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DEVELOPMENT OF THE SNU COELOSTAT: CONCEPTUAL DESIGN KCI 등재 SCOPUS

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  • URLhttps://db.koreascholar.com/Article/Detail/383947
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천문학회지 (Journal of The Korean Astronomical Society)
한국천문학회 (Korean Astronomical Society)
초록

A coelostat is often used for solar observations, because it corrects the image rotation auto- matically by guiding sunlight into a fixed telescope with two plane mirrors. For the purposes of education and spectroscopic observation, the solar group at Seoul National University (SNU) plans to develop the SNU coelostat (SNUC) and install it in the SNU Astronomical Observatory (SAO). Requirements of the SNUC are < 1′′ positioning accuracy with 30 cm beam size on the entrance pupil in the compact dome. To allow for installation in the small dome, we design a compact slope type coelostat with a 45 cm primary plane mirror and a 39 cm secondary plane mirror. The motion of the SNUC is minimized by fixing the position of the slope frame. Numerical simulations of the available observational time of the designed coelostat shows that the sun can be observed ay all times from June to early August and at least three hours in other months. Since the high accuracy driving motors installed in the SNUC can be affected by external environment factors such as humidity and temperature variations, we design a prototype to test the significance of these effects. The prototype consists of a 20 cm primary plane mirror, a 1 m slope rail, a direct drive motor, a ballscrew, a linear motion guide, an AC servo motor, a reduction gear and a linear encoder. We plan to control and test the accuracy of the prototype with varying atmospheric conditions in early 2019. After testing the prototype, the SNUC will be manufactured and installed in SAO by 2020.

목차
Abstract
1. INTRODUCTION
2. OBSERVATORY
3. CONCEPTUAL DESIGN OF THE SNUC
    3.1. Requirements
    3.2. MathematicalModel
    3.3. Driving Components
4. PROTOTYPE DESIGN
5. SUMMARY AND PLAN
REFERENCES
저자
  • Juhyung Kang(Department of Physics and Astronomy, Seoul National University)
  • Jongchul Chae(Department of Physics and Astronomy, Seoul National University) Corresponding author
  • Hannah Kwak(Department of Physics and Astronomy, Seoul National University)
  • Heesu Yang(Korea Astronomy and Space Science Institute)