Co-declination
Co-latitude
Declination
Latitude
A. Co-declination
Isocenter
Principal point
Perspective centre
Plumb line
In truly vertical photographs without relief angles are true at the plumb point
In tilted photographs without relief, angles are true at the iso-centre
In tilled photographs with relief, angles are true at the principal point
None of these
Isocenter
Plumb point
Principal point
None of these
Rational horizon
True horizon
Celestial horizon
All the above
10° N
50° N Latitude
Equator
5° S latitude
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
Its altitude and azimuth
Its declination and hour angle
Its declination and right ascension
All the above
One less than mean solar days
One more than mean solar days
Equal to mean solar days
None of these
Principal point coincides the isocenter
Iso-centre coincides the plumb point
Plumb point coincides the principal point
All the above
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
One minute arc of the great circle passing through two points
One minute arc of the longitude
1855.109 m
All the above
Apparent solar time is measured from the lower transit of the true sun
Mean solar time is measured from the lower transit of the mean sun
Sidereal time is measured from the lower transit of the first point of Aries
Sidereal time is measured from the upper transit of the first point of Aries
Principal point
Isocenter
Plumb point
Perspective centre
The east point of the horizon
The west point of the horizon
The zenith point of the observer
All the above
Vernal equinox
Autumnal equinox
Summer solstice
Winter solstice
80°
70°
60°
40°
Control points for surveys of large areas
Control points for photogrammetric surveys
Engineering works, i.e. terminal points of long tunnels, bridge abutments, etc.
All the above
h tan α/S
h tan β/S
h (tan α + tan β)/S
h (tan α - tan β)/S
Is the period of time taken by the earth in making a complete rotation with reference to stars
Is slightly shorter than an ordinary solar day
Is divided into the conventional hours, minutes and seconds
All the above
58 cot α
58 tan α
58 sin α
58 cos α
Hour angle
Azimuth
Right ascension
Declination
500 m
1000 m
1500 m
2000 m
4000 m
5000 m
6000 m
7000 m
Rotate round the North Pole
Rotate round the celestial pole
Remain always above the horizon
Are seldom seen near the pole star
1 : 10,000
1 : 15,000
1 : 20,000
1 : 30,000
24 %
36 %
40 %
60 %
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
Greater than the longitude of the place
Less than the latitude of the place
Equal to the latitude of the place
None of these
Do not follow any definite mathematical law
Cannot be removed by applying corrections to the observed values
Are generally small
All the above
1/3
1/2
3/4
5/4