High oblique
Low oblique
Vertical
None of these
C. Vertical
sin λ
cos λ
tan λ
cot λ
Eastward
Westward
Northward
Southward
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
i = v. t. H/f
i = v. f/t. H
i = v. t. (f/H)
i = t. H/v. f
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
Parallel to the principal line
Perpendicular to the principal line
Along the bisector of the angle between the principal line and a perpendicular line through principal plane
None of these
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
Once
Twice
Thrice
Four times
Co-declination
Co-altitude
Co-latitude
Polar distance
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
Parallel projection
Orthogonal projection
Central projection
None of these
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
1 minute of latitude
1 minute of longitude
1 degree of latitude
1 degree of longitude
h tan α/S
h tan β/S
h (tan α + tan β)/S
h (tan α - tan β)/S
1 m
2 m
4 m
8 m
58 mm
60 mm
62 mm
64 mm
Photo principal point
Ground principal point
Ground isocenter
All the above
The standard meridian
The international date line
That of Greenwich
Both (a) and (c) of above
Control points for surveys of large areas
Control points for photogrammetric surveys
Engineering works, i.e. terminal points of long tunnels, bridge abutments, etc.
All the above
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
March 21
June 21
September 21
December 22
h/H f tan θ
h/H f² tan θ
h/H f² sin θ
h/H f cos θ
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
sin c sin B
cos c cos B
tan c tan B
sin c cos B
f2
2f2
3f2
½f
March 21 to June 21
June 21 to September 21
September 21 to December 21
Both (a) and (b) of above
Do not follow any definite mathematical law
Cannot be removed by applying corrections to the observed values
Are generally small
All the above
At east elongation
At upper culmination
At west elongation
At lower culmination
Elevation of the elevated pole
Declination of the observer's zenith
Angular distance along the observer's meridian between equator and the observer
All the above