新型固态纳米团簇NaXe在核磁共振中的量子尺寸效应

介绍了从体材料、薄膜(面材料)至量子点材料的发展。讨论了纳米材料中量子尺寸效应的重要意义。在实验中,用Xe离子注入NaCl微晶的方法,获得了尺寸小于80 nm的新型固态纳米团簇NaXe,测得了这种新型纳米材料在核磁共振中化学位移的量子尺寸效应。     

街道峡谷湍流流动的风洞试验与数值计算

在１：２５０的风洞模型上,测量街道峡谷的平均流速,湍流度等参数,分析了街道峡谷内的湍流流动状态,探讨了屋顶来流风在街道峡谷内产生复杂流场的主要特征,并用三维湍流流模型对风洞试验模型进行了数值计算,试验和计算结果为研究街道峡谷风环境以及街道峡谷的传热传质过程提供了基础。     

低膨胀高温合金的发展及在航空航天业的应用

回顾了低膨胀高温合金的发展历史."因瓦效应"和"时效硬化"现象的发现奠定了低膨胀高温合金发展的基础.20世纪70年代航空航天事业的迅猛发展以及能源危机的爆发为低膨胀高温合金在航空航天业的实际应用提供了宝贵的契机, 最早的商用Fe-Ni-Co(IN9××)系列合金,经过用Nb、Ti强化,去Al,加Si等一系列成分上的变化,显著改善其应力加速晶界氧化脆性(SAGBO性能),从此低膨胀高温合金在航空航天领域得到大量应用.为改善此类合金的抗氧化和降低裂纹扩展速率等性能,又进行了新合金系的研究,即以Inconel 783合金为代表的Fe-Ni-Co-Al-Cr系合金和以Haynes 242合金为代表的Ni-Mo-Cr系合金的研究,这些合金在750℃仍能达到完全抗氧化,为新一代飞机发动机的发展提供了优质材料.     

上证指数"百点效应"实证研究——基于前景理论的分析

通过研究上证指数落在百点附近区间的频率和日K线图的表现，揭示了其分布规律和运行特征。实证结果表明，从市场总体看，百点区间内样本较大时上证指数落在百点附近区间的频率接近均匀分布时的概率，上涨行情时，越过大多数百点位比较困难，而下跌行情时比较容易，百点位在某段行情的稳定性与上证指数在该百点附近区间的横盘整理时间有关。     

多卜勒湍流检测

对湍流目标进行检测,是多卜勒效应在现代机载气象雷达中的应用。鉴于目前在新型机载气象雷达中普遍装备了湍流信号处理电路,本文就有关的湍流目标及其检测原理和方法作简要介绍。     

转轴位置对俯仰动态特性的影响

研究了转轴位置对机翼、机身和三个组合体上翼面的动态特性的影响，对于机翼和机身，当转轴位置后移时其动态迟滞效应更为强烈。当翼面处于转轴之前，上仰时会出现更为的动态迟滞效应。因此鸭翼达到失速状态较晚。而当翼面处于转轴之后时，如尾翼，将会更早地出现动失速，转轴位置对动态迟滞特性的影响可以认为主要是由于俯仰运动时的动态洗流影响所导致的实际有效迎角的变化。由此影响了动态分离涡及其发展。     

高压不稳定环境中的燃料液滴蒸发

对燃料液滴在高压不稳定环境中的蒸发进行了研究，着重讨论了气相介质压力振荡对液滴蒸发特性的影响，计算了Ｃ１２Ｈ２６液滴在Ｎ２介质中蒸发时的蒸发速率、滴温和无因次滴径随时间的变化。结果表明：（１）蒸发速率、滴温发生相同频率的振荡，相位滞后分别为π和π／２；（２）压力振荡使蒸发速率平均值增大，液滴生存时间减少；（３）在不定常加热阶段压力振荡影响很小。     

Principal components in the PG-X-ray QSO sample

We have performed a spectral principal component analysis for a complete sample of 22 low redshift QSOs with spectra from Ly to H, and found three significant principal components, which account for 78% of the spectrum-to-spectrum variance. We present strong arguments that the first principal component represents the Baldwin effect, relating equivalent widths to the luminosity (i.e. accretion rate). The second component represents continuum variations, probably dominated by intrinsic reddening. The third principal component is directly related to broad emission-line width and X-ray spectral index, and therefore probably driven by Eddington accretion ratio, L/L_Edd. The third set of relationships tie directly to the optical Principal Component 1 found by Boroson and Green [Boroson, T., Green, R.F., Astrophys. J. Suppl. 80, 109, 1992 (BG92)], and are the primary cause of scatter in the Baldwin relationships.     

Spectra and time variability of black-hole binaries in the low/hard state

We propose a jet model for the low/hard state of galactic black-hole X-ray sources which explains the energy spectra from radio to X-rays and a number of timing properties in the X-ray domain such as the time lag spectra, the hardening of the power density spectra and the narrowing of the autocorrelation function with increasing photon energy. The model assumes that (i) there is a magnetic field along the axis of the jet, (ii) the electron density in the jet drops inversely proportional to distance, (iii) the jet is “hotter” near its center than at its periphery, and (iv) the electrons in the jet follow a power-law distribution function. We have performed Monte Carlo simulations of Compton upscattering of soft photons from the accretion disk and have found power-law high-energy spectra with photon-number index in the range 1.5–2 and cutoff at a few hundred keV, power-law time lags versus Fourier frequency with index 0.8, and an increase of the rms amplitude of variability and a narrowing of the autocorrelation function with increasing photon energy as they have been observed in Cygnus X-1. The spectrum at long wavelengths (radio, infrared, optical) is modeled to come from synchrotron radiation of the energetic electrons in the jet. We find flat to inverted radio spectra that extend from the radio up to about the optical band. For magnetic field strengths of the order 10⁵–10⁶ G at the base of the jet, the calculated spectra agree well in slope and flux with the observations.     

New multifrequency measurements of the spectrum of the cosmic background radiation

New measurements of the Cosmic Background Radiation temperature at 12 cm, 6.3 cm, 3 cm, 0.9 cm and 0.3 cm have made in July 1982 from the White Mountain High Altitude Research Station. The results are presented and the existence of spectral distortions discussed.