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
D. All the above
8,000 m
10,000 m
12,000 m
14,000 m
Eastward
Westward
Northward
Southward
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
All the above
March 21
June 21
September 21
December 22
365
365.2224
365.2422
366.2422
Sun and moon are in line with earth
Solar tidal force acts opposite to lunar tidal force
Solar tidal force and lunar tidal force both coincide
None of these
Ground principal point
Ground plumb point
Iso-centre
Perspective centre
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
θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°
Lengths
Angles
Heights
All of these
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
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
1 cm
2 cm
3 cm
4 cm
Nadir
Isocenter
Principal point
Plumb point
Sidereal time
Apparent solar time
Mean solar time
All the above
The standard meridian
The international date line
That of Greenwich
Both (a) and (c) of above
The length of the air base is increased
The scale of the model is altered
y-parallax is not affected
All the above
30°
35°
40°
45°
0.01 second
0.001 second
0.0001 second
None of these
29 days
29.35 days
29.53 days
30 days
Swing
Tilt
Tip
None of these
The measured stereoscopic base of photographs is obtained by dividing the air base in metres by the mean scale of the photograph
The difference between the absolute parallax of two points depends upon the difference in their elevations
The line joining the principal point of a photograph and the transferred principal point of the adjoining photograph, is called stereoscopic base
All the above
h tan α/S
h tan β/S
h (tan α + tan β)/S
h (tan α - tan β)/S
Opposite corners of a photograph
Nodal points of the camera lens
Corresponding points on the ground and photograph
Plumb points of stereo pair of photographs
At east elongation
At upper culmination
At west elongation
At lower culmination
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
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
Declination must be 0°
Declination must be 90°
Distance from the pole must be less than the latitude of the observer
Hour angle must be 180°
50 %
60 %
70 %
75 %
Westward from the first point of Libra
Eastward from the first point of Aeries
Westward from the first point of Aeries
Eastward from the first point of Libra