A.the departure
B.the polar arc
C.longitude
D.Greenwich hour angle
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A.when the declination and latitude are of different names
B.when the declination is greater than and the same name as the latitude
C.if the vessel is stopped or making bare steerageway
D.on a fast vessel on northerly or southerly headings
A.the Sun is at maximum declination north or south
B.a planet crosses the external plane of the ecliptic
C.the Sun is between the Earth and a planet
D.two planets are in line
A.used with the equation of time
B.used in the form of LHA Aries
C.calculating the time of moonrise
D.determining local apparent time
A.as the basis for star charts
B.to enter a star finder
C.in sight reduction using Pub 249
D.in sight reductions of planet observations
A.calculating amplitudes
B.calculating great circle sailings by the Agiton method
C.entering the Air Navigation Tables (Selected Stars) Pub 249
D.plotting on star finders
最新試題
使用航海六分儀測天時,不能用近物標測定的指標差作為觀測天體時的六分儀指標差,是因為()
測者可自行校正的六分儀誤差有:①定鏡差;②指標差;③動鏡差。三者正確的校正順序是()
航海上測定指標差時,可以利用()①星體②太陽③水天線
英版《航海天文歷》高度修正表中太陽高度總改正表的查表引數(shù)是()
英版海圖上回轉流表列潮流在某個方向上有兩個速度,表示()
在中版《航海天文歷》的“恒星視位置表”中可查取恒星的()①地方時角②格林時角③共軛赤經(jīng)④赤緯
《航海天文歷》中列出的太陽出沒時刻是()
縮小六分儀邊差的方法是()
關于英版《航海天文歷》高度修正表中的眼高差表的說法正確的是()
觀測天體高度前的準備工作包括()①預求觀測時間②檢查秒表狀態(tài),使表時歸零③推算測天時的天文鐘鐘差④提前將六分儀拿到室外,適應環(huán)境溫度⑤檢查校正六分儀誤差,調整好望遠鏡焦距