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
在六分儀上直接讀取太陽的下邊緣觀測高度,并利用英版《航海天文歷》求太陽的真高度,則需要修正哪些誤差?()①器差②指標差③眼高差④綜合改正⑤附加改正
下列哪項不是高度差法求天文船位線的三要素?()
在觀測太陽中天高度求緯度計算中,當其高度命名為N,頂距命名為S,說明太陽方位為正()
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()
測定羅經差精度較高的方法是()
根據《航海天文歷》查取天體位置的查表引數是()
將觀測高度修正為真高度時,不必進行視差改正的天體是()
縮小六分儀邊差的方法是()
使用英版《航海天文歷》高度修正表求取行星真高度時,總改正的查表引數是()
將觀測高度修正為真高度時,需要進行半徑差改正的天體是()