1 m
2 m
4 m
8 m
A. 1 m
High oblique
Low oblique
Vertical
None of these
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
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
Altitude and azimuth system
Declination and hour angle system
Declination and right ascension system
Declination and altitude system
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
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
24 hours 10 minutes
20 hours 25 minutes
24 hours 50 minutes
23 hours 50 minutes
Tangents of two adjacent parts
Sines of two adjacent parts
Cosines of two adjacent parts
Both (a) and (b) above
1 minute of latitude
1 minute of longitude
1 degree of latitude
1 degree of longitude
The vertical plane containing the zenith, the station of observation and the celestial pole is the observer's meridian plane
The angle between the direction of star in vertical plane and the direction of the star in horizontal plane is called the altitude of the star
The complement of the altitude of star is called the zenith distance of the star
All the above
H. f
H/f
f/H
H + f
Astronomical latitude
Astronomical longitude
Astronomical bearing
All of these
1 in 12
1 in 10
1 in 8
1 in 6
At east elongation
At upper culmination
At west elongation
At lower culmination
Greenwich to the place
Equator to the poles
Equator to the nearer pole
None of these
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
sin c sin B
cos c cos B
tan c tan B
sin c cos B
Sidereal time
Apparent solar time
Mean solar time
All the above
S - 90°
S - 180°
S - 270°
S - 360°
Astronomical latitude
Astronomical co-latitude
Co-declination of star
Declination of star
A great circle passing through the place and the poles
A great circle whose plane is perpendicular to the axis of rotation and it also passes through the place
A semi-circle which passes through the place and is terminated at the poles
An arc of the great circle which passes through the place and is perpendicular to the equator
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
Eastward
Westward
Northward
Southward
4.4 mm
5.5 mm
6.5 mm
7.5 mm
Is prepared, by graphical method
Is suitable for large areas with less control
Is rapid and accurate
All the above
Co-declination
Co-altitude
Co-latitude
Polar distance
500 m
1000 m
1500 m
2000 m
Declination must be 0°
Declination must be 90°
Distance from the pole must be less than the latitude of the observer
Hour angle must be 180°
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
All the above
Declination
Altitude
Zenith distance
Co-latitude