Sidereal time
Apparent solar time
Mean solar time
All the above
D. All the above
The sun's right ascension increases for 0 h to 24 h when it returns to the First point of Aries
The maximum declination of the sun increases up to 23 ½° N on about 21st June
The minimum declination of the sun is zero' on 22nd September
All the above
1 minute of latitude
1 minute of longitude
1 degree of latitude
1 degree of longitude
Declination
Altitude
Zenith distance
Co-latitude
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
Ground elevation
Flying height
Length of air base
All the above
cos δ/cos λ
cos (90° - δ)/cos (90° - λ)
sin (90° - δ)/sin (90° - λ)
tan (90° + δ)/tan (90° + λ)
Nadir point
Iso centre
Principal point
All the above
λ = α
λ = 90° - α
λ = α - 90°
λ = 180° - α
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
Plane surveying
Geodetic surveying
Star observations
Planet observations
Standard meridian
Greenwich meridian
Equator
180° longitude
δ - θ
θ - δ
θ + δ
½ (θ - δ)
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
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
Co-declination
Co-altitude
Co-latitude
Polar distance
Co-declination
Co-latitude
Declination
Latitude
L.M.T. - East longitude in time
L.M.T. + East longitude in time
L.M.T. - West longitude in time
None of these
Satellite station
Eccentric station
False station
Pivot station
4000 m
5000 m
6000 m
7000 m
B = bH/f
B =f/bH
B = b/fH
B = H/bf
Rotate round the North Pole
Rotate round the celestial pole
Remain always above the horizon
Are seldom seen near the pole star
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
Photo plumb point
Plumb point
Nadir point
Isocenter
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°
Rational horizon
True horizon
Celestial horizon
All the above
22° 30'
23° 27'
23° 30'
24° 0'
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
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
sin α = sin φ cosec δ
sin α = sin φ sec δ
sin α = cos φ sec δ
sin α = cos φ cosec δ