High oblique
Low oblique
Vertical
None of these
A. High oblique
fB/(H - h)
fB/(H - h)2
fB/(H + h)
fB/(H + h)2
Gauss' Mid Latitude formula
D'Alembert's method
Legendre's method
Least square method
Eastward
Westward
Northward
Southward
Altitude and azimuth system
Declination and hour angle system
Declination and right ascension system
Declination and altitude system
1 cm
2 cm
3 cm
4 cm
Northward
Southward
From south to north of the equator
From north to south of the equator
The direction of the vertical, the axis of rotation of the instrument
The direction of the poles of the celestial sphere
The direction of the star from the instrument
All the above
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
If the applied tension to the tape is more than the standard, the tension correction is positive
If the applied tension to the tape is less than the standard, the tension correction is negative
If the temperature during measurement is greater than the standard temperature, the temperature correction is positive
All the above
Visible horizon
Sensible horizon
Celestial horizon
True horizon
Lengths
Angles
Heights
All of these
Equator
Horizon
Pole
None of these
Photo principal point
Ground principal point
Ground isocenter
All the above
80°
70°
60°
50°
H. f
H/f
f/H
H + f
Elevation of the elevated pole
Declination of the observer's zenith
Angular distance along the observer's meridian between equator and the observer
All the above
Apparent solar time is measured from the lower transit of the true sun
Mean solar time is measured from the lower transit of the mean sun
Sidereal time is measured from the lower transit of the first point of Aries
Sidereal time is measured from the upper transit of the first point of Aries
Rotate round the North Pole
Rotate round the celestial pole
Remain always above the horizon
Are seldom seen near the pole star
Mean sun
True sun
Vernal equinox
All the above
cos H = tan λ/tan δ
sin α = sin λ/sin δ
sin A = cos δ/cos λ
All the above
Control points for surveys of large areas
Control points for photogrammetric surveys
Engineering works, i.e. terminal points of long tunnels, bridge abutments, etc.
All the above
2 mm
4 mm
6 mm
10 mm
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
At east elongation
At upper culmination
At west elongation
At lower culmination
1/3
1/2
3/4
5/4
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
North end of the polar axis is known as North Pole
South end of the polar axis is known as South Pole
Point where polar axis when produced northward intersects the celestial sphere, is known as north celestial pole
All the above
Ground principal point
Ground plumb point
Iso-centre
Perspective centre
Isocenter
Plumb point
Principal point
None of these