i = v. t. H/f
i = v. f/t. H
i = v. t. (f/H)
i = t. H/v. f
C. i = v. t. (f/H)
Centre of the celestial sphere is taken as the position of the observer
Centre of the celestial sphere is taken as the centre of the earth
Stars move and maintain their relative positions
All the above
Ground principal point
Ground plumb point
Iso-centre
Perspective centre
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
24 %
36 %
40 %
60 %
L.M.T. - East longitude in time
L.M.T. + East longitude in time
L.M.T. - West longitude in time
None of these
1°
2°
3°
4°
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
1 cm
2 cm
3 cm
4 cm
4000 m
5000 m
6000 m
7000 m
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
30°
35°
40°
45°
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
5100 nautical miles
5700 nautical miles
120 nautical miles
500 nautical miles
March 21 to June 21
June 21 to September 21
September 21 to December 21
Both (a) and (b) of above
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
Sidereal time
Apparent solar time
Mean solar time
All the above
When its altitude is maximum
When its azimuth is 180°
When it is in south
All the above
Eastward
Westward
Northward
Southward
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
80°
70°
60°
50°
Is prepared, by graphical method
Is suitable for large areas with less control
Is rapid and accurate
All the above
Sun and moon are in line with earth
Solar tidal force acts opposite to lunar tidal force
Solar tidal force and lunar tidal force both coincide
None of these
The star's movement is apparent due to the actual steady rotation of the earth about its axis
The stars move round in circular concentrated parts
The centre of the circular paths of stars is the celestial pole
All the above
58 cot α
58 tan α
58 sin α
58 cos α
10 km
25 km
30 km
50 km
7 h 00 m
7 h 30 m
8 h 00 m
9 h 00 m
Isocenter
Principal point
Perspective centre
Plumb line
f tan θ
f sin θ
f cot θ
f cos θ
f sin θ
f cos θ
f tan θ
f sec θ
Isocenter
Plumb point
Principal point
None of these