密集根之特征向量导数的改进高精度动柔度法

作者曾为许多特征向量导数计算，提出过一种介于直接法（指直接求解线代方程组的，以Nelson为代表的一类方法）和模态法之间的高精度动柔度法。这种方法与作者建立的一般动柔度法一样，不能用于密集根之特征向量导数的计算。为使该方法扩展到密集根状态，本文将作者发展的混合移频技术应用于原高精度动柔度法，并重新推导了混合移频系统 的高精度动柔度式，从而形成能适用于许多密集根之特征向量导数计算的改进高精度动柔度法。     

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.     

Two magnetars: SGR 1627–41 and 1E 1547–5408

We describe the results obtained with Target of Opportunity observations of the galactic sources SGR 1627–41 and 1E 1547–5408. These two transients show several similarities supporting the interpretation of Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters as a single class of strongly magnetized neutron stars.     

Investigation of phase transition-based tethered systems for small body sample capture

This paper summarizes the modeling, simulation, and testing work related to the development of technology to investigate the potential that shape memory actuation has to provide mechanically simple and affordable solutions for delivering assets to a surface and for sample capture and possible return to Earth. We investigate the structural dynamics and controllability aspects of an adaptive beam carrying an end-effector which, by changing material equilibrium phases, is able to actively decouple the end-effector dynamics from the spacecraft dynamics during the surface contact phase. Asset delivery and sample capture and return are at the heart of several emerging potential missions to small bodies, such as asteroids and comets, and to the surface of large bodies, such as Titan.     

一种主动悬架式火星车稳定裕度优化控制策略

针对火星车在非结构化环境下行驶存在的稳定性不足而导致倾覆的风险,提出针对一种六轮主动悬架式火星车的稳定裕度优化控制方法。首先,考虑了火星车悬架机构调整过程中车轮与接触地面滑移和侧倾等运动关系,建立和完善了六轮主动悬架式火星车行驶的运动学模型。然后,以火星车夹角调整机构角度为变量,推导火星车在非结构环境下的稳定裕度模型。之后,使用内点法求解火星车稳定裕度的最优解,并获得期望的夹角调整机构关节角度。在此基础上,对夹角调整机构的关节角度进行规划和控制,实现火星车悬架机构构型的调整,从而提高火星车在非结构化环境下行驶的稳定裕度。最后,对火星车稳定裕度优化控制策略的有效性进行仿真验证,结果表明,所提出的控制方法可有效提高火星车在非结构化环境下行驶的稳定裕度。     

The radiation environment in the ISS-USLab measured by ALTEA: Spectra and relative nuclear abundances in the polar,equatorial and SAA regions

We present here the energy spectra relative to different geomagnetic regions as measured by the ALTEA (Anomalous Long Term Effects on Astronauts) detector in the International Space Station – USLab from August 2006 to July 2007.     

四维超混沌射频隐身跳频通信设计方法

为提高飞行器通信系统的抗截获性能,提出了一种基于四维超混沌系统的射频隐身跳频通信设计方法。该方法构建了四维超混沌系统,扩展了系统解空间,有效增加了系统复杂度,并通过引入周期性扰动措施,解决了有限精度带来的短周期现象。在四维超混沌系统的基础上,利用超混沌系统生成的双通道超混沌序列,实现了跳频通信系统的频率序列和周期序列联合不确定设计方法。仿真结果表明：四维超混沌系统与传统混沌系统相比,其复杂度最优,在相同有限精度条件下,超混沌系统的周期性明显减弱。另外,基于四维超混沌设计的跳频系统,其截获概率优于常规跳频系统,具有较好的射频隐身性能。     

Stochastic modelling considering ionospheric scintillation effects on GNSS relative and point positioning

Global Navigation Satellite Systems (GNSS), in particular the Global Positioning System (GPS), have been widely used for high accuracy geodetic positioning. The Least Squares functional models related to the GNSS observables have been more extensively studied than the corresponding stochastic models, given that the development of the latter is significantly more complex. As a result, a simplified stochastic model is often used in GNSS positioning, which assumes that all the GNSS observables are statistically independent and of the same quality, i.e. a similar variance is assigned indiscriminately to all of the measurements. However, the definition of the stochastic model may be approached from a more detailed perspective, considering specific effects affecting each observable individually, as for example the effects of ionospheric scintillation. These effects relate to phase and amplitude fluctuations in the satellites signals that occur due to diffraction on electron density irregularities in the ionosphere and are particularly relevant at equatorial and high latitude regions, especially during periods of high solar activity. As a consequence, degraded measurement quality and poorer positioning accuracy may result.