Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
D. None of these
sin a cos A
cos a sin A
tan a cot A
cot A tan a
πR²E/90°
πR²E/180°
πR²E/270°
πR²E/360°
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
Principal point
Isocenter
Plumb point
Perspective centre
4000 m
5000 m
6000 m
7000 m
Its altitude and azimuth
Its declination and hour angle
Its declination and right ascension
All the above
Isocenter
Principal point
Perspective centre
Plumb line
Mean sun
True sun
Vernal equinox
All the above
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
1/3
1/2
3/4
5/4
30°
35°
40°
45°
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
At east elongation
At upper culmination
At west elongation
At lower culmination
1 in 12
1 in 10
1 in 8
1 in 6
Planimetric control
Height control
Both planimetric and height control
None of these
Altitude and azimuth system
Declination and hour angle system
Declination and right ascension system
Declination and altitude system
i = v. t. H/f
i = v. f/t. H
i = v. t. (f/H)
i = t. H/v. f
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
0.01 second
0.001 second
0.0001 second
None of these
Standard meridian
Greenwich meridian
Equator
180° longitude
sin α = sin φ cosec δ
sin α = sin φ sec δ
sin α = cos φ sec δ
sin α = cos φ cosec δ
1600
1615
1630
1650
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
Nadir point
Iso centre
Principal point
All the above
58 mm
60 mm
62 mm
64 mm
Aerial photographs may be either vertical or oblique
Vertical photographs are taken with the axis of camera pointing vertically downward
Vertical photographs are used for most accurate maps
All the above
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
Rotate round the North Pole
Rotate round the celestial pole
Remain always above the horizon
Are seldom seen near the pole star
365
365.2224
365.2422
366.2422