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.     

30.4 nm波长处Mg基多层膜反射镜

太阳光谱中重要的He-Ⅱ谱线(波长30.4 nm)的观测对于研究太阳活动和日地空间环境具有重要意义,实现空间极紫外太阳观测需要采用多层膜作为反射元件.研究了工作在30.4 nm的Mg基多层膜.以反射率最高为评价函数设计了多层膜,采用直流磁控溅射技术制备了SiC/Mg,B4C/Mg和C/Mg多层膜,用X射线衍射仪测量了多层膜的结构.研究表明虽然B4C/Mg多层膜理论反射率最高,但实际制备结果显示,SiC/Mg多层膜的成膜质量最好,反射率最高.同步辐射反射率测量表明:在入射角10°时实测的SiC/Mg多层膜反射率为44.6%.     

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%。     

19.5nm极紫外反射镜的研制

介绍了一种用于太阳观测19.5nm极紫外多层膜的研究工作。利用软件对规整的Mo/Si膜系结构进行了优化,拓宽了反射带宽,提高了积分反射率。采用双离子束溅射技术,时间控厚,成功制备了该反射镜。通过同步辐射反射率计测试表明,峰值反射率27.5%,均匀性在1%以内,已初步达到预设要求。     

4.48 nm正入射软X射线激光用Cr/C多层膜高反射镜的研制

针对4.48nm类镍钽软X射线激光及其应用实验,设计制备了工作于这一波长的近正入射多层膜高反射镜。选择Cr/C为制备4.48nm高反射多层膜的材料对,通过优化设计,确定了多层膜的周期、周期数以及两种材料的厚度比。模拟了多层膜非理想界面对高反射多层膜性能的影响。采用直流磁控溅射方法在超光滑硅基片上实现了200周期Cr/C多层膜高反射镜的制备。利用X射线衍射仪测量了多层膜结构,在德国BessyⅡ同步辐射上测量了在工作波长处多层膜反射率,测量的峰值反射率达7.5%。对衍射仪测量的掠入射反射曲线和同步辐射测量的反射率曲线分别进行拟合,得到的粗糙度和厚度比的结果相近。测试结果表明,所制备的Cr/C多层膜样品结构良好,在指定工作波长处有较高的反射峰,达到了设计要求。     

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.     

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.     

表面层对1 064 nm高反射镜损伤阈值影响

 采用电子束蒸发的方法制备了３种具有不同表面层材料及结构的中心波长为1 064 nm的零度高反镜,３种膜系表面层分别为1/4波长光学厚度的HfO₂,1/2波长光学厚度的SiO₂,以及1/4波长光学厚度的SiO₂。光谱测试表明：三者在1 064 nm处均有较高的反射率（高于99.8%）,利用热透镜的方法测量得到３个膜系辐照激光正入射情况下,薄膜对光的吸收比例分别为3.0×10^-6,5.0×10^-6和6.5×10^-6,其损伤阈值分别为32.5,45.2和28.4 J/cm²。并在膜层内部电场分布和膜层材料物理特性的基础上分析了３种不同表面层膜系吸收和损伤阈值差别的原因。     

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。     

可见光波段及1 064 nm波长处用于Glan-Taylor棱镜减反射膜

为了提高Glan-Taylor棱镜的透射率,研究了Glan-Taylor棱镜在可见光波段及1 064 nm波长处减反射膜膜的设计和制备.为提高薄膜和冰洲石晶体的附着力,采用沉积Al2O3为过渡层,ZrO2作缓冲层的方法,用单纯形优化的方法进行膜系优化设计.用电子束沉积和离子束辅助沉积的方法制备了多层减反射膜,并采用石英晶体振荡法监控膜厚和沉积速率.测量结果表明,在可见光波段及1 064 nm波长处的剩余反射率均小于0.5%经测试薄膜与冰洲石晶体的附着力性能良好.     

B4C/Mo/Si high reflectivity multilayer mirror at 30.4 nm

The B4C/Mo/Si high reflectivity multilayer mirror was designed for He-Ⅱ radiation (30.4 nm) using the layer-by-layer method. The theoretical peak reflectivity was up to 38.2% at the incident angle of 5°. The B4C/Mo/Si multilayer was fabricated by direct current magnetron sputtering and measured at the National Synchrotron Radiation Laboratory (NSRL) of China. The experimental reflectivity of the B4C/Mo/Si multilayer at 30.4 nm was about 32.5%. The promising performances of the B4C/Mo/Si multilayer mirror could be used for the construction of solar physics instrumentation.     

Design and performance of two-channel EUV multilayer mirrors with enhanced spectral selectivity

In this paper, we present a study on two-channel multilayer mirrors which can operate at two wavelengths in Extreme Ultraviolet (EUV) spectral range. We propose a new method to design two-channel EUV multilayer mirrors with enhanced spectral selectivity. The mirror structure is a stack of two periodic multilayers separated by a buffer layer. We have defined the main parameters which allow adjustment of the distance between different order Bragg’s peak and of wavelength positions of reflectivity minima. Two mirrors have been designed and deposited for solar EUV telescope applications by using this method. The first mirror reflects Fe IX–X line (17.1 nm) and Fe XVI (33.5 nm) lines with attenuation of the He II line (30.4 nm). The second mirror reflects Fe IX–X and He II lines with attenuation of Fe XV (28.4 nm) and Fe XVI lines. Measurements with synchrotron radiation source confirm that, in both cases, for these mirrors, we are able to adjust reflectivity maxima (Bragg peak position) and minima. Such multilayers offer new possibilities for compact design of multi-wavelength EUV telescopes and/or for high spectral selectivity.     

Effect of defects on the reflectivity of Cr/C multilayer soft X-ray mirror at 4.48 nm

Cr/C is a promising material combination for multilayer mirror in the “near water window region” (4.4-6.7 nm). In the present paper, the effect of defects on the reflectivity of Cr/C soft X-ray multilayer mirror deposited by magnetron sputtering was studied. Formation of thin interlayer due to the interdiffusion, rough interface due to the non-sharp layer and contamination of O happened during the deposition process were found by a method combined by XPS, soft X-ray reflectivity at 4.48 nm and grazing incidence hard X-ray reflectivity at 0.154 nm. The XPS results show that both interlayers (Cr-on-C and C-on-Cr) are mixture composed of C sp2, C sp3, CO, CO, CrCr and CrO bondings. No chromium carbide was found at the interlayer probably due to the blocking of oxides’ formation. Through the analysis of X-ray reflectivity, we obtained the multilayer structure parameters (thickness and roughness) and optical constants of each layer at 4.48 nm. Based on those results, a further calculation was carried out. The result shows that the formation of the thin interlayer contributes little to the decrease of the reflectivity, the rough interface decreases the reflectivity most and the contaminant (O) not only decreases the reflectivity but also shifts the position of the peak.     

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。     

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）。     

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...     

500 nm带宽啁啾镜对的设计与应用

设计了中心波长在825 nm、有效带宽在600 nm～1100 nm的超宽带啁啾镜对,色散补偿量目标值为-100 fs2。配对设计的啁啾镜对有效抑制了单个啁啾镜的色散振荡,啁啾镜对色散振荡幅度的最大值为50 fs2,用设计制作的啁啾镜对进行色散补偿,用频率分辨光学开关测量装置对脉冲进行测量。将10.3 fs的超短脉冲通过0.5 mm厚的LBO晶体,色散效应导致脉冲展宽,半峰值处的全宽度为39.6 fs,实验结果表明,经过啁啾镜对一次色散补偿后的脉冲形状,半峰值处得全宽度为11.6 fs;脉冲经过2次补偿后,脉冲被压缩到10.7 fs。