Exploring The Saturn System In The Thermal Infrared: The Composite Infrared Spectrometer

The Composite Infrared Spectrometer (CIRS) is a remote-sensing Fourier Transform Spectrometer (FTS) on the Cassini orbiter that measures thermal radiation over two decades in wavenumber, from 10 to 1400 cm^{− 1} (1 mm to 7μ m), with a spectral resolution that can be set from 0.5 to 15.5 cm^{− 1}. The far infrared portion of the spectrum (10–600 cm^{− 1}) is measured with a polarizing interferometer having thermopile detectors with a common 4-mrad field of view (FOV). The middle infrared portion is measured with a traditional Michelson interferometer having two focal planes (600–1100 cm^{− 1}, 1100–1400 cm^{− 1}). Each focal plane is composed of a 1× 10 array of HgCdTe detectors, each detector having a 0.3-mrad FOV. CIRS observations will provide three-dimensional maps of temperature, gas composition, and aerosols/condensates of the atmospheres of Titan and Saturn with good vertical and horizontal resolution, from deep in their tropospheres to high in their mesospheres. CIRS’s ability to observe atmospheres in the limb-viewing mode (in addition to nadir) offers the opportunity to provide accurate and highly resolved vertical profiles of these atmospheric variables. The ability to observe with high-spectral resolution should facilitate the identification of new constituents. CIRS will also map the thermal and compositional properties of the surfaces of Saturn’s icy satellites. It will similarly map Saturn’s rings, characterizing their dynamical and spatial structure and constraining theories of their formation and evolution. The combination of broad spectral range, programmable spectral resolution, the small detector fields of view, and an orbiting spacecraft platform will allow CIRS to observe the Saturnian system in the thermal infrared at a level of detail not previously achieved.This revised version was published online in July 2005 with a corrected cover date.     

电离辐射对部分耗尽SOI器件关态电流的影响

针对辐射前后环栅与条栅结构部分耗尽绝缘体上硅(SOI,Silicon On Insulator)器件关态电流的变化展开实验,研究结果表明辐射诱使关态电流增加主要取决于侧壁泄漏电流、背栅寄生晶体管导通、带-带隧穿与背栅泄漏电流的耦合效应.在条栅结构器件中,辐射诱生场氧化层固定电荷将使得器件侧壁泄漏电流增加,器件前、背栅关态电流随总剂量变化明显;在环栅结构器件中,辐射诱使背栅晶体管开启将使得前栅器件关态电流变大,而带-带隧穿与背栅泄漏电流的耦合效应将使得器件关态电流随前栅电压减小而迅速增加.基于以上结果,可通过改良版图结构以提高SOI器件的抗总剂量电离辐射能力.     

基于多模型简化CDKF的故障诊断方法

针对使用传统卡尔曼滤波器对非线性系统进行故障诊断,估计精度低的问题,提出了一种新的故障诊断方法.该方法结合多模型自适应估计和简化中央差分卡尔曼滤波器的优点,能在线快速地检测出故障,利用中央差分代替了雅可比矩阵的求解,使系统状态估计准确收敛到真实值附近,而且避免了反复求解量测预测方差等一系列繁杂过程.在执行机构不同故障的情况下,通过与其他算法进行诊断对比,结果表明提出的算法在精度上和运行速度上具有明显的优势.     

导弹滑模抗干扰自动驾驶仪设计

针对拦截弹的抗干扰控制问题，设计了一种基于扩张状态观测器和快速滑模控制的三通道自动驾驶仪。首先建立考虑有界未知不确定性和外界干扰的拦截弹系统模型，构建扩张状态观测器对有界未知不确定性和外界干扰进行估计；在此基础上，根据自动驾驶仪系统特性，设计了一种快速滑模控制算法使得系统在受到有界未知不确定性和外界干扰的情况下仍然能精准快速跟踪指令信号，并基于李雅普诺夫函数证明了其稳定性。仿真结果验证了所设计控制算法的有效性。