May have tilt up to 30°
May include the image of the horizon
May not include the image of the horizon
None of these
D. None of these
1°
2°
3°
4°
Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
1/3
1/2
3/4
5/4
Lie on the parallel of the latitude
Are equidistant from the nearer pole
Are equidistant from both the poles
All the above
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
Co-declination
Co-latitude
Declination
Latitude
The sun's right ascension increases for 0 h to 24 h when it returns to the First point of Aries
The maximum declination of the sun increases up to 23 ½° N on about 21st June
The minimum declination of the sun is zero' on 22nd September
All the above
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
h tan α/S
h tan β/S
h (tan α + tan β)/S
h (tan α - tan β)/S
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
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
365
365.2224
365.2422
366.2422
Mean sun
First point of Aries
First point of Libra
The polar star
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
Photo principal point and ground principal point
Photo isocenter and ground isocenter
Photo plumb point and ground plumb point
All the above
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
Co-declination
Co-altitude
Co-latitude
Polar distance
Is prepared, by graphical method
Is suitable for large areas with less control
Is rapid and accurate
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
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
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
1 m
2 m
4 m
8 m
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
2 mm
4 mm
6 mm
10 mm
Eastward
Westward
Northward
Southward
Is the point in the celestial sphere where zero meridian crosses the celestial equator
Is usually denoted by the Greek letter γ
Is located near the very conspicuous rectangle of stars in the constellations of Pegasus and Andromeda
All the above
f tan θ
f sin θ
f cot θ
f cos θ
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
Swing
Tilt
Tip
None of these
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