SOLAR EPHEMERIS BY DE405

DE405를 이용한 태양계 천체력 계산

  • KIM HYO RYOUNG (Taeduk Radio Astronomy Observatory, Korea Astronomy Observatory) ;
  • ROH DUK GYOO (Taeduk Radio Astronomy Observatory, Korea Astronomy Observatory) ;
  • CHUNG HYUN SOO (Taeduk Radio Astronomy Observatory, Korea Astronomy Observatory) ;
  • JUNG JAE HOON (Taeduk Radio Astronomy Observatory, Korea Astronomy Observatory) ;
  • CHO SE HYUNG (Taeduk Radio Astronomy Observatory, Korea Astronomy Observatory) ;
  • AHN YOUNG SOOK (Taeduk Radio Astronomy Observatory, Korea Astronomy Observatory)
  • 김효령 (한국천문연구원, 대덕전파천문대) ;
  • 노덕규 (한국천문연구원, 대덕전파천문대) ;
  • 정현수 (한국천문연구원, 대덕전파천문대) ;
  • 정재훈 (한국천문연구원, 대덕전파천문대) ;
  • 조세형 (한국천문연구원, 대덕전파천문대) ;
  • 안영숙 (한국천문연구원, 대덕전파천문대)
  • Published : 2001.12.01

Abstract

The DE405 ephemeride is introduced as TRAO solar ephemeris system to support the apparent coordinates of planets after 2000. The time delay between planets and observer has to be regarded to get the apparent position of planet. Some fast algorithms about time delay are suggested to reduce the computing time. The CSI method is applied to run these algorithms on any O/S including both real-time and run-time machine.

Keywords