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사진측량법을 이용한 대덕전파천문대 13.7미터 안테나의 경면 조정
이창훈,정재훈,강현우,김현구,이영웅,정진오,손영득,배민수,Lee, Changhoon,Jung, J.H.,Kang, H.W.,Kim, H.G.,Lee, Youngung,Jung, J.O.,Sohn, Y.D.,Bae, M.S. 한국천문학회 2014 天文學論叢 Vol.29 No.3
We improved the antenna efficiency of the Taeduk Radio Astronomy Observatory (TRAO) 13.7-m radio telescope by adjusting the antenna panels based on digital photogrammetric measurements. First of all, we measured the surface accuracy of the main reflector of this antenna at three elevation angles of $35^{\circ}$, $45^{\circ}$, and $60^{\circ}$. We performed a total of four sets of the photogrammetric measurements and panel adjustments. When adjusting the panels, we positioned the antenna to the zenith and applied the measured data sets at the elevation of $45^{\circ}$. We found that the antenna surface accuracy has been improved by a factor of ~ 3 times after the final adjustment in comparison with the value before the adjustments. And we also found that the antenna surface accuracy tended to be slightly better at the elevation angles of $35^{\circ}$ and $60^{\circ}$ than that at the elevation angle of $45^{\circ}$. After the final panel adjustment, the aperture and beam efficiencies of the telescope have has been improved from 35% to 44%, and from 41% to 51%, respectively.