Ground elevation
Flying height
Length of air base
All the above
D. All the above
58 cot α
58 tan α
58 sin α
58 cos α
Reduction to mean sea level
Correction for horizontal alignment
Correction for slope
All the above
Photo plumb point
Plumb point
Nadir point
Isocenter
Principal point
Isocenter
Plumb point
Perspective centre
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
All the above
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
4.4 mm
5.5 mm
6.5 mm
7.5 mm
0.1 mm
0.5 mm
1.00 mm
1.1 mm
East of observer
West of observer
North of observer
South of observer
λ = α
λ = 90° - α
λ = α - 90°
λ = 180° - α
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
March 21
June 21
September 21
December 22
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
Geodetic triangulation of greatest possible sides and accuracy is carried out
Primary triangles are broken down into secondary triangles of somewhat lesser accuracy
Secondary triangles are further broken into third and fourth order triangles, the points of which are used for detail surveys
All the above
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
High oblique
Low oblique
Vertical
None of these
The sum of the angles around a station should be 360°
The sum of the three angles of a plane triangle should be 180°
The sum of the eight angles of a braced quadrilateral should be 360°
All the above
Eastward
Westward
Northward
Southward
2 mm
4 mm
6 mm
10 mm
Parallel projection
Orthogonal projection
Central projection
None of these
Plane surveying
Geodetic surveying
Star observations
Planet observations
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
Optical projection
Optical mechanism projection
Mechanical projection
All the above
Parallel lines do not appear parallel in central projection
The two sides of a road meet at the vanishing point
The lines parallel to the negative plane are projected as parallel lines
All the above
Every angle is less than two right angles
Sum of the three angles is equal to two right angles
Sum of the three angles less than six right angles and greater than two right angles
Sum of any two sides is greater than the third
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
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
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
Tension = (P - Ps)L/AE
Sag = L3w²/24P² where w is the weight of tape/m
Slope = (h²/2L) + (h4/8L3) where h is height difference of end supports
All the above
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