XUV光谱仪

发布:谈谈光电子 2014-11-02 18:37 阅读:1190
XUV光谱仪是新型的像差校正平场入射X射线光谱仪,光谱范围可涵盖1-80nm.模块化设计,可以满足不同的实验条件和环境。 F",TP,X  
    单光栅标准配置)可覆盖5-80nm测量范围 vy{k"W&S  
技术参数
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波长范围
pe2:~}WB  
5-20
H(P]Z~et  
10-60
p<#aXs jy  
25-80
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光源距离(m)
Y:L[Iz95o  
0"T/a1S7bl  
0.4-0.6
$eG_LY 1v  
0.5-1.5
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平场尺寸(mm)
)KVr2y;RF  
25.4
M \  
50
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50
LjTSu9I>  
色散(nm/mm)
*78c2`)[  
0.5-0.7
J:gC1g^  
0.7-1.1
_ SOwiz  
0.9-1.3
#+V4<o  
光谱分辨率(nm)
9H/R@i[E  
0.06
|iX>hJSl  
0.09
dcD#!v\0  
0.11
Q"nw.FjUG  
0.02(CCD探测器)
OFyy!r@?  
升级波长范围
r@qLG"[\c  
可拓展至1-5nm(搭配该范围光栅)
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探测器选择
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X-Ray 相机,MCP探测器,fiber taper系统
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光栅台
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电控
]@<VLP?  
工作环境
B["+7\c<~  
<10-6mbar
DuR9L'  
操作性
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极易安装使用,用户自己即可安装使用
v[{7\Hha  
k{{3nenAG  
技术优势介绍: v<g=uEpN  
- Direct imaging of the source / Superior signal strength 6Aq]I$  
In contrast to conventional devices our XUV spectrometer does not zow8 Q6f  
require a narrow entrance aperture but rather images the harmonic source ,d38TN  
directly onto the detector. Thus 80% or more of the incoming beam can be 0XCAnMVo  
used for measurement. Please see Z|Rc54Ct  
http://www.hoerlein-partner.com/#!services/cihc for a sketch drawing. `[(XZhN  
This configuration typically collects 15 to 25 times more light than jll:Rh(b  
standard versions, resulting in a signal-to-noise figure improved by the g3&nxZ  
same ratio. n7K%lj-.P  
In some experiments, this improved signal strength is the crucial step 9T5 F0?qd  
for realizing a measurement at all. ^>Z_3 {s:$  
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- Flat-field imaging technology fW+ "Kuw  
Our instruments are based on high quality aberration-corrected yq k8)\p  
flat-field gratings. In contrast to conventional gratings these focus 4:NMZ `~  
all wavelengths onto a plane rather than a circle. This allows for l5Ko9CG  
positioning the entire detector in the focal plane of the grating for 8a)Brl}u  
superior spectral resolution. gj @9(dk%  
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- Compactness / Modularity [~ 2m*Q  
The spectrometer is very compact and can be bolted directly to a vacuum P-gjSE|yh  
chamber. It is capable of carrying its own weight, no table required. G~(\N?2  
There are no externally moving parts. [r8[lkR  
Through its modular design, our spectrometer can be adapted to a number K-#d1+P+  
of configurations (source distance, spectral range, detectors, vacuum FGHCHSqLq  
pumping, etc). This makes it highly flexible for varying requirements "``>ii  
and experiments. =RD>#'sUK  
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- Robust against misalignment l1'v`!  
The compact design of the spectrometer makes it inherently insensitive (?R!y -  
against mechanical and environmental disturbances (vibrations, pC,[!>0g8  
acoustics, etc). No externally moving parts and closed-loop grating ]bh%pn  
actuators with absolute position monitoring add to the robustness and *nJ,|T  
allow for monitoring of the grating alignment at all times. df@NV Ld  
In addition, the concept of a spectrometer without entrance slit also v+in:\Dv  
makes the instrument less sensitive to misalignment. Under typical E]/2 u3p  
operating conditions a misalignment of the beam in the dispersion {G x=QNd  
direction on the entrance of the spectrometer by 500um would lead to a 6Yodx$  
signal reduction by more than 20% in an instrument with entrance slit s9CmR]C  
while it is less than 10% for our design. Z^%a 1>`  
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- Customization B t}90#  
The adaptability of our XUV spectrometer makes it possible to highly RIXeV*ix  
custom-fit the device to requirements. Thus we offer to customize every Q\kWQOB_  
spectrometer to exactly match the desired research application. This gs3(B/";c  
includes e.g. interfacing to experimental chambers, adaption of the b)KEB9w  
source distance, integration of customer-supplied detectors, )G^k$j  
user-defined filter mounts, non-magnetic instruments, special mounting E9j<+Ik  
situations, etc. s.Z{mnD6  
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典型客户: T%6JVFD  
1) 苏黎世联邦理工学院 bS~Y_]B  
2) The Institute of Electronic Structure and Laser of the Foundation for Research and Technology-Hellas (IESL-FORTH) \u[}  
3) MPQ D|)_c1g  
4) Los Alamos 1q-;+Pd;  
5) Max Planck Institute qm><}N7f  
上海达灿光电科技有限公司 99ZWB  
021-60450828
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