24 %
36 %
40 %
60 %
B. 36 %
10°
20°
30°
40°
50 %
60 %
70 %
75 %
Ground principal point
Ground plumb point
Iso-centre
Perspective centre
Lie on the parallel of the latitude
Are equidistant from the nearer pole
Are equidistant from both the poles
All the above
Optical projection
Optical mechanism projection
Mechanical projection
All the above
Altitude and azimuth system
Declination and hour angle system
Declination and right ascension system
Declination and altitude system
Parallax
Height
Parallax difference
Height difference
Astronomical latitude
Astronomical co-latitude
Co-declination of star
Declination of star
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
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
500 m
1000 m
1500 m
2000 m
Photo plumb point
Plumb point
Nadir point
Isocenter
The principal point coincides with plumb point on a true vertical photograph
The top of a hill appears on a truly vertical photograph at greater distance than its bottom from the principal point
The top of a hill is represented on a vertical photograph at larger scale than the area of a nearby valley
All the above
By subtracting their longitudes if places are in the same hemisphere
By adding their longitudes if places are in the different hemispheres
By subtracting the sum of their longitudes exceeding 180° from 360° if places are in different hemispheres
All the above
Greenwich to the place
Equator to the poles
Equator to the nearer pole
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
10 km
25 km
30 km
50 km
In truly vertical photographs without relief angles are true at the plumb point
In tilted photographs without relief, angles are true at the iso-centre
In tilled photographs with relief, angles are true at the principal point
None of these
Apparent solar time is measured from the lower transit of the true sun
Mean solar time is measured from the lower transit of the mean sun
Sidereal time is measured from the lower transit of the first point of Aries
Sidereal time is measured from the upper transit of the first point of Aries
Correction for refraction is always negative
Correction for parallax is always positive
Correction for semi-diameter is always negative
Correction for dip is always negative
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
S - 90°
S - 180°
S - 270°
S - 360°
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
Ground elevation
Flying height
Length of air base
All the above
Rational horizon
True horizon
Celestial horizon
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
λ = α
λ = 90° - α
λ = α - 90°
λ = 180° - α
h/H f tan θ
h/H f² tan θ
h/H f² sin θ
h/H f cos θ
North pole
Pole star
Celestial pole
All the above
Swing
Tilt
Tip
None of these