θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°
C. θ = 180° - (z + δ)
The area is divided into triangular figures
Control stations are located from which detailed surveys are carried out
Sides are not measured excepting the base line
All the above
Photo plumb point
Plumb point
Nadir point
Isocenter
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
Optical projection
Optical mechanism projection
Mechanical projection
All the above
10° N
50° N Latitude
Equator
5° S latitude
North pole
Pole star
Celestial pole
All the above
Standard meridian
Greenwich meridian
Equator
180° longitude
The standard meridian
The international date line
That of Greenwich
Both (a) and (c) of above
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
Reduction to mean sea level
Correction for horizontal alignment
Correction for slope
All the above
The angle between the plane of the negative and the horizontal plane containing perspective axis is the tilt of the photograph
The direction of maximum tilt is defined by the photo principal line
The principal plane is truly vertical plane which contains perspective centre as well as principal point and plumb point
All the above
Mean sun
True sun
Vernal equinox
All the above
Declination
Altitude
Zenith distance
Co-latitude
Nadir
Isocenter
Principal point
Plumb point
Parallax
Height
Parallax difference
Height difference
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
Satellite station
Eccentric station
False station
Pivot station
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
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
Normal to base line
Parallel to base line
Both (a) and (b)
Neither (a) nor (b)
Rational horizon
True horizon
Celestial horizon
All the above
f sin θ
f cos θ
f tan θ
f sec θ
1/3
1/2
3/4
5/4
Photo principal point
Ground principal point
Ground isocenter
All the above
1000 km
800 km
600 km
500 km
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
Equator
Horizon
Pole
None of these
High oblique
Low oblique
Vertical
None of these
Eastward
Westward
Northward
Southward
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