紧凑型空间外差成像光谱仪设计

设计了一种适合微小卫星平台应用的紧凑型空间外差成像光谱仪,该系统利用两套干涉结构将干涉条纹定域于系统外部,并将前置透镜的成像面与系统干涉面重合以获取目标的空间位置信息和光谱信息.根据系统轴上光表达式和奈奎斯特采样定律,给出了系统光谱分辨率和光谱范围与元件参数的匹配关系.通过光线追迹的方式,理论证明了干涉图定域位置,并推导了普适仪器函数表达式.针对氧原子气辉(O[1 D]630nm)星载测量,完成了该紧凑型空间外差成像光谱仪的系统设计和仿真,系统光谱采样间隔为0.762 3cm-1,光谱范围为601.674 9~631.324 6nm.最后通过搭建实验装置获取632.8nm激光光源的目标图像和复原光谱.仿真和实验结果表明:系统光谱采样间隔达到设计要求,且光谱分辨能力为20 822(@630nm);λ/4波长和线偏振器的装调误差(±1°)对系统干涉图调制度影响很小.该系统具有成像能力和光谱探测能力,可作为一种时空联合型干涉光谱仪使用.     

Reconstruction of baryon number distributions

The maximum entropy method(MEM) and Gaussian process(GP) regression,which are both wellsuited for the treatment of inverse problems,are used to reconstruct net-baryon number distributions based on a finite number of cumulants of the distribution.B ary on number distributions across the chiral phase transition are reconstructed.It is deduced that with the increase of the order of cumulants,distribution in the long tails,i.e.,far away from the central number,would become increasingly important.We ...