80°
70°
60°
40°
D. 40°
10 km
25 km
30 km
50 km
Planimetric control
Height control
Both planimetric and height control
None of these
1 cm
2 cm
3 cm
4 cm
Swing
Tilt
Tip
None of these
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
All the above
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
A great circle passing through the place and the poles
A great circle whose plane is perpendicular to the axis of rotation and it also passes through the place
A semi-circle which passes through the place and is terminated at the poles
An arc of the great circle which passes through the place and is perpendicular to the equator
The length of the air base is increased
The scale of the model is altered
y-parallax is not affected
All the above
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
f2
2f2
3f2
½f
2 mm
4 mm
6 mm
10 mm
High oblique
Low oblique
Vertical
None of these
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
500 m
1000 m
1500 m
2000 m
1°
2°
3°
4°
h tan α/S
h tan β/S
h (tan α + tan β)/S
h (tan α - tan β)/S
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
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
Sidereal time at any instant is equal to the hour angle of the first point of Aries
Local sidereal time of any place is equal to the right ascension of its meridian
Sidereal time is equal to the right ascension of a star at its upper transit
All the above
Once
Twice
Thrice
Four times
S - 90°
S - 180°
S - 270°
S - 360°
1 minute of latitude
1 minute of longitude
1 degree of latitude
1 degree of longitude
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
Eastward
Westward
Northward
Southward
sin c sin B
cos c cos B
tan c tan B
sin c cos B
Normal to base line
Parallel to base line
Both (a) and (b)
Neither (a) nor (b)
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
The sun's right ascension increases for 0 h to 24 h when it returns to the First point of Aries
The maximum declination of the sun increases up to 23 ½° N on about 21st June
The minimum declination of the sun is zero' on 22nd September
All the above
δ - θ
θ - δ
θ + δ
(θ + δ)/2