Opposite corners of a photograph
Nodal points of the camera lens
Corresponding points on the ground and photograph
Plumb points of stereo pair of photographs
C. Corresponding points on the ground and photograph
1 cm
2 cm
3 cm
4 cm
Reduction to mean sea level
Correction for horizontal alignment
Correction for slope
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
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 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
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
i = v. t. H/f
i = v. f/t. H
i = v. t. (f/H)
i = t. H/v. f
At culmination
At elongation
Neither at culmination nor at elongation
Either at culmination or at elongation
Isocenter
Principal point
Perspective centre
Plumb line
When its altitude is maximum
When its azimuth is 180°
When it is in south
All the above
30°
35°
40°
45°
Astronomical latitude
Astronomical co-latitude
Co-declination of star
Declination of star
Tangents of two adjacent parts
Sines of two adjacent parts
Cosines of two adjacent parts
Both (a) and (b) above
At east elongation
At upper culmination
At west elongation
At lower culmination
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
80°
70°
60°
50°
March 21
June 21
September 21
December 22
Its altitude and azimuth
Its declination and hour angle
Its declination and right ascension
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
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
Centre of the celestial sphere is taken as the position of the observer
Centre of the celestial sphere is taken as the centre of the earth
Stars move and maintain their relative positions
All the above
4.4 mm
5.5 mm
6.5 mm
7.5 mm
Rational horizon
True horizon
Celestial horizon
All the above
Once
Twice
Thrice
Four times
First point of Aeries
First point of Libra
Vernal Equinox
Both (b) and (d) of the above
Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
Co-declination
Co-altitude
Co-latitude
Polar distance
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
Nadir
Isocenter
Principal point
Plumb point
Standard meridian
Greenwich meridian
Equator
180° longitude