천문학회지 (Journal of The Korean Astronomical Society)

  • 제38권4호
  • /
  • Pages.463-470
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  • 2005
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  • 1225-4614(pISSN)
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  • 2288-890X(eISSN)
한국천문학회 (The Korean Astronomical Society)
권호 표지
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COMPONENT-BASED DEVELOPMENT OF OBSERVATIONAL SOFTWARE FOR KASI SOLAR IMAGING SPECTROGRAPH

  • Choi, Seong-Hwan (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Kim, Yeon-Han (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Moon, Yong-Jae (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Choi, Kyung-Seok (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Park, Young-Deuk (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Jang, Bi-Ho (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Kim, Su-Jin (Solar and Space Weather Research Group, Korea Astronomy and Space Science Institute) ;
  • Kim, Kap-Sung (Department of Astronomy and Space Science, Kyunghee University)
  • 발행 : 2005.12.01
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초록

In this paper, we have made the component-based development of observational software for KASI solar imaging spectrograph (KSIS) that is able to obtain three-dimensional imaging spectrograms by using a scanning mirror in front of the spectrograph slit. Since 2002, the KASI solar spectrograph has been successfully operated to observe solar spectra for a given slit region as well as to inspect the response functions of narrow band filters. To improve its capability, we have developed the KSIS that can perform sequential observations of solar spectra by simultaneously controlling the scanning mirror and the CCD camera via Visual C++. Main task of this paper is to introduce the development of the component-based software for KSIS. Each component of the software is reusable on the level of executable file instead of source code because the software was developed by using CBD (component-based development) methodology. The main advantage of such a component-based software is that key components such as image processing component and display component can be applied to other similar observational software without any modifications. Using this software, we have successfully obtained solar imaging spectra of an active region (AR 10708) including a small sunspot. Finally, we present solar $H{\alpha}$ spectra ($6562.81{\AA}$) that were obtained at an active region and a quiet region in order to confirm the validity of the developed KSIS and its software.

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참고문헌

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