1 minute of latitude
1 minute of longitude
1 degree of latitude
1 degree of longitude
B. 1 minute of longitude
Increases as the horizontal distance increases from the principal point
Increases as the ground elevation increases
Decreases as the flying height increases
All the above
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
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
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
Lengths
Angles
Heights
All of these
58 cot α
58 tan α
58 sin α
58 cos α
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
Once
Twice
Thrice
Four times
Co-declination
Co-latitude
Declination
Latitude
λ = α
λ = 90° - α
λ = α - 90°
λ = 180° - α
22° 30'
23° 27'
23° 30'
24° 0'
Optical projection
Optical mechanism projection
Mechanical projection
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
Northward
Southward
From south to north of the equator
From north to south of the equator
0.1 mm
0.5 mm
1.00 mm
1.1 mm
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
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
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
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
180° eastward
180° westward
180° east or westward
360° eastward
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
Swing
Tilt
Tip
None of these
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
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
7 h 00 m
7 h 30 m
8 h 00 m
9 h 00 m
f tan θ
f sin θ
f cot θ
f cos θ
Focal length of the camera
Overall size of the photo graphs
Percentage of overlap
All the above
High oblique
Low oblique
Vertical
None of these
8,000 m
10,000 m
12,000 m
14,000 m