复杂目标红外辐射特性大数据知识表示及建模方法

为了提升复杂目标红外辐射特性建模效率及置信度问题，提出一种目标红外辐射特性的大数据知识表示及建模方法。首先利用机理分析法、主成分分析法确定目标红外辐射特性大数据维度;然后基于主成分分析的结果，进行目标红外辐射特性大数据知识表示，建立目标红外辐射特性仿真模型;最后进行模型的仿真应用，在应用过程中进一步完善目标红外辐射特性数据或知识表示。本文提供的大数据驱动的目标红外辐射特征建模方法，能够推广应用于复杂电磁环境的仿真。     

Solar wind-driven electron radiation belt response functions at 100-min time scales

We present a simple yet numerically robust technique, using autoregressive linear filters, to remove unwanted “colored noise” from solar wind and radiation belt electron data at sub-daily resolution. The remaining signal is then studied using finite impulse response linear prediction filters to represent the driven portion of the linear dynamics that describe the coupling between solar wind speed and electron flux. Sub-daily resolution response profiles covering magnetic L-shells between 1.1 and 8.0 R_E are presented which are consistent with daily resolution response functions. Namely, while there is strong global coherence governing electron flux dynamics, there are at least two distinct responses. The first response is an immediate dropout of electrons between L = 4 and L = 7 that is at least a partly adiabatic effect associated with enhancements in the ring current. This is followed by a 1–2 day delayed enhancement across the same L-shells that is likely a result of increased radial diffusion. The second response is an immediate enhancement seen between L = 3 and L = 4 with a typical duration of less than one day. Plausible explanations for this second response are briefly discussed, but neither empirical nor theoretical evidence can establish conclusively a definite physical cause. Finally, the response profiles show significant solar cycle and seasonal dependencies, indicating that better model output might be achieved with: (1) additional simultaneous solar wind inputs; (2) more sophisticated dynamical model structures capable of incorporating non-linear feedback; and/or (3) time-adaptive linear filters that can track non-stationary dynamics in time.     

轴对称矢量喷管的气膜冷却及红外辐射耦合计算分析

为考察喷管壁面气膜冷却以及红外辐射特性对高性能航空发动机壁温分布的影响,对燃气红外波带的光谱特性采用窄波段模型计算,对壁面-燃气辐射采用封闭腔模型计算,对喷管收敛段的气膜冷却采用绝热温比计算。对于包含喷管壁面、隔热屏、套筒的多层结构传热建立壁温-热流耦合的热平衡方程,用Newt on-Raphson求解得到喷管及内外结构的壁温。对NASA TN D-1988中试验台架发动机喷管扩张段的气膜冷却及壁温进行验证计算,并详细计算了收敛段采用多排缝槽气膜冷却的轴对称矢量喷管。结果表明:气膜冷却有效降低了喷管收敛段的壁温,使得喷管扩张段成为受热严峻的部位;扩张段偏转改变了扩张段壁面温度和红外辐射的圆周分布,沿偏转方向的壁温和红外辐射都明显低于偏转反方向的,2个方向上的平均壁温相差约4.8%,喷管在后半球的辐射沿偏转方向增强。数值模拟结果与试验测量值吻合良好,可用于发动机喷管壁温分布精确计算。     

飞机环控系统管道气流温度的测量

根据实际使用中出现的问题，对各种实用的管道气流温度传感器的误差进行了计算，对电阻式和热电偶式温度传感器的误差原因作了定量分析。由于带密封罩的温度传感器在实际使用中存在着明显的缺点，建议今后使用热电偶测量飞机环控系统管道气流温度，并提出了一种实用热电偶温度传感器的结构形式，同时也介绍了如何减小由于热传导和热辐射引起的误差。     

Improving DORIS geocenter time series using an empirical rescaling of solar radiation pressure models

Even if Satellite Laser Ranging (SLR) remains the fundamental technique for geocenter monitoring, DORIS can also determine this geophysical parameter. Gobinddass et al. (2009) found that part of the systematic errors at 118 days and 1 year can be significantly reduced by rescaling the current solar radiation pressure models using satellite-dependent empirical models. Here we extend this study to all DORIS satellites and propose a complete set of empirical solar radiation parameter coefficients. A specific problem related to SPOT-5 solar panel realignment is also detected and explained. New DORIS geocenter solutions now show a much better agreement in amplitude with independent SLR solutions and with recent geophysical models. Finally, the impact of this refined DORIS data strategy is discussed in terms of Z-geocenter monitoring as well as for other geodetic products (altitude of high latitude station such as Thule in Greenland) and Precise Orbit Determination. After reprocessing the full 1993.0-2008.0 DORIS data set, we confirm that the proposed strategy allows a significant reduction of systematic errors at periods of 118 days and 1 year (up to 20 mm), especially for the most recent data after 2002.5, when more DORIS satellites are available for geodetic purposes.     

Infrared radiation signature of exhaust plume from solid propellants with different energy characteristics

The infrared radiation signature of the plume from solid propellants with different energy characteristics is not the same. Three kinds of double-base propellants of different energy characteristics are chosen to measure the infrared spectral radiance from 1000 cm 1 to 4500 cm 1 of their plumes. The radiative spectrum is obtained in the tests. The experimental results indicate that the infrared radiation of the plume is determined by the energy characteristics of the propellant. The radiative transfer calculation models of the exhaust plume for the solid propellants are established. By including the chemical reaction source term and the radiation source term into the energy equation, the plume field and the radiative transfer are solved in a coupled way. The calculated results are consistent with the experimental data, so the reliability of the models is confirmed. The temperature distribution and the extent of the afterburning of the plume are distinct for the propellants of different energy characteristics, therefore the plume radiation varies for different propellants. The temperature of the fluid cell in the plume will increase or decrease to some extent by the influence of the radiation term.     

2010年后国外主要航天装备的辐射特性

介绍了2010年后的美国主要军事航天装备的主要发展状况，重点介绍了2010年后的美国军事航天装备工作过程中的空间辐射特性，以及主要采用的反空间信息对抗措施，为未来的空间系统的发展选择提供了参考。     

一种窄带辐射温度计智能标定及检定系统

文章描述了由串行电可改写擦除存储器（ＥＰＲＯＭ）、ＲＳ－２３２通讯口和个人计算机（ＰＣ）组成的窄带辐射温度计标定检定系统。系统除了能够在标定过程中自动完成仪器的标定，给出听输出误差分布、提高仪器的速度以外，在检定时还可以通过修改检定参数很容易地修正仪器的各种源移量，使被检测仪器无需作入动或调整即可重新使用。     

Plasma Waves in the Hermean Magnetosphere

The Hermean magnetosphere is likely to contain a number of wave phenomena. We briefly review what little is known so far about fields and waves around Mercury. We further discuss a number of possible phenomena, including ULF pulsations, acceleration-related radiation, bow shock waves, bremsstrahlung (or braking radiation), and synchrotron radiation. Finally, some predictions are made as to the likelihood that some of these types of wave emission exist.     

GTEM小室放置被测物后的场分布

使用球坐标系下的FDTD和球坐标系下Mur型二阶吸收边界条件计算了 GTEM小室中放置被测物后的场分布，分析了被测物对GTEM小室中电磁场的扰动情况