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%。     

月基极紫外相机多层膜反射镜

月基极紫外相机用于月球表面对地球等离子体层辐射出的30.4 nm谱线进行成像观测,多层膜反射镜是月基极紫外相机的重要光学元件。根据月基极紫外相机技术参数,选择了B₄C/Mg,B₄C/Mg₂Si,B₄C/Al,B₄C/Si,Mo/Si等材料,对其周期厚度、材料比例、周期数等参数进行优化。计算了以上材料组合在30.4 nm的反射率曲线。考虑到月球环境的特殊性和材料的物理化学性质,从中选择出Mo/Si和B₄C/Si两种组合,利用磁控溅射进行镀制。Mo/Si和B₄C/Si多层膜在30.4 nm反射率分别达到15.3%和22.8%。     

低原子序数材料窄带多层膜的研制

为研制极紫外波段窄带多层膜反射镜,采用低原子序数材料组合设计了30.4 nm波长处Mg/SiC,Si/SiC,Si/B4C和Si/C多层膜反射镜,并与极紫外波段传统的Mo/Si多层膜反射镜进行对比。采用直流磁控溅射技术制备了这些多层膜,在国家同步辐射实验室辐射与计量光束线完成了多层膜反射率测量,测量结果表明:Mg/SiC多层膜的带宽最小,为1.44 nm,且反射率最高,为44%;而Mo/Si多层膜的反射率仅为24%,带宽为3.11 nm。实验结果证明了采用低原子序数材料组成的多层膜的带宽要比常规多层膜窄,该方法可以应用于极紫外波段高分辨研究。     

高反射率Mo/B4C多层膜设计及制备

 运用遗传算法优化设计了Mo/B₄C多层膜结构。入射光入射角度取10°时,设计的理想多层膜膜对数为150,周期为3.59 nm,Gamma值（Mo膜厚与周期的比值）为0.41,峰值反射率为33.29%。采用恒功率模式直流磁控溅射方法制作Mo/B₄C多层膜。通过在Mo/B4C多层膜与基底之间增加15 nm厚的Cr粘附层,提高多层膜与基底的粘附力。另外,还采用调整多层膜Gamma值的方法减小其内应力,调整后多层膜结构周期为3.59 nm, Mo膜厚1.97 nm, B4C膜厚1.62 nm,峰值反射率26.34％。制备了膜对数为150的Mo/B₄C膜并测量了其反射率,在波长7.03 nm处,Mo/B₄C多层膜的近正入射反射率为21.0％。最后对测量结果进行了拟合,拟合得到Mo/B₄C多层膜的周期为3.60 nm,Gamma值0.60,界面粗糙度为0.30 nm。     

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）。     

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.     

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。     

Mo/Si多层膜表面保护层设计

为提高Mo/Si多层膜的稳定性与使用寿命,通过分析多层膜驻波电场的分布,对表面保护层及多层膜最上层材料的厚度进行优化设计,使优化后的反射率最高.计算表明,一定厚度的表面保护层总对应一个最优的最上层材料厚度.在13.36 nm波长,膜对数为50的Mo/Si多层膜10度入射的理论反射率为74.47%;当添加厚度为2.3 nm的Ru作为表面保护层,对应多层膜最上层Si的优化厚度为3.93 nm,其理论反射率为75.20％.设计结果表明,通过优化设计表面保护层,可以提高多层膜稳定性,改善多层膜性能.     

正入射Mo/B_4C软X射线多层膜

采用Ｍｏ／Ｂ４Ｃ材料在短波长波段（λ＜１０．０ｎｍ）进行软Ｘ射线多层膜实验研究。在指定波长（８．０ｎｍ附近）处对多层膜进行结构设计，并制备出了周期结构准确的Ｍｏ／Ｂ４Ｃ多层膜样品。     

Design of chirped Mo/Si multilayer mirror in the extreme ultraviolet region

The chirped Mo/Si multilayer mirror in the extreme ultraviolet region is designed to obtain sub-femtosecond pulses from high-order harmonics. Numerical simulations of temporal profile of the pulses are made for superposition of incident high-order harmonics and that of reflected ones by the chirped multilayer mirror.The normal incidence reflectivity and chirp in the wavelength range of 12.5 - 16.5 nm are 6.7% ±0.5%and-3617±171 as2, respectively. Simulation results indicate that the designed chirped multilayer mirror can be used for producing 104-as pulses.     

EUV damage threshold measurements of Mo/Si multilayer mirrors

We present 1-on-1 and 10-on-1 damage threshold investigations on Mo/Si multilayers with EUV radiation of 13.5 nm wavelength, using a table-top laser produced plasma source based on solid gold as target material. The experiments were performed on different types of Mo/Si mirror, showing no significant difference in single pulse damage thresholds. However, the damage threshold for ten pulses is ??60?% lower than the single pulse threshold, implying a defect dominated damage process. Using Nomarski (DIC) and atomic force microscopy (AFM) we analysed the damage morphologies, indicating a primarily thermally induced damage mechanism. Additionally, we studied the radiation-induced change of reflectivity upon damage of a multilayer mirror.     

质子辐照下Mo/Si多层膜反射镜的微观结构状态

利用透射电子显微镜对质子辐照前后空间太阳望远镜Mo/Si多层膜的微观结构进行了表征, 并对其辐照前后反射率的变化进行了测量.研究表明, Mo/Si多层膜经质子辐照后形成了一些缺陷结构,局部区域Mo/Si的周期性遭到破坏, Mo层与Si层的宽度发生了变化,多层膜层与层之间的界面也比辐照前更为粗糙,部分层状结构由于质子辐照发生了明显的扭曲和折断等现象;此外,质子辐照导致了Mo/Si多层膜反射率的下降,这些微观缺陷的形成是光学性能降低的直接诱因. 关键词： 空间太阳望远镜 Mo/Si多层膜 微观结构 反射率     

单发实验测量软X射线多层膜反射镜反射特性

 提出了一种单发实验测量软X射线波段多层膜反射镜反射特性的简易方法。实验采用激光等离子体软X射线源作为光源,用平焦场光栅谱仪分光,在光路中引入掠入射镜以消除高级次谱的影响,用软X光CCD记录,在一发激光打靶实验中,测量了设计中心波长为13.9 nm的Mo/Si多层膜反射镜的反射特性。     

中心波长为13．9nm的正入射Mo／Si多层膜

用由铜靶激光等离子体光源等组成的反射率计对自行设计的周期厚度为7.14nm的120层Mo/Si多层膜进行极紫外(EUV)波段反射率测量。由于多层膜层数增加所引起的吸收、膜层界面之间的扩散以及镀膜过程中的膜厚控制误差或表面被氧化(污染)等原因,正入射Mo/Si多层膜在13.9nm处的反射率低于理论计算值73.2%,最后用原子力显微镜(AFM)测量其表面粗糙度为σ=0.401nm。     

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。     

低温退火的X射线W/Si多层膜应力和结构性能

W/Si多层膜反射镜在硬X射线天文望远镜中有重要应用. 为减小其应力对反射镜面形和望远镜分辨率的影响, 同时保证较高的反射率, 采用150, 175和200 ℃ 的低温退火工艺对采用磁控溅射镀制的W/Si周期多层膜进行后处理. 利用掠入射X射线反射测试和样品表面面形测试对退火前后W/Si多层膜的应力和结构进行表征. 结果表明, 在150 ℃ 退火3 h 后, 多层膜1级峰反射率和膜层结构几乎没有发生变化, 应力减少约27%; 在175 ℃ 退火3 h后, 多层膜膜层结构开始发生变化, 应力减少约50%; 在200 ℃退火3 h 后, 多层膜应力减小超过60%, 但1级布拉格峰反射率相对下降17%, 且膜层结构发生了较大变化. W, Si界面层的增大和相互扩散加剧是应力和反射率下降的主要原因.     

Comprehension of the effects of proton on reflectivity of Mo/Si multilayer

Wavelength dependent reflectivity is crucial relationship in determining the physical property of optic system. The first object of this work is to search for the applicable method of using wavelength to predict the reflectivity of Mo/Si multilayer mirror before and after irradiation with proton. Predicated on the principle of non-linear curve fitting, a typical numerical method is highlighted because the wavelength-dependent reflectivity of Mo/Si multilayer irradiated by proton with different energies and flux are quantitative analyzed by this method. The simulations agree very well with the observed spectroscopy of 6 curves for reflectivity versus wavelength. The minimum value of correlation coefficients between actual and calculated data is 0.994. The other objects of this work are to find the optic band gap of Mo/Si multilayer and check the influences of proton on it using reflectivity spectra. In the light of the calculated results by Tauc method, the optic band gap is theoretically explained successfully via the relationship between band gap and absorption coefficient. The estimated results by both theoretical and experimental data demonstrate that the optic band gap of Mo/Si multilayer is not sensitive to proton radiation.     

Thermal cycles, interface chemistry and optical performance of Mg/SiC multilayers

The interplay between optical performance and the thermally activated interface chemistry of periodic Mg/SiC multilayers designed for application at 30.4 nm are investigated by optical (hard X-ray, soft X-ray and ultraviolet ranges, i.e. from 0.154 to 30.4 nm) reflectivity and X-ray emission spectroscopy. The multilayers are prepared by magnetron sputtering and then annealed up to a temperature of 500 °C. Two clear changes take place in the multilayer upon annealing. At first, between 200 and 300 °C a strong decrease of the reflectivity is observed, due to the development of interfacial roughness following the crystallization of the Mg layers. No interfacial compound is detected. Then, between 350 and 400 °C there is formation of the Mg₂Si magnesium silicide at the interfaces following the reaction between the Mg and SiC layers. This also leads to the almost total loss of reflectivity of the multilayer. Thus, this kind of multilayer is thermally stable only for application requiring no heating above 200 °C.     

23.4nm软X射线多层膜反射镜研制

为了满足类氖-锗X射线激光研究的需要,设计制备了23.4 nm软X射线多层膜反射镜.依据多层膜选材原则并考虑材料的物理化学特性选择新的材料Ti与Si组成材料对.设计优化材料多层膜的周期厚度(d),材料比例(Γ),周期数(N),计算出Ti/Si反射率曲线.通过实验优化各种镀膜工艺参数,制备出了23.4 nm的Ti/Si多...     

Influence of Beryllium Barrier Layers on the Properties of Mo/Si Multilayer Mirrors

Technical Physics - The performance of multilayer Mo/Si mirrors with B4C and Be spacers near a wavelength of 13.5 nm has been studied. It has been shown that four-component Mo/Be/Si/B4C...