Principal distance
Principal line
Isocentric distance
Focal length
A. Principal distance
March 21
June 21
September 21
December 22
1°
2°
3°
4°
sin z = sec φ . cos δ
cos z = sec φ . cos δ
tan z = sec φ . cos δ
None of these
Base line of the left photograph of stereo pair
Base line of the right photograph of stereo pair
Sum of the base lines of stereo pair
Mean of the base lines of the stereo pair
Is a good property
Is a function of tilt
Is not affected by the change of flying height between photographs
Is minimum when θ is 3°
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
Normal to base line
Parallel to base line
Both (a) and (b)
Neither (a) nor (b)
Positive for points above datum
Negative for points below datum
Zero for points vertically below the air station
All the above
High oblique
Low oblique
Vertical
None of these
North pole
Pole star
Celestial pole
All the above
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
Photo principal point
Ground principal point
Ground isocenter
All the above
1/3
1/2
3/4
5/4
Mean sun
First point of Aries
First point of Libra
The polar star
Principal point
Isocenter
Plumb point
Perspective centre
Eastward
Westward
Northward
Southward
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
Plane surveying
Geodetic surveying
Star observations
Planet observations
f sin θ
f cos θ
f tan θ
f sec θ
4.4 mm
5.5 mm
6.5 mm
7.5 mm
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
Nadir point
Iso centre
Principal point
All the above
7 h 00 m
7 h 30 m
8 h 00 m
9 h 00 m
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
The angle between the plane of the negative and the horizontal plane containing perspective axis is the tilt of the photograph
The direction of maximum tilt is defined by the photo principal line
The principal plane is truly vertical plane which contains perspective centre as well as principal point and plumb point
All the above
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
sin λ
cos λ
tan λ
cot λ
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
πR²E/90°
πR²E/180°
πR²E/270°
πR²E/360°
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these