在19.5 nm处高反在30.4 nm处抑制的双功能薄膜

 研究了极紫外波段的双功能光学元件。采用周期膜叠加的思想,运用遗传方法优化设计了在19.5 nm处高反,在30.4 nm处抑制的双功能多层膜。采用磁控溅射技术制备了多层膜,利用X射线衍射仪测试了多层膜的结构,在国家同步辐射实验室测试了双功能多层膜的反射特性。结果表明：制备出的双功能膜性能与设计相符,在入射角13°,19.5 nm处的反射率达到33.3%,接近传统的19.5 nm周期高反膜的反射率,并且在30.4 nm附近将反射率由1.1%降到9.6×10^-4。     

13 nm窄带Si/Mo/C多层膜反射镜

基于多层膜准单色覆盖50~1500 eV能谱的多能点发射光谱测量系统可获得聚龙一号装置Z-pinch等离子体X射线源的能谱结构和总能量等信息。考虑装置的条件,在13 nm处的多层膜需要工作在掠入射角60。常规的Mo/Si多层膜尽管反射率最高,但其带宽较大,不能满足多层膜准单色的要求。因此提出将Mo和C共同作为多层膜的吸收层材料与Si组成Si/Mo/C多层膜,可使反射率降低较小而带宽明显减小。采用磁控溅射方法制备了Si/Mo/C多层膜,其掠入射X射线反射测量表面多层膜的结构清晰完整,同步辐射工作条件下反射率测量,得到Si/Mo/C多层膜在13 nm处和掠入射角60时的反射率为56.5%,带宽为0.49 nm（3.7 eV）。     

基于遗传算法的30.4 nm多层膜设计

阐述了用遗传算法设计周期和非周期多层膜的原理和实现过程,完成了30.4 nm Mg/SiC周期和非周期多层膜设计,研究了遗传算法中不同种群数和多层膜膜厚取值范围对优化结果的影响.计算发现,种群数的恰当选取是使算法快速达到或逼近最优解的前提,膜厚取值范围的合理选择是提高算法效率的关键.设计得到入射角10°的周期多层膜和15°~22°范围内的宽角多层膜在波长30.4 nm处的反射率依次为56.57%与39.96±0.29%,5°入射的双功能多层膜在波长30.4 nm和58.4 nm处的反射率分别为54.1%和0.1%.结果表明遗传算法也是一种很好的多层膜设计方法.     

nm量级薄膜厚度测量

 为了获得nm量级薄膜样品的精确厚度,采用软X射线反射率拟合方法、Bragg衍射方程方法和反射率Fourier变换方法分析了常规Cu靶X射线衍射数据及软X射线反射率数据。对厚度测量结果进行比较,3种方法得到的结果一致性很好。其中,软X射线反射率拟合和Bragg衍射方程方法精度很高,优于1 nm,Fourier变换方法精度稍低。对于单层W薄膜样品,3种方法获得厚度分别为(15.21±0.60) nm,(14.0±1.0) nm和(13.8±1.5) nm;对于双层W/C薄膜样品,W层厚度分别为(12.64±0.60) nm,(13.0±1.0) nm和(13.9±1.5) nm。这3种方法测量结果精度主要取决于反射率数据测量精度,而Fourier变换方法精度随着能量升高而提高,随着掠入射角范围增大而提高。     

50~110 nm波段高反射率多层膜的设计与制备

阐述了50~110 nm强吸收波段亚四分之一波长多层膜的设计方法.这种膜系是由强吸收材料叠加而成，每层膜光学厚度小于四分之一个波长.与常规周期多层膜相比，这种膜系更适用于提高强吸收波段的反射率.利用该方法设计了50 nm处高反射多层膜，并以此为初始条件通过Levenberg-Marquart优化方法完成了50~110 nm强吸收波段宽带高反射率Si/W/Co多层膜的设计，其平均反射率达到45%.采用直流磁控溅射方法制备了Si/W/Co多层膜,用X射线衍射仪(XRD)对膜层结构进行了测试，测试结果表明制作出的多层膜结构与设计结构基本相符.     

X射线Kirkpatrick-Baez显微镜用超反射镜的研制

 介绍了一种可应用于X射线Kirkpatrick-Baez（KB）显微镜的光学元件—X射线超反射镜。选用的W和B₄C作为镀膜材料，膜对数为20，采用单纯型调优的方法实现了X射线超反射镜设计，用磁控溅射的方法在Si基片上完成了W/B₄C X射线超反射镜的制备。采用高分辨率X射线衍射仪（8 keV）测量了X射线超反射镜的反射特性。制备的X射线超反射镜在掠入射角分别为1.052°和1.143°处，反射角度带宽为0.3°，反射率达到20%，可满足KB型显微镜的要求。     

一种软X射线多层膜界面粗糙度的计算方法

提出一个利用多层膜小角X射线衍射谱衍射峰积分强度计算多层膜界面粗糙度的公式。用磁控溅射技术制备Mo／Si多层膜，用波长为0．154nm的硬X射线测量样品在小掠入射角区的衍射曲线，分别用本文公式和反射率曲线拟合方法计算了样品的界面粗糙度。实验结果表明：由本文公式获得的界面粗糙度近似于拟合方法获得的界面粗糙度，它们略等于多层膜界面实际粗糙度。     

50～11O nm波段高反射率多层膜的设计与制备

阐述了50～110 nm强吸收波段亚四分之一波长多层膜的设计方法.这种膜系是由强吸收材料叠加而成,每层膜光学厚度小于四分之一个波长.与常规周期多层膜相比,这种膜系更适用于提高强吸收波段的反射率.利用该方法设计了50 nm处高反射多层膜,并以此为初始条件通过Levenberg-Marquart优化方法完成了50～110 nm强吸收波段宽带高反射率Si/W/Co多层膜的设计,其平均反射率达到45%.采用直流磁控溅射方法制备了Si/W/Co多层膜,用X射线衍射仪(XRD)对膜层结构进行了测试,测试结果表明制作出的多层膜结构与设计结构基本相符.     

磁控溅射法制备极紫外6.8~11.0 nm波段Mo/B4C横向梯度多层膜

用直流磁控溅射法结合掩模板控制膜厚的方法在Si衬底上制备了工作于6.8~11.0 nm波段的[Mo/B₄C]₆₀横向梯度多层膜。利用X射线掠入射反射测试以及同步辐射反射率测试对梯度多层膜的结构及性能进行了测试。X射线掠入射反射测试结果表明,多层膜周期厚度沿着长轴方向从4.39 nm逐渐增加到7.82 nm,周期厚度平均梯度为0.054 nm/mm。对横向梯度多层膜沿长轴方向每隔5 mm进行了一次同步辐射反射率测试,结果显示,横向梯度多层膜在45°入射角下的反射率约为10%,反射峰的半高全宽介于0.13 nm到0.31 nm之间。     

磁控溅射方法制备直径120mm高均匀性Mo/Si多层膜

为满足极紫外、软X射线和X射线大口径多层膜反射镜的需求,采用基板扫掠过矩形靶材表面的镀膜方法,在直径120 mm的平面基板上镀制了Mo/Si周期多层膜。通过调整基板扫掠过矩形靶材表面的速率修正了薄膜的沉积速率,极大地提高了薄膜厚度的均匀性。采用X射线衍射仪对反射镜不同位置多层膜周期厚度进行了测量,结果表明,在直径120 mm范围内,Mo/Si多层膜周期厚度的均匀性达到了0.26%。同步辐射测量多层膜样品不同位置处的反射率,结果表明,在直径120 mm范围内,多层膜的膜层厚度均匀,在入射角10°时13.75 nm波长处平均反射率为66.82%。     

软X射线多层膜反射镜反射率测量

 采用线状激光等离子体作为软X光源,用具有空间分辨的掠入射光栅谱仪对正入射多层膜反射镜进行了反射率测量。谱仪测谱范围20~40nm,谱分辨0.05nm,测得50层C/Al反射镜在中心波长28.6nm处反射率为22%,带宽约为2.5nm。     

基于模拟退火算法的宽角度X射线超反射镜设计研究

应用于硬X射线波段的宽带多层膜光学元件———宽角度X射线超反射镜的设计可以归结为一个连续变量的多维多极值的全局优化问题。缺少一种有效的全局优化方法是阻碍解决这一难题的一个关键。模拟退火算法是一种简单而且通用的全局优化算法。结合光学多层膜的设计原理提出了利用模拟退火算法来进行宽角度X射线超反射镜设计的新方法。结合已有的方法选择了W和C作为膜层的膜对材料,设计出Cu的Kα线处角度范围0.9°~1.1°反射率达到20%的宽角度X射线超反射镜。并在此基础上采用改进的自适应模拟退火算法实现了Cu的Kα线处宽角度X射线超反射镜的理想设计结果。设计结果表明了模拟退火算法在多层膜最优化设计领域的正确性和有效性。     

30.4 nm波长SiC/Mg多层膜反射镜

波长30.4 nm的He-II谱线是极紫外天文观测中最重要的谱线之一,空间极紫外太阳观测光学系统需要采用多层膜作为反射元件。为此研究了SiC/Mg、B4C/Mg、C/Mg、C/Al、Mo/Si、B4C/Si、SiC/Si、C/Si、Sc/Si等材料组合的多层膜在该波长处的反射性能。基于反射率最大与多层膜带宽最小的设计优化原则,选取了SiC/Mg作为膜系材料。采用直流磁控溅射技术制备了SiC/Mg多层膜,用X射线衍射仪测量了多层膜的周期厚度,用国家同步辐射计量站的反射率计测量了多层膜的反射率,在入射角12°时,实测30.4 nm处的反射率为38.0%。     

Performance of a polarizer using synthetic mica crystal in the 12-25 nm wavelength range

To develop polarizer functioning in the extreme ultraviolet (EUV) and soft X-ray region, the polar- ization performance of synthetic mica has been investigated theoretically with a simulation code using Fresnel equations and optical constants from the Henke database. The reflectance of synthetic mica crystal for s and p polarization was measured to investigate its polarization performance in a home-made synchrotron radiation soft X-ray polarimeter at beamline 3W1B, Beijing Synchrotron Radiation Facility (BSRF). The reflectivity of the synthetic mica crystal at an angle of grazing incidence of 48° was obtained from the experimental data, which is about 4.8x10<'-3> at 25 nm and 6.0×10<'-4> at 12 nm, and the linear polarizance of the X-ray reflected by the synthetic mica crystal that we measured using an analyzer-rotating method increases from 80% to 96.6% in this EUV region, while higher than 98.2% in the simulation. The result indicates that this synthetic mica crystal works as a practical polarizer in this EUV region of 12-25 nm, and also in an extensive wavelength region higher than 25 nm.     

ESR膜及在POLAR探测器中的应用

基于巨双折射光学的增强型镜面反射膜(ESR)具有高分子多层膜结构。在10~80°反射角范围内,利用623.8nm,532nm,441.6nm和413.1nm激光对ESR的反射率进行了测量,结果显示,在整个范围内有较均匀的反射率,平均反射率大于95%,平均透过率小于0.5%。XRD分析显示ESR在大尺度范围内有良好的晶化结构。在γ射线极化仪POLAR应用中,ESR作为BC448塑料闪烁体探测器反射层比用黑漆反射层的光子收集效率提高了近10倍。     

Co/C and W/Si multilayers deposited by ion-beam sputtering for the soft X-ray range

We deposited Co/C multilayer mirrors for a wavelength of 4.77 nm and W/Si multilayer mirrors for a wavelength of 1.77 nm by use of ion-beam sputtering. The small-angle diffraction spectrum was used to analyze the structure of the multilayers. With a combination of the experimental diffraction spectra and Apeles’ theory for calculation of the interfacial roughnesses of the multilayers, the interfacial roughnesses of Co/C and W/Si are 0.80 nm and 0.60 nm, respectively, which are lower than that of the substrate. The reflectivity of the Co/C multilayer is measured to be about 20% and that of the W/Si multilayer about 1% at the grazing incidence angle of about 12°. Received: 30 May 2000 / Accepted: 1 August 2000 / Published online: 11 February 2002     

Mo/Si aperiodic multilayer broadband reflective mirror for 12.5-28.5-nm wavelength range

Aperiodic molybdenum/silicon (Mo/Si) multilayer designed as a broadband reflective mirror with mean reflectivity of 10% over a wide wavelength range of 12.5-28.5 nm at incidence angle of 5° is developed using a numerical optimized method. The multilayer is prepared using direct current magnetron sputtering technology. The reflectivity is measured using synchrotron radiation. The measured mean reflectivity is 7.0% in the design wavelength range of 12.5-28.5 nm. This multilayer broadband reflective mirror can be used in extreme ultraviolet measurements and will greatly simplify the experimental arrangements.     

Ion beam sputter deposited W/Si multilayers: Influence of re-sputtering on the interface structure and structure modification at ultra short periods

X-ray multilayer mirrors of period ranging from 9.6 to 1.7 nm, deposited using ion beam sputtering, have been examined using grazing incidence X-ray reflectivity (GIXRR) and grazing incidence X-ray diffraction. Detailed analysis of GIXRR data revealed that significant amount of re-sputtering of Si layer takes place while W deposition is underway. Re-sputtering is mainly due to bombardment of high-energy neutrals getting reflected from the W target. Due to re-sputtering interface of the multilayer becomes asymmetric. This puts a major hindrance in avoiding the intermixing and achieving sharp interfaces at shorter periods. Maximum thickness of Si which gets lost due to re-sputtering during deposition is ∼0.8 nm. The shortest period multilayer estimated, that could be deposited without intermixing, was 2.7 nm. These results are of significance for developing low period W/Si multilayers.     

Space solar telescope in soft X-ray and EUV band

In this paper we have reviewed our achievements in soft X-ray and extreme ultraviolet (EUV) optics. Up to now, the research system of soft X-ray and EUV optics has been established, including light sources, detectors, calibrations, optical testing and machining of super smooth mirrors, and fabrications of multilayer film mirrors. Based on our achievements, we have developed two types of solar space telescopes for the soft X-ray and EUV space solar observations. One is an EUV multilayer normal incident telescope array including 4 different operation wavelength telescopes. The operation wavelengths of the EUV telescope are 13.0, 17.1, 19.5 and 30.4 nm. The other is a complex space solar telescope, which is composed of an EUV multilayer normal incident telescope and a soft X-ray grazing incident telescope. The EUV multilayer normal incident telescope stands in the central part of the soft X-ray grazing incident telescope. The normal incident telescope and the grazing incident telescope have a common detector. The different operation wavelengths can be changed by rotating a filter wheel.