天体周日视运动过程中天体高度的变化率  

The Altitude Ratio of a Celestial Body in its Diurnal Apparent Motion

作　　者：毕修颖[1] 崔照明[1] 

机构地区：[1]广东海洋大学航海学院,广东湛江524025

出　　处：《湛江海洋大学学报》2006年第1期49-52,共4页Journal of Zhanjiang Ocean University

摘　　要：天体周日视运动过程中天体的高度不断变化,对天体观测的质量有直接的影响,通过分析天体周日视运动过程中天体高度的变化率,给出不同观测时机进行天体高度观测的特性,并用曲线图的形式给出天体高度变化率的极值点和零值点。航海人员可以从更深的层次认识天体周日视运动的规律,指导天文定位过程中对天体高度的观测。The altitudes of a celestial body are always changing during its diurnal apparent motion, which affects directly the quality of celestial observations. This paper analyses the altitude ratio of a celestial body in its diurnal apparent motion, puts forward the characteristics of altitude observation in different sighting opportunities, and gives the altitude ratio exttremun using curves and graphs. Therefore, mariners can fully understand the rules of diurnal apparent motion, and can be guided in their future observations.

关 键 词：天体周日视运动 天体高度观测 观测时机 

分 类 号：U675.6[交通运输工程—船舶及航道工程]