Latitudes north of the equator are taken as positive
Latitudes south of the equator are taken as negative
Longitudes east of Greenwich are taken as negative
Longitudes west of Greenwich are taken as positive
C. Longitudes east of Greenwich are taken as negative
Satellite station
Eccentric station
False station
Pivot station
Plane surveying
Geodetic surveying
Star observations
Planet observations
29 days
29.35 days
29.53 days
30 days
Principal point coincides the isocenter
Iso-centre coincides the plumb point
Plumb point coincides the principal point
All the above
Swing
Tilt
Tip
None of these
Refraction correction is zero when the celestial body is in the zenith
Refraction correction is 33' when the celestial body is on the horizon
Refraction correction of celestial bodies depends upon their altitudes
All the above
March 21
June 21
September 21
December 22
180° eastward
180° westward
180° east or westward
360° eastward
Centre of the celestial sphere is taken as the position of the observer
Centre of the celestial sphere is taken as the centre of the earth
Stars move and maintain their relative positions
All the above
1 in 12
1 in 10
1 in 8
1 in 6
5100 nautical miles
5700 nautical miles
120 nautical miles
500 nautical miles
Eastward
Westward
Northward
Southward
- 8.8 cos α
+ .8 sin α
+ 8.8 cos α
- 8.8 cos α
Focal length of the camera
Overall size of the photo graphs
Percentage of overlap
All the above
λ = α
λ = 90° - α
λ = α - 90°
λ = 180° - α
Meridian
Vertical circle
Prime vertical
None of these
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
Control points for surveys of large areas
Control points for photogrammetric surveys
Engineering works, i.e. terminal points of long tunnels, bridge abutments, etc.
All the above
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
Nadir
Isocenter
Perspective centre
None of these
365
365.2224
365.2422
366.2422
Elevation of the elevated pole
Declination of the observer's zenith
Angular distance along the observer's meridian between equator and the observer
All the above
1000 km
800 km
600 km
500 km
Photo principal point
Ground principal point
Ground isocenter
All the above
Isocenter
Plumb point
Principal point
None of these
2 mm
4 mm
6 mm
10 mm
1 cm
2 cm
3 cm
4 cm
The direction of the vertical, the axis of rotation of the instrument
The direction of the poles of the celestial sphere
The direction of the star from the instrument
All the above
The plane passing through the perspective centre of a stereo pair and a ground point, is known as basal plane
Each pair of image points on stereo pair have their own basal plane
Relative orientation means reconstructing the basal plane
All the above
The horizontal direction of the pole is called astronomical north
The angle between the direction of true north and the direction of a survey line is called astronomical bearing
The astronomical bearing is generally called azimuth
All the above