:其中一束光被会聚后作为测量光针扫瞄制件表面;另一束光则被用作参考光束。这两束光经反射后形成干涉,所得信号的光程差与制件表面高度变化成正比。量仪的横向分辩力小于2μm,垂直分辩力小于1nm。制件不需要进行大的调整。制件表面同时亦被作为测量参考面。经光电转换后,信号由微机处理,从而快速完成测量、计算、显示与打印各种参数与图形。     

固体火箭发动机／导弹一体化设计

以某一两级固体地—空导弹作为算例,研究了固体火箭发动机/导弹一体化设计问题。研究以导弹起飞质量最轻和可用过载最大为目标建立了目标函数,利用优化理论完成了7个设计变量的优化设计。优化结果表明,所建立的数学模型是正确的。     

Wave measurements in active experiments on plasma beam injection

The paper presents the results and discussion of VLF wave measurements carried out in the course of two rocket experiments on injection of a dense cesium ion beam into the ionosphere at the heights of 165–240 km. The injection was accompanied by enhancement of the broad-band noise by several orders of magnitude. The wave measurements in the frequency range of 1–11 kHz revealed two pronounced frequencies somewhat exceeding that of the lower-hybrid resonance oscillations in the background plasma and the cesium beam. The oscillations were modulated by frequencies close to the ion-cyclotron frequencies of the background plasma.