Nadir
Isocenter
Principal point
Plumb point
C. Principal point
When the star momentarily moves vertically
When the angle at the star of the spherical triangle is 90°
When the star's declination is greater than the observer's latitude
All the above
180° eastward
180° westward
180° east or westward
360° eastward
Eastward
Westward
Northward
Southward
52 m
62 m
72 m
82 m
The principal point coincides with plumb point on a true vertical photograph
The top of a hill appears on a truly vertical photograph at greater distance than its bottom from the principal point
The top of a hill is represented on a vertical photograph at larger scale than the area of a nearby valley
All the above
Parallax
Height
Parallax difference
Height difference
30°
35°
40°
45°
1/3
1/2
3/4
5/4
Refraction correction is zero when the celestial body is in the zenith
Refraction correction is 33' when the celestial body is on the horizon
Refraction correction of celestial bodies depends upon their altitudes
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
North pole
Pole star
Celestial pole
All the above
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
22° 30'
23° 27'
23° 30'
24° 0'
Swing
Tilt
Tip
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°
f2
2f2
3f2
½f
Zenith
Celestial point
Nadir
Pole
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
δ - θ
θ - δ
θ + δ
(θ + δ)/2
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
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
365
365.2224
365.2422
366.2422
Satellite station
Subsidiary station
Pivot station
Main station
B = bH/f
B =f/bH
B = b/fH
B = H/bf
Mean sun
True sun
Vernal equinox
All the above
1°
2°
3°
4°
The horizontal direction of the pole is called astronomical north
The angle between the direction of true north and the direction of a survey line is called astronomical bearing
The astronomical bearing is generally called azimuth
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°
Isocenter
Principal point
Perspective centre
Plumb line
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