Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
C. Equal to the latitude of the place
24 %
36 %
40 %
60 %
Reduction to mean sea level
Correction for horizontal alignment
Correction for slope
All the above
Zenith
Celestial point
Nadir
Pole
h/H f tan θ
h/H f² tan θ
h/H f² sin θ
h/H f cos θ
Photo principal point and ground principal point
Photo isocenter and ground isocenter
Photo plumb point and ground plumb point
All the above
North pole
Pole star
Celestial pole
All the above
f/H
f/(H + h)
f/(H - h)
(H - h)/f
B = bH/f
B =f/bH
B = b/fH
B = H/bf
Nadir
Isocenter
Principal point
Plumb point
8,000 m
10,000 m
12,000 m
14,000 m
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
1600
1615
1630
1650
f2
2f2
3f2
½f
Gauss' Mid Latitude formula
D'Alembert's method
Legendre's method
Least square method
Is prepared, by graphical method
Is suitable for large areas with less control
Is rapid and accurate
All the above
Every angle is less than two right angles
Sum of the three angles is equal to two right angles
Sum of the three angles less than six right angles and greater than two right angles
Sum of any two sides is greater than the third
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
Eastward
Westward
Northward
Southward
Parallax
Height
Parallax difference
Height difference
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
Ground principal point
Ground plumb point
Iso-centre
Perspective centre
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
Astronomical latitude
Astronomical co-latitude
Co-declination of star
Declination of star
East of observer
West of observer
North of observer
South of observer
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
Normal to base line
Parallel to base line
Both (a) and (b)
Neither (a) nor (b)
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
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
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
Plane surveying
Geodetic surveying
Star observations
Planet observations