Photometric Calibration of the Barium Cloud Image in a Space Active Experiment: Determining the Release Efficiency

The barium release experiment is an effective method to explore the near-earth environment and to study all kinds of space physics processes. The first space barium release experiment in China was successfully carried out by a sounding rocket on April 5, 2013. This work is devoted to calculating the...

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Published inChinese physics letters Vol. 31; no. 1; pp. 186 - 189
Main Author 谢良海 李磊 王劲东 陶然 程炳钧 张艺腾
Format Journal Article
LanguageEnglish
Published 2014
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ISSN0256-307X
1741-3540
DOI10.1088/0256-307X/31/1/019401

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Summary:The barium release experiment is an effective method to explore the near-earth environment and to study all kinds of space physics processes. The first space barium release experiment in China was successfully carried out by a sounding rocket on April 5, 2013. This work is devoted to calculating the release efficiency of the barium release by analyzing the optical image observed during the experiment. First, we present a method to calibrate the images grey value of barium cloud with the reference stars to obtain the radiant fluxes at different moments. Then the release efficiency is obtained by a curve fitting with the theoretical evolution model of barium cloud. The calculated result is basically consistent with the test value on ground.
Bibliography:11-1959/O4
XIE Liang-Hai, LI Lei, WANG Jing-Dong, TAO Ran, CHENG Bing-Jun, ZHANG Yi-Teng (1 Center for Space Science and Applied Research, Chinese Academy of Sciences, Bcijing 100190 2 University of Chinese Academy of Sciences, Beijing 100049)
The barium release experiment is an effective method to explore the near-earth environment and to study all kinds of space physics processes. The first space barium release experiment in China was successfully carried out by a sounding rocket on April 5, 2013. This work is devoted to calculating the release efficiency of the barium release by analyzing the optical image observed during the experiment. First, we present a method to calibrate the images grey value of barium cloud with the reference stars to obtain the radiant fluxes at different moments. Then the release efficiency is obtained by a curve fitting with the theoretical evolution model of barium cloud. The calculated result is basically consistent with the test value on ground.
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ISSN:0256-307X
1741-3540
DOI:10.1088/0256-307X/31/1/019401