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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
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高能物理研究所 [2]
长春光学精密机械与物... [1]
上海应用物理研究所 [1]
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OAI收割 [5]
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期刊论文 [4]
会议论文 [1]
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1998 [2]
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Performance on absolute scattering intensity calibration and protein molecular weight determination at BL16B1, a dedicated SAXS beamline at SSRF
期刊论文
OAI收割
JOURNAL OF SYNCHROTRON RADIATION, 2017, 卷号: 24, 页码: 509-520
作者:
Zeng, JR
;
Bian, FG
;
Wang, J
;
Li, XH
;
Wang, YZ
  |  
收藏
  |  
浏览/下载:20/0
  |  
提交时间:2017/12/08
Beamline
Saxs
Absolute Intensity
Calibration
Molecular Weight
A Comparative Study of the Laser Induced Breakdown Spectroscopy in Single- and Collinear Double-Pulse Laser Geometry
期刊论文
OAI收割
PLASMA SCIENCE & TECHNOLOGY, 2014, 卷号: 16, 页码: 374-379
作者:
Sun Duixiong
;
Su Maogen
;
Dong Chenzhong
;
Wen Guanhong
  |  
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2018/07/05
Plasma Diagnostics
Intensity Calibration
Emission Signal Enhancement
The calibration of faint simulation star magnitude based on single photon count technique (EI CONFERENCE)
会议论文
OAI收割
International Symposium on Photoelectronic Detection and Imaging 2009: Advances in Imaging Detectors and Applications, June 17, 2009 - June 19, 2009, Beijing, China
作者:
Xu S.-Y.
;
Guo J.
;
Guo J.
收藏
  |  
浏览/下载:37/0
  |  
提交时间:2013/03/25
A calibration method of faint star magnitude of the star scene simulation device is proposed in this paper. In the research of simulation star magnitude
luminometers and CCD devices are the general calibration devices which are used to measure the illumination intensity and calibrate its magnitude. But if the simulation magnitude is only sixth magnitude
its illumination intensity is only 1.010-8 Lux. This illumination intensity level is the lowest illumination intensity that the commercial luminometer can detect. Hence the simulation star magnitude lower than six magnitude cannot be calibrated by luminoters. Likewise CCD devices also need an additive cooler in this case. When the single photon characteristic is presented due to the low luminosity of simulating light sources
the simulation star magnitude can be calibrated by detecting its photon flux of radiation with the method of single photon count. In this paper the detection principle of single photon based on a compact designed PMT detecting of the radiation level of simulation star magnitude is advanced. Especially a spectrum match method is proved theoretically to be an effective means for selecting PMT photosensitive type. In the case of the detection object of the simulation star in visible wavelength
a analysis indicates that the material of tri-alkali cathode materials its best choice after being compared the Signal-to-Noise of photon detector of several PMT photosensitive materials based on the different spectrum match ratio of different object light sources and different cathode materials. An experiment is employed to show the relationship of control voltage of PMT and its dark counter
the relationship of the environment temperature of PMT and its dark counter
which proves its only decades of CPS at room temperature. The so low dark counter avoids a bulky cooler and is convenient for installing it on the star scene simulation equipment. Finally in the experiment of calibrating the simulation star magnitudes the ability of its calibration is confirmed to reaches up to 12m
meanwhile its calibration error is within 0.2m. 2009 SPIE.
Design and calibration of the measuring system for soft X-ray absolute intensity
期刊论文
OAI收割
HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION, 1998, 卷号: 22, 期号: 2, 页码: #REF!
作者:
Cui CW(崔聪悟)
;
Cui MQ(崔明启)
;
Cui, CW
;
Cui, MQ
;
Yi, RQ
收藏
  |  
浏览/下载:28/0
  |  
提交时间:2016/04/12
soft X-ray absolute intensity measurement
ionization chamber
calibration
A new ion chamber with a movable photodiode monitor for absolute intensity measurements of soft X-rays
期刊论文
OAI收割
JOURNAL OF SYNCHROTRON RADIATION, 1998, 卷号: 5, 期号: 3, 页码: 872-873
作者:
Cui CW(崔聪悟)
;
Cui MQ(崔明启)
;
Cui, CW
;
Cui, MQ
;
Yi, RQ
收藏
  |  
浏览/下载:23/0
  |  
提交时间:2016/06/28
ion chambers
calibration
soft X-ray absolute intensity measurements