Length of the equator between their longitudes
Length of the parallel between their longitudes
Length of the arc of the great circle passing through them
None of these
C. Length of the arc of the great circle passing through them
North pole
Pole star
Celestial pole
All the above
Tension = (P - Ps)L/AE
Sag = L3w²/24P² where w is the weight of tape/m
Slope = (h²/2L) + (h4/8L3) where h is height difference of end supports
All the above
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
Swing
Tilt
Tip
None of these
Principal point coincides the isocenter
Iso-centre coincides the plumb point
Plumb point coincides the principal point
All the above
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
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
Mean sun
True sun
Vernal equinox
All the above
The area is divided into triangular figures
Control stations are located from which detailed surveys are carried out
Sides are not measured excepting the base line
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
B = bH/f
B =f/bH
B = b/fH
B = H/bf
Is prepared, by graphical method
Is suitable for large areas with less control
Is rapid and accurate
All the above
By subtracting their longitudes if places are in the same hemisphere
By adding their longitudes if places are in the different hemispheres
By subtracting the sum of their longitudes exceeding 180° from 360° if places are in different hemispheres
All the above
Hour angle
Azimuth
Right ascension
Declination
Astronomical latitude
Astronomical longitude
Astronomical bearing
All of these
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
Gauss' Mid Latitude formula
D'Alembert's method
Legendre's method
Least square method
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
500 m
1000 m
1500 m
2000 m
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
10° N
50° N Latitude
Equator
5° S latitude
The standard meridian
The international date line
That of Greenwich
Both (a) and (c) of above
Parallel lines do not appear parallel in central projection
The two sides of a road meet at the vanishing point
The lines parallel to the negative plane are projected as parallel lines
All the above
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
4.4 mm
5.5 mm
6.5 mm
7.5 mm
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
Meridian
Vertical circle
Prime vertical
None of these
Observation equation
Conditional equation
Normal equation
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
Is the period of time taken by the earth in making a complete rotation with reference to stars
Is slightly shorter than an ordinary solar day
Is divided into the conventional hours, minutes and seconds
All the above