f tan θ
f sin θ
f cot θ
f cos θ
A. f tan θ
Length of the equator between their longitudes
Length of the parallel between their longitudes
Length of the arc of the great circle passing through them
None of these
Photo principal point and ground principal point
Photo isocenter and ground isocenter
Photo plumb point and ground plumb point
All the above
L.M.T. - East longitude in time
L.M.T. + East longitude in time
L.M.T. - West longitude in time
None of these
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
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
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
Two angle equations and two side equations
One angle equation and three side equations
Three angle equations and one side equation
None of these
80°
70°
60°
50°
Tangents of two adjacent parts
Sines of two adjacent parts
Cosines of two adjacent parts
Both (a) and (b) above
1 cm
2 cm
3 cm
4 cm
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
Declination must be 0°
Declination must be 90°
Distance from the pole must be less than the latitude of the observer
Hour angle must be 180°
50 %
60 %
70 %
75 %
f2
2f2
3f2
½f
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
Increases as the horizontal distance increases from the principal point
Increases as the ground elevation increases
Decreases as the flying height increases
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
Is the point in the celestial sphere where zero meridian crosses the celestial equator
Is usually denoted by the Greek letter γ
Is located near the very conspicuous rectangle of stars in the constellations of Pegasus and Andromeda
All the above
2 mm
4 mm
6 mm
10 mm
Nadir point
Iso centre
Principal point
All the above
Photo principal point
Ground principal point
Ground isocenter
All the above
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
1600
1615
1630
1650
f tan θ
f sin θ
f cot θ
f cos θ
58 cot α
58 tan α
58 sin α
58 cos α
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
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
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
365
365.2224
365.2422
366.2422