高纬极区电离层中离子声波谱线增强的解释

大量的实验研究表明, 在顶部极光区电离层, 利用EISCAT非相干散射雷达和Millstone Hill雷达可以观测到不对称、增强的离子声波谱线. 考虑到低能H+离子束沉降到背景电离层, 以及电离层顶部O+离子的外流事件, 采用含有场向热流项的双麦克斯韦分布描述H+离子束的分布函数, 进而基于离子－离子双流不稳定性理论来解释增强的离子声波谱线. 场向热流的引入可以减小离子声波谱线的不对称现象, 这样得到的结果更符合实际.     

利用光谱拟合法反演中间层顶大气温度

本文提出了利用梳状函数进行模拟光谱计算的方法, 并根据在北京郊区观测的OHMeinel(9, 4)带夜气辉光谱, 利用加权最小二乘法与模拟光谱进行拟合, 得出了转动温度的最佳值, 同时还分析了OH(9, 4)气辉强度和转动温度随时间的变化特性.     

硼酸盐玻璃中稀土离子的发光研究

应用荧光光谱、红外振动光谱等研究了在可见光区发光的Ｐｒ（３＋）,Ｓｍ（３＋）,Ｅｕ（３＋）,Ｔｂ（３＋）,Ｄｙ（３＋）,Ｅｒ（３＋）和Ｔｍ（３＋）等镧系稀土离子在硼酸盐玻璃中的发光行为,系统地分析了稀土离子在硼酸盐玻璃基质中的激发谱和发光谱特性。     

火星进入器高超声速气动力/热研究综述

以火星大气条件下飞行器非平衡流场研究为背景,采用态-态模型对定容静止CO₂系统自30 km火星大气条件（181 K）瞬时升温后的热非平衡过程开展数值模拟。考虑CO₂分子的对称拉伸、弯曲和非对称拉伸三个振动模态共201个振动能级,微观过程包括：振动-平动（VT）能量交换过程引起的同一模态内部的和不同模态间的振动能级跃迁,振动-振动（VV）能量交换过程引起的同一模态内部振动能级跃迁。分析不同振动模态的能级分布演化特点,并考察对应微观过程细节探究内在原因,结果表明：VT过程起支配作用,对由初始低温突然升温后保持定温的气体非平衡过程,VV过程的贡献可以忽略;CO₂分子的弯曲振动模态具有最快的激发速率,平衡时也具有最高的粒子数占比,升温至相似文献   

Magnetar spectra and twisted magnetospheres

The huge potential drop between the footpoints of the closed field lines in the twisted magnetospheres of magnetars may accelerate electrons up to very high energies, γ ? 10⁶. On the other hand, the comparison between the observed spectra of magnetars and spectra obtained by accurate theoretical models seems to favor of a picture in which the magnetosphere is filled by “slow” electrons (v ? 0.8c), rather than by ultra-relativistic particles.     

Changes in hyperspectral reflectance signatures of lettuce leaves in response to macronutrient deficiencies

The adaptation of specific remote sensing and hyperspectral analysis techniques for the determination of incipient nutrient stress in plants could allow early detection and precision supplementation for remediation, important considerations for minimizing mass of advanced life support systems on space station and long term missions. This experiment was conducted to determine if hyperspectral reflectance could be used to detect nutrient stress in Lactuca sativa L. cv. Black Seeded Simpson. Lettuce seedlings were grown for 90 days in a greenhouse or growth chamber in vermiculite containing modified Hoagland’s nutrient solution with key macronutrient elements removed in order to induce a range of nutrient stresses, including nitrogen, phosphorus, potassium, calcium, and magnesium. Leaf tissue nutrient concentrations were compared with corresponding spectral reflectances taken at the end of 90 days. Spectral reflectances varied with growing location, position on the leaf, and nutrient deficiency treatment. Spectral responses of lettuce leaves under macronutrient deficiency conditions showed an increase in reflectance in the red, near red, and infrared wavelength ranges. The data obtained suggest that spectral reflectance shows the potential as a diagnostic tool in predicting nutrient deficiencies in general. Overlapping of spectral signatures makes the use of wavelengths of narrow bandwidths or individual bands for the discrimination of specific nutrient stresses difficult without further data processing.     

Soft X-Ray and Extreme Ultraviolet Excess Emission from Clusters of Galaxies

An excess over the extrapolation to the extreme ultraviolet and soft X-ray ranges of the thermal emission from the hot intracluster medium has been detected in a number of clusters of galaxies. We briefly present each of the satellites (EUVE, ROSAT PSPC and BeppoSAX, and presently XMM-Newton, Chandra and Suzaku) and their corresponding instrumental issues, which are responsible for the fact that this soft excess remains controversial in a number of cases. We then review the evidence for this soft X-ray excess and discuss the possible mechanisms (thermal and non-thermal) which could be responsible for this emission.     

小鹰-500飞机疲劳试验载荷谱的编制方法

针对小鹰500飞机的设计和使用特点，选用了FAA推荐的通用飞机实测载荷谱数据，按照民机的TWIST编谱原则编制出用重心过载表示的“飞-续-飞”随机疲劳试验载荷谱，用于小鹰-500飞机机翼疲劳试验，并参照国外文献中有关尾翼载荷谱的保守处理方法，采用了从重心载荷谱计算出配套平衡的平尾机动载荷，将其幅值放大1.2倍和频次放大3倍的做法，编制出了平尾疲劳试验载荷谱。     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.