XUV光谱仪

发布:谈谈光电子 2014-11-02 18:37 阅读:1226
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。 cPSti  
    单光栅标准配置)可覆盖5-80nm测量范围 ' rvE  
技术参数
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波长范围
ILNXaJ'0a  
5-20
YLE/w@*  
10-60
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25-80
K9^"NS3  
光源距离(m)
eZ A6D\  
cXMa\#P  
0.4-0.6
ZLuPz#  
0.5-1.5
h*l cEzG?A  
平场尺寸(mm)
) u-ns5  
25.4
1Lc8fP$  
50
*iYMX[$  
50
C&e8a9*,(a  
色散(nm/mm)
8ZFH}v@V1'  
0.5-0.7
R7,p ukK  
0.7-1.1
Z|}H^0~7S  
0.9-1.3
i"< ZVw  
光谱分辨率(nm)
{x|MA(NO  
0.06
:Fc8S9  
0.09
d;<.;Od$`  
0.11
k5q(7&C  
0.02(CCD探测器)
|MVV +.X  
升级波长范围
'Z y{mq\  
可拓展至1-5nm(搭配该范围光栅)
u!M& ;QL  
探测器选择
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X-Ray 相机,MCP探测器,fiber taper系统
8cB=}XgYS  
光栅台
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电控
M*v^N]>"G  
工作环境
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<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: uht(3  
- Direct imaging of the source / Superior signal strength DhHtz.6  
In contrast to conventional devices our XUV spectrometer does not 2UQN*_  
require a narrow entrance aperture but rather images the harmonic source `..EQ BM  
directly onto the detector. Thus 80% or more of the incoming beam can be . c#90RP  
used for measurement. Please see &:-GI)[o  
http://www.hoerlein-partner.com/#!services/cihc for a sketch drawing. $x/J+9Ww  
This configuration typically collects 15 to 25 times more light than )eVzSj>MT  
standard versions, resulting in a signal-to-noise figure improved by the <. ezw4ju  
same ratio. mSy|&(l  
In some experiments, this improved signal strength is the crucial step av"Dljc  
for realizing a measurement at all. Xad G\_?t`  
u6]gQP">I  
- Flat-field imaging technology {n pOlV  
Our instruments are based on high quality aberration-corrected  MK<  
flat-field gratings. In contrast to conventional gratings these focus /@6E3lh S  
all wavelengths onto a plane rather than a circle. This allows for <1TlW ~q<  
positioning the entire detector in the focal plane of the grating for ux%&lff  
superior spectral resolution. c]S+70!n  
=CWc`  
- Compactness / Modularity 'W}~)+zK  
The spectrometer is very compact and can be bolted directly to a vacuum pHigxeV2  
chamber. It is capable of carrying its own weight, no table required. w{RNv%hJ$=  
There are no externally moving parts. 8moUK3w  
Through its modular design, our spectrometer can be adapted to a number Pv^(Q ]  
of configurations (source distance, spectral range, detectors, vacuum v`@5enr  
pumping, etc). This makes it highly flexible for varying requirements ;OQ#@|D  
and experiments.  <WO&$&  
f34_?F<h  
- Robust against misalignment zuK/(qZ  
The compact design of the spectrometer makes it inherently insensitive d&O'r[S  
against mechanical and environmental disturbances (vibrations, =PI^X\if88  
acoustics, etc). No externally moving parts and closed-loop grating [8 {_i?wY  
actuators with absolute position monitoring add to the robustness and pK-_R#  
allow for monitoring of the grating alignment at all times. [c,|Lw4  
In addition, the concept of a spectrometer without entrance slit also #(m `2Z`H  
makes the instrument less sensitive to misalignment. Under typical 0*/mc96  
operating conditions a misalignment of the beam in the dispersion MA~|y_V  
direction on the entrance of the spectrometer by 500um would lead to a Pn~pej5'K  
signal reduction by more than 20% in an instrument with entrance slit :;|)/  
while it is less than 10% for our design. n ;Ql=4  
:!r9 =N9  
- Customization 7qCJ]%)b6  
The adaptability of our XUV spectrometer makes it possible to highly }IxY(`:qs  
custom-fit the device to requirements. Thus we offer to customize every WZfk}To1#  
spectrometer to exactly match the desired research application. This 53g8T+`\(  
includes e.g. interfacing to experimental chambers, adaption of the $q4XcIX 7  
source distance, integration of customer-supplied detectors, QC$=Fs5+  
user-defined filter mounts, non-magnetic instruments, special mounting ykErt%k<n  
situations, etc. Ukk-(gjX  
)$2%&9b  
典型客户: G1`mn$`kq  
1) 苏黎世联邦理工学院 Z"teZ0H  
2) The Institute of Electronic Structure and Laser of the Foundation for Research and Technology-Hellas (IESL-FORTH) .=.yZ  
3) MPQ MAm1w'ol"  
4) Los Alamos hNu>s  
5) Max Planck Institute [lDt0l5^  
上海达灿光电科技有限公司 z*??YUT\M  
021-60450828
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