Always follow some definite mathematical law
Can be removed by applying corrections to the observed values
Are also known as cumulative errors
All the above
D. All the above
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
f sin θ
f cos θ
f tan θ
f sec θ
4000 m
5000 m
6000 m
7000 m
Satellite station
Eccentric station
False station
Pivot station
Isocenter
Principal point
Perspective centre
Plumb line
Equator
Horizon
Pole
None of these
North pole
Pole star
Celestial pole
All the above
Geodetic triangulation of greatest possible sides and accuracy is carried out
Primary triangles are broken down into secondary triangles of somewhat lesser accuracy
Secondary triangles are further broken into third and fourth order triangles, the points of which are used for detail surveys
All the above
In truly vertical photographs without relief angles are true at the plumb point
In tilted photographs without relief, angles are true at the iso-centre
In tilled photographs with relief, angles are true at the principal point
None of these
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
April 15
June 14
September 1
All the above
58 mm
60 mm
62 mm
64 mm
Astronomical latitude
Astronomical longitude
Astronomical bearing
All of these
Gauss' Mid Latitude formula
D'Alembert's method
Legendre's method
Least square method
1000 km
800 km
600 km
500 km
Horizon and equator
Zenith and pole
Equator and zenith
Pole and horizon
δ - θ
θ - δ
θ + δ
½ (θ - δ)
Mean sun
True sun
Vernal equinox
All the above
Co-declination
Co-latitude
Declination
Latitude
Parallax
Height
Parallax difference
Height difference
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
Is a good property
Is a function of tilt
Is not affected by the change of flying height between photographs
Is minimum when θ is 3°
Principal point
Isocenter
Plumb point
Perspective centre
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
1°
2°
3°
4°
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
180° eastward
180° westward
180° east or westward
360° eastward
θ = z + δ
θ = δ - z
θ = 180° - (z + δ)
θ = (z + δ) - 180°
58 cot α
58 tan α
58 sin α
58 cos α