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
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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
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
最新試題
主、附港的潮時(shí)差為“-,說(shuō)明()
一般觀測(cè)天體定位應(yīng)避免觀測(cè)高度較低的天體,其主要原因是()
平放六分儀,刻度弧朝外將指標(biāo)桿移至(),眼睛置于動(dòng)鏡后檢查六分儀的動(dòng)鏡差。
根據(jù)《航海天文歷》查取天體位置的查表引數(shù)是()
英版《航海天文歷》高度修正表中太陽(yáng)高度總改正表的查表引數(shù)是()
英版海圖上回轉(zhuǎn)流表列潮流在某個(gè)方向上有兩個(gè)速度,表示()
使用英版《航海天文歷》高度修正表求取真高度時(shí),所有天體必須修正的是()
下列天體觀測(cè)高度的幾個(gè)訂正值中恒為“-”的是()①眼高差②視差③蒙氣差④半徑差
影響蒙氣差的因素有()①氣溫②氣壓③天體高度
將觀測(cè)高度修正為真高度時(shí),不必進(jìn)行視差改正的天體是()