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
D. All the above
sin λ
cos λ
tan λ
cot λ
1000 km
800 km
600 km
500 km
Equator
Celestial equator
Ecliptic
None of these
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
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
365
365.2224
365.2422
366.2422
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
Nadir point
Iso centre
Principal point
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)
North pole
Pole star
Celestial pole
All the above
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
One degree of longitude has greatest value at the equator
One degree of longitude has greatest value at the poles
One degree of longitude has the same value everywhere
One degree of latitude decreases from the equator to the poles
Co-declination
Co-altitude
Co-latitude
Polar distance
L.M.T. - East longitude in time
L.M.T. + East longitude in time
L.M.T. - West longitude in time
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
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
sin a cos A
cos a sin A
tan a cot A
cot A tan a
180° eastward
180° westward
180° east or westward
360° eastward
Parallel to the principal line
Perpendicular to the principal line
Along the bisector of the angle between the principal line and a perpendicular line through principal plane
None of these
Lie on the parallel of the latitude
Are equidistant from the nearer pole
Are equidistant from both the poles
All the above
Co-declination
Co-latitude
Declination
Latitude
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
A great circle passing through the place and the poles
A great circle whose plane is perpendicular to the axis of rotation and it also passes through the place
A semi-circle which passes through the place and is terminated at the poles
An arc of the great circle which passes through the place and is perpendicular to the equator
Astronomical latitude
Astronomical co-latitude
Co-declination of star
Declination of star
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
Principal point coincides the isocenter
Iso-centre coincides the plumb point
Plumb point coincides the principal point
All the above
Once
Twice
Thrice
Four times
Satellite station
Eccentric station
False station
Pivot station
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