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谈谈光电子 2014-11-02 18:37

XUV光谱仪

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。  ~ e?af  
    单光栅(标准配置)可覆盖5-80nm测量范围 . U6(>6-  
技术参数
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波长范围
"#pxZ B=  
5-20
*ezMS   
10-60
^"I@ 8k  
25-80
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光源距离(m)
{_(R?V]w,  
-!7Z  
0.4-0.6
c0e[vrP:  
0.5-1.5
@0EY5{&  
平场尺寸(mm)
 #9}1Lo>  
25.4
B2$cY;LH  
50
}XUI1H]jk  
50
5!'1;GLs  
色散(nm/mm)
V/\Y(Mxc  
0.5-0.7
c ZYvP  
0.7-1.1
]pB5cq7o  
0.9-1.3
9xJtDdy-O  
光谱分辨率(nm)
cX1?4e8  
0.06
r$4d4xtK  
0.09
5V(#nz  
0.11
PJm@fK(j  
0.02(CCD探测器)
_oa*E2VN  
升级波长范围
RgH 6l2  
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
H1?C:R  
光栅台
~kV>nx2  
电控
*wx%jbJo  
工作环境
$Lfbt=f  
<10-6mbar
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操作性
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极易安装使用,用户自己即可安装使用
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技术优势介绍: UzSDXhzObf  
- Direct imaging of the source / Superior signal strength b-VQn5W  
In contrast to conventional devices our XUV spectrometer does not JDa_;bqL  
require a narrow entrance aperture but rather images the harmonic source on8$Kc  
directly onto the detector. Thus 80% or more of the incoming beam can be 1jKj' 7/K  
used for measurement. Please see OB=bRLd.IR  
http://www.hoerlein-partner.com/#!services/cihc for a sketch drawing. &x*l{s[  
This configuration typically collects 15 to 25 times more light than 1+3-Z>^e  
standard versions, resulting in a signal-to-noise figure improved by the 6||%T$_;}  
same ratio. Q: -&  
In some experiments, this improved signal strength is the crucial step kc$W"J@  
for realizing a measurement at all. lz>.mXdx  
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- Flat-field imaging technology hEo$Jz`  
Our instruments are based on high quality aberration-corrected so.}WU  
flat-field gratings. In contrast to conventional gratings these focus N@Ap|`Ei  
all wavelengths onto a plane rather than a circle. This allows for v;z8g^L  
positioning the entire detector in the focal plane of the grating for "UY34a^I  
superior spectral resolution. T,/<'cl"  
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- Compactness / Modularity mV"F<G; H  
The spectrometer is very compact and can be bolted directly to a vacuum KU/QEeqbrp  
chamber. It is capable of carrying its own weight, no table required. hB>FJZQ_  
There are no externally moving parts. &a\w+  
Through its modular design, our spectrometer can be adapted to a number =7kn1G.(  
of configurations (source distance, spectral range, detectors, vacuum &uaSp, L  
pumping, etc). This makes it highly flexible for varying requirements leSBR,C  
and experiments. qD"~5vtLqQ  
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- Robust against misalignment TL"+Iv2]/$  
The compact design of the spectrometer makes it inherently insensitive Ssir?ZUm   
against mechanical and environmental disturbances (vibrations, e :ub]1I=  
acoustics, etc). No externally moving parts and closed-loop grating Xe`$SNM  
actuators with absolute position monitoring add to the robustness and _a$5"  
allow for monitoring of the grating alignment at all times. iV@\v0k  
In addition, the concept of a spectrometer without entrance slit also 75P!`9bE  
makes the instrument less sensitive to misalignment. Under typical YGyw^$.w  
operating conditions a misalignment of the beam in the dispersion GM^H )8U  
direction on the entrance of the spectrometer by 500um would lead to a tycVcr \(  
signal reduction by more than 20% in an instrument with entrance slit * >NML]#0  
while it is less than 10% for our design. (IHR {m  
:SMf (E 5  
- Customization ) .V,zmI  
The adaptability of our XUV spectrometer makes it possible to highly &C9)%5 O)  
custom-fit the device to requirements. Thus we offer to customize every $i3`cX)g  
spectrometer to exactly match the desired research application. This rnMi >?  
includes e.g. interfacing to experimental chambers, adaption of the WqCER^~'>  
source distance, integration of customer-supplied detectors, 5Em.sz;:8  
user-defined filter mounts, non-magnetic instruments, special mounting K-.%1d@$y  
situations, etc. D 7thLqA  
z+0#H39&  
典型客户: PK{FQ3b2{  
1) 苏黎世联邦理工学院 "K|':3n|  
2) The Institute of Electronic Structure and Laser of the Foundation for Research and Technology-Hellas (IESL-FORTH) $Mx?Y9!  
3) MPQ 3$_- 0>  
4) Los Alamos \\oa[nvL~  
5) Max Planck Institute o {q8An)  
上海达灿光电科技有限公司 :< ]sJf N  
021-60450828
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