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
1600
1615
1630
1650
By subtracting their longitudes if places are in the same hemisphere
By adding their longitudes if places are in the different hemispheres
By subtracting the sum of their longitudes exceeding 180° from 360° if places are in different hemispheres
All the above
2 mm
4 mm
6 mm
10 mm
fB/(H - h)
fB/(H - h)2
fB/(H + h)
fB/(H + h)2
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
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
Isocenter
Principal point
Perspective centre
Plumb line
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
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°
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
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
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
High oblique
Low oblique
Vertical
None of these
Eastward
Westward
Northward
Southward
Correction for refraction is always negative
Correction for parallax is always positive
Correction for semi-diameter is always negative
Correction for dip is always negative
4000 m
5000 m
6000 m
7000 m
Equator
Celestial equator
Ecliptic
None of these
Horizon and equator
Zenith and pole
Equator and zenith
Pole and horizon
Equator
Horizon
Pole
None of these
Do not follow any definite mathematical law
Cannot be removed by applying corrections to the observed values
Are generally small
All the above
Base line of the left photograph of stereo pair
Base line of the right photograph of stereo pair
Sum of the base lines of stereo pair
Mean of the base lines of the stereo pair
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
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°
Photo principal point
Ground principal point
Ground isocenter
All the above
North end of the polar axis is known as North Pole
South end of the polar axis is known as South Pole
Point where polar axis when produced northward intersects the celestial sphere, is known as north celestial pole
All the above
March 21
June 21
September 21
December 22
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