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
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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
A.refraction of light as it enters the Earth's atmosphere
B.rotation of the Earth on it's axis
C.the body's orbital motion during the time required for its light to reach Earth
D.a false horizon
A.is nearest to the Earth
B.is farthest from the Earth
C.is on the opposite side of the Earth from the Moon
D.and Moon and Earth are in line
A.Sirius
B.Canopus
C.Venus
D.Jupiter
最新試題
以()為引數(shù)查《航海天文歷》獲取太陽、行星的格林時角和赤緯。
根據(jù)《航海天文歷》查取天體位置的查表引數(shù)是()
英版海圖上回轉(zhuǎn)流表列潮流在某個方向上有兩個速度,表示()
一般觀測天體定位應(yīng)避免觀測高度較低的天體,其主要原因是()
使用英版《航海天文歷》高度修正表求取真高度時,所有天體必須修正的是()
縮小六分儀邊差的方法是()
下列天體觀測高度的幾個訂正值中恒為“-”的是()①眼高差②視差③蒙氣差④半徑差
英版《潮汐表》中,潮高差是()
航用海圖上繪畫天文船位線,當(dāng)天體真高度大于天體計算高度時,應(yīng)()截取高度差。
觀測天體高度前的準(zhǔn)備工作包括()①預(yù)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(yīng)環(huán)境溫度⑤檢查校正六分儀誤差,調(diào)整好望遠鏡焦距