Parallel projection
Orthogonal projection
Central projection
None of these
C. Central projection
180° eastward
180° westward
180° east or westward
360° eastward
Isocenter
Principal point
Perspective centre
Plumb line
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
March 21 to June 21
June 21 to September 21
September 21 to December 21
Both (a) and (b) of above
Parallel projection
Orthogonal projection
Central projection
None of these
500 m
1000 m
1500 m
2000 m
f sin θ
f cos θ
f tan θ
f sec θ
Declination
Altitude
Zenith distance
Co-latitude
Always follow some definite mathematical law
Can be removed by applying corrections to the observed values
Are also known as cumulative errors
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
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
Ground elevation
Flying height
Length of air base
All the above
f tan θ
f sin θ
f cot θ
f cos θ
Principal point coincides the isocenter
Iso-centre coincides the plumb point
Plumb point coincides the principal point
All the above
When its altitude is maximum
When its azimuth is 180°
When it is in south
All the above
Is a good property
Is a function of tilt
Is not affected by the change of flying height between photographs
Is minimum when θ is 3°
Zenith
Celestial point
Nadir
Pole
Latitudes north of the equator are taken as positive
Latitudes south of the equator are taken as negative
Longitudes east of Greenwich are taken as negative
Longitudes west of Greenwich are taken as positive
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
50 %
60 %
70 %
75 %
1000 km
800 km
600 km
500 km
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
30°
35°
40°
45°
Eastward
Westward
Northward
Southward
March 21
June 21
September 21
December 22
Eastward
Westward
Northward
Southward
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
4000 m
5000 m
6000 m
7000 m
Parallel projection
Orthogonal projection
Central projection
None of these
θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°