f/H
f/(H + h)
f/(H - h)
(H - h)/f
C. f/(H - h)
δ - θ
θ - δ
θ + δ
(θ + δ)/2
Parallax
Height
Parallax difference
Height difference
1/3
1/2
3/4
5/4
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
2 mm
4 mm
6 mm
10 mm
4000 m
5000 m
6000 m
7000 m
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
Horizon and equator
Zenith and pole
Equator and zenith
Pole and horizon
sin a cos A
cos a sin A
tan a cot A
cot A tan a
Declination
Altitude
Zenith distance
Co-latitude
πR²E/90°
πR²E/180°
πR²E/270°
πR²E/360°
Ground elevation
Flying height
Length of air base
All the above
sin c sin B
cos c cos B
tan c tan B
sin c cos B
The horizontal direction of the pole is called astronomical north
The angle between the direction of true north and the direction of a survey line is called astronomical bearing
The astronomical bearing is generally called azimuth
All the above
30°
35°
40°
45°
Optical projection
Optical mechanism projection
Mechanical projection
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
0.01 second
0.001 second
0.0001 second
None of these
Eastward
Westward
Northward
Southward
Eastward
Westward
Northward
Southward
Aerial photographs may be either vertical or oblique
Vertical photographs are taken with the axis of camera pointing vertically downward
Vertical photographs are used for most accurate maps
All the above
The measured stereoscopic base of photographs is obtained by dividing the air base in metres by the mean scale of the photograph
The difference between the absolute parallax of two points depends upon the difference in their elevations
The line joining the principal point of a photograph and the transferred principal point of the adjoining photograph, is called stereoscopic base
All the above
f2
2f2
3f2
½f
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
f/H sec θ
f sec θ/H
f/H
f/H cos ½θ
1°
2°
3°
4°
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
0.50 sq km
0.56 sq km
0.60 sq km
0.64 sq km
Nadir point
Iso centre
Principal point
All the above