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Surveying

Surveying
The correction for parallax, is

- 8".8 cos α
+ 8".8 cos α
- 8".8 cos α
+ .8" sin α

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Surveying
The great circle along which the sun appears to trace on the celestial sphere with earth as centre during the year, is called

Celestial equator
None of these
Ecliptic
Equator

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Surveying
Rotation of the camera at exposure about its vertical axis, is known as

Swing
None of these
Tip
Tilt

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Surveying
The flying height of the camera is 1,000 m above mean ground level, the distance of the top of a building from a nadir point is 10 cm and the relief displacement of building is 7.2 mm. The height of the building, is

62 m
52 m
82 m
72 m

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Surveying
The altitudes of a circumpolar star at culminations are 70° and 10°, both culminations being north of zenith. The latitude of the place, is

80°
70°
40°
60°

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Surveying
The rate of change of parallax dp/dh with respect to change in h, may be expressed as

fB/(H + h)
fB/(H - h)²
fB/(H + h)²
fB/(H - h)

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