The sum of the angles around a station should be 360°
The sum of the three angles of a plane triangle should be 180°
The sum of the eight angles of a braced quadrilateral should be 360°
All the above
D. All the above
Reduction to mean sea level
Correction for horizontal alignment
Correction for slope
All the above
Nadir
Isocenter
Principal point
Plumb point
The star's movement is apparent due to the actual steady rotation of the earth about its axis
The stars move round in circular concentrated parts
The centre of the circular paths of stars is the celestial pole
All the above
22° 30'
23° 27'
23° 30'
24° 0'
Horizon and equator
Equator and zenith
Zenith and pole
Pole and horizon
Eastward
Westward
Northward
Southward
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
500 m
1000 m
1500 m
2000 m
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
sin α = sin φ cosec δ
sin α = sin φ sec δ
sin α = cos φ sec δ
sin α = cos φ cosec δ
May have tilt up to 30°
May include the image of the horizon
May not include the image of the horizon
None of these
10°
20°
30°
40°
Correction for refraction is always negative
Correction for parallax is always positive
Correction for semi-diameter is always negative
Correction for dip is always negative
Rotate round the North Pole
Rotate round the celestial pole
Remain always above the horizon
Are seldom seen near the pole star
Horizon and equator
Zenith and pole
Equator and zenith
Pole and horizon
58 cot α
58 tan α
58 sin α
58 cos α
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
29 days
29.35 days
29.53 days
30 days
Eastward
Westward
Northward
Southward
Astronomical latitude
Astronomical longitude
Astronomical bearing
All of these
Lengths
Angles
Heights
All of these
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
Photo principal point and ground principal point
Photo isocenter and ground isocenter
Photo plumb point and ground plumb point
All the above
Eastward
Westward
Northward
Southward
Two angle equations and two side equations
One angle equation and three side equations
Three angle equations and one side equation
None of these
1°
2°
3°
4°
The principal point coincides with plumb point on a true vertical photograph
The top of a hill appears on a truly vertical photograph at greater distance than its bottom from the principal point
The top of a hill is represented on a vertical photograph at larger scale than the area of a nearby valley
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
πR²E/90°
πR²E/180°
πR²E/270°
πR²E/360°