Bibliography



Notice:

  • Clicking on the title will open a new window with all details of the bibliographic entry.
  • Clicking on the DOI link will open a new window with the original bibliographic entry from the publisher.
  • Clicking on a single author will show all publications by the selected author.
  • Clicking on a single keyword, will show all publications by the selected keyword.



Found 2 entries in the Bibliography.


Showing entries from 1 through 2


2013

Study on near-far ultraviolet imaging spectrometer with high resolution

A near-far ultraviolet imaging spectrometer with high resolution is developed，which can be applied to the upper atmosphere observation in 115nm-295nm. The application demands of the corresponding remote sensing are analyzed. Because the imaging spectrum technology has been rarely utilized for the ionosphere observation in our country, we study some foreign advanced loads to apply the standard to our design. According to the analysis, the optical system of the imaging spectrometer is designed. The system includes an off-axis parabolic mirror as the telescope and Czerny-Turner structure as the imaging spectrum system. The photon counting detector is adopted to satisfy the observation for that the radiation is weak in near-far ultraviolet waveband. The receiving surface of the detector should be coated by different photocathode for better quantum efficiency in the near and far ultraviolet wavebands. The traditional Czerny-Turner system is not suit for the broadband imaging spectrometer because aberrations in the structure can\textquoterightt be corrected homogeneously. The geometric analysis and 1st order differential calculation method are introduced to improve disadvantages based on the aberration theory. We designed an example for the advanced imaging spectrometer. The results demonstrate that the modulation transfer function (MTF) in total field of view and the waveband is more than 0.6. The design has high spatial resolution and high spectral resolution. It certificates that the design theory can be applied to the near-far ultraviolet imaging spectrometer especial for upper atmosphere observation. \textcopyright (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.

Cong, Hai-fang; Wang, Chunhui; Wang, Yu;

Published by:       Published on:

YEAR: 2013     DOI: 10.1117/12.2032920

Imaging spectrometer; Near-far ultraviolet; Spatial resolution; Spectral resolution

2009

Design of FUV imaging spectrometer based on crossed Czerny-Turner structure

This article describes the characteristics of the far ultraviolet (FUV) radiation and its applications in the space weather s research and prediction. The FUV imaging spectrometer is irreplaceable to get the FUV radiation data of the earth s upper atmosphere. Some key technologies of FUV spectrometer are analyzed respectively, including window materials, FUV light source, FUV detectors and FUV coating, which offer theoretical foundation for FUV imaging spectrometer. The paper presents a FUV band imaging spectrometer s optical system which is based on crossed Czerny-Turner structure with all reflective components in it. The wavelength range of the FUV spectrometer optical system is from 100nm to 200nm and the initial structure is simulated and optimized by Zemax in order to improve the spectral resolution. The theoretical spectral resolution of the system is better than 1nm, and it has a certain imaging capacity.

Wu, Yan; Tang, Yi; Ni, Guoqiang; Sheng, Yunlong; Wang, Yongtian; Zeng, Lijiang;

Published by:       Published on:

YEAR: 2009     DOI: 10.1117/12.806967

space weather; far ultraviolet; Imaging spectrometer; crossed Czerny-Turner system; optical design



  1