Visible horizon
Sensible horizon
Celestial horizon
True horizon
B. Sensible horizon
Parallel projection
Orthogonal projection
Central projection
None of these
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 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
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
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
1 m
2 m
4 m
8 m
Co-declination
Co-latitude
Declination
Latitude
Is the period of time taken by the earth in making a complete rotation with reference to stars
Is slightly shorter than an ordinary solar day
Is divided into the conventional hours, minutes and seconds
All the above
Optical projection
Optical mechanism projection
Mechanical projection
All the above
f2
2f2
3f2
½f
Visible horizon
Sensible horizon
Celestial horizon
True horizon
1600
1615
1630
1650
Aerial photographs may be either vertical or oblique
Vertical photographs are taken with the axis of camera pointing vertically downward
Vertical photographs are used for most accurate maps
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
52 m
62 m
72 m
82 m
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
50 %
60 %
70 %
75 %
Nadir
Isocenter
Perspective centre
None of these
Satellite station
Subsidiary station
Pivot station
Main station
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
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
10° N
50° N Latitude
Equator
5° S latitude
Mean sun
First point of Aries
First point of Libra
The polar star
9 cos α
9 sin α
9 tan α
9 cot α
7 h 00 m
7 h 30 m
8 h 00 m
9 h 00 m
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
Northward
Southward
From south to north of the equator
From north to south of the equator
h/H f tan θ
h/H f² tan θ
h/H f² sin θ
h/H f cos θ
365
365.2224
365.2422
366.2422
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