High-resolution diffraction grating interferometric transducer of linear displacements

Author(s):  
Ping Shang ◽  
Haojie Xia ◽  
Yetai Fei
2005 ◽  
Vol 13 ◽  
pp. 790-792
Author(s):  
Webster Cash

AbstractThe diffraction grating spectra from Chandra and XMM-Newton have given the astronomical community a huge step forward in x-ray spectroscopy of celestial sources. They have proven the scientific richness of the field. But the spectra have resolution of only 300 to 1000 – low by the standards of the visible and the ultraviolet. We discuss some of the exciting new science that can be addressed if spectral resolution of up to 10,000 (or more) can be achieved in the x-ray. We then show how practical, high efficiency, high resolution x-ray spectrographs can be built for high throughput missions like Constellation-X and XEUS.


2016 ◽  
Vol 5 (3) ◽  
pp. 20 ◽  
Author(s):  
N. Moultif ◽  
E. Joubert ◽  
O. Latry

In this paper, we present one of the most important failure analysis tools that permits the localizing and the identification of the failure mechanisms. It is a new spectral photon emission system, enabling to localize the failure, and quickly get the photon emission spectra that characterize the failure with high resolution. A diffraction grating is used as a spectrometer in the system. Application results on mechatronic power devices such as HEMT AlGaN/GAN and SiC MOSFETs are reported.


2000 ◽  
Author(s):  
Jerzy Helsztynski ◽  
Wieslaw Jasiewicz ◽  
Kazimierz P. Jedrzejewski ◽  
Lech Lewandowski ◽  
Krzysztof T. Pozniak

2006 ◽  
Author(s):  
M. P. Kowalski ◽  
F. B. Berendse ◽  
T. W. Barbee, Jr. ◽  
W. R. Hunter ◽  
K. F. Heidemann ◽  
...  

2013 ◽  
Vol 347-350 ◽  
pp. 49-54
Author(s):  
Li Dong Wang ◽  
Zhen Hua Mao ◽  
Zhe Min Chen ◽  
Bing Hui Ma

This paper introduces a homemade high-resolution miniature fiber optic spectrometer for LIBS detection. The circuit part of the system is mainly controlled by a cortex-M3 chip, transmits data to the personal computer (PC) through the Universal Serial BUS (USB2.0), and a set of spectrometer test software is finished. The optical system is based on Czerny-Turner imaging system, using 1800grv/mm plane diffraction grating, 16μm slit and 2048 pixels linear array CCD as detector, high-resolution spectral output in the range of 335-455nm is required. By precisely calibration and testing, the precision of the system is 0.05nm, and the resolution of the wavelength at the blaze wavelength can up to 0.1nm which can fulfill the general LIBS detection.


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