1 cm
2 cm
3 cm
4 cm
D. 4 cm
If the applied tension to the tape is more than the standard, the tension correction is positive
If the applied tension to the tape is less than the standard, the tension correction is negative
If the temperature during measurement is greater than the standard temperature, the temperature correction is positive
All the above
Ursa Minor's remains always north of pole star
Polar star remains always north of Polaris
Polaris remains always north of Ursa Minor's
Ursa Minor's pole star and Polaris are the names of the same star
52 m
62 m
72 m
82 m
f tan θ
f sin θ
f cot θ
f cos θ
Zenith
Celestial point
Nadir
Pole
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
10°
20°
30°
40°
Once
Twice
Thrice
Four times
500 m
1000 m
1500 m
2000 m
Focal length of the camera
Overall size of the photo graphs
Percentage of overlap
All the above
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
- 8.8 cos α
+ .8 sin α
+ 8.8 cos α
- 8.8 cos α
Photo principal point
Ground principal point
Ground isocenter
All the above
Every angle is less than two right angles
Sum of the three angles is equal to two right angles
Sum of the three angles less than six right angles and greater than two right angles
Sum of any two sides is greater than the third
Reduction to mean sea level
Correction for horizontal alignment
Correction for slope
All the above
1 in 12
1 in 10
1 in 8
1 in 6
Nadir
Isocenter
Perspective centre
None of these
Principal point
Isocenter
Plumb point
Perspective centre
Isocenter
Principal point
Perspective centre
Plumb line
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
Mean sun
First point of Aries
First point of Libra
The polar star
One degree of longitude has greatest value at the equator
One degree of longitude has greatest value at the poles
One degree of longitude has the same value everywhere
One degree of latitude decreases from the equator to the poles
Triangulation surveying
Astronomical surveying
Hydrographical surveying
Photogrammetric surveying
The star's movement is apparent due to the actual steady rotation of the earth about its axis
The stars move round in circular concentrated parts
The centre of the circular paths of stars is the celestial pole
All the above
Plane surveying
Geodetic surveying
Star observations
Planet observations
δ - θ
θ - δ
θ + δ
½ (θ - δ)
North end of the polar axis is known as North Pole
South end of the polar axis is known as South Pole
Point where polar axis when produced northward intersects the celestial sphere, is known as north celestial pole
All the above
9 cos α
9 sin α
9 tan α
9 cot α
θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°
Ground elevation
Flying height
Length of air base
All the above