Related Questions
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The declination and right ascension of the sun becomes 23° 27' S and 270° respectively on
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The principal line is the line joining the principal point and
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4
The shortest distance between two places measured along the surface of the earth, is
A. Length of the equator between their longitudes
B. Length of the parallel between their longitudes
C. Length of the arc of the great circle passing through them
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4
For plane ground the scale of a vertical photograph will be same as that of a tiled photograph along the photo parallel through
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4
If f is the focal length of the camera lens and θ is the angle of tilt, the distance of the plumb point from the principal point will be
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If E is the spherical excess and R the radius of the earth, the surface area of the triangle, is
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Equation of time which is the difference between apparent solar time and mean solar time at any instant, vanishes during one year
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The latitude of a place was obtained by subtracting the declination of a star from its zenith distance, the observed star was between
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In a tropical year, the numbers of sidereal days are
A. One less than mean solar days
B. One more than mean solar days
C. Equal to mean solar days
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The correction for parallax, is
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Pick up the in-correct statement from the following:
A. Apparent solar time is measured from the lower transit of the true sun
B. Mean solar time is measured from the lower transit of the mean sun
C. Sidereal time is measured from the lower transit of the first point of Aries
D. Sidereal time is measured from the upper transit of the first point of Aries
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The flying height of the camera is 1, 000 m above mean ground level, the distance of the top of a building from a nadir point is 10 cm and the relief displacement of building is 7.2 mm. The height of the building, is
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The net ground area of a vertical photograph 20 cm × 20 cm on scale 1 : 10,000 having overlaps 60% and 30%, is
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4
Pick up the incorrect statement from the following:
A. In truly vertical photographs without relief angles are true at the plumb point
B. In tilted photographs without relief, angles are true at the iso-centre
C. In tilled photographs with relief, angles are true at the principal point
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4
The solar tidal force divided by lunar tidal force is
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The correction applied to the measured base of length L is
A. Tension = (P - Ps)L/AE
B. Sag = L3w²/24P² where w is the weight of tape/m
C. Slope = (h²/2L) + (h4/8L3) where h is height difference of end supports
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4
Pick up the correct statement for horizontal photographs.
A. Parallel lines do not appear parallel in central projection
B. The two sides of a road meet at the vanishing point
C. The lines parallel to the negative plane are projected as parallel lines
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Assuming human normal vision distance 25 cm, smallest measurable angle 20, and intraocular distance 6.5 cm, the smallest depth to be discerned is
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The normal longitudinal overlap is generally kept
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International Date Line is located along
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The principal plane contains
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The latitude (λ) of a place and the altitude (α) of the pole are related by
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A star is said to elongate
A. When the star momentarily moves vertically
B. When the angle at the star of the spherical triangle is 90°
C. When the star's declination is greater than the observer's latitude
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The equation which is obtained by multiplying each equation by the coefficient of its un-knowns and by adding the equations thus formed, is known as
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4
According to Napier's Rules of circular parts for a right angled triangle, sine of middle part equals the product of
A. Tangents of two adjacent parts
B. Sines of two adjacent parts
C. Cosines of two adjacent parts
D. Both (a) and (b) above
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The point on the photograph where bisector between the vertical line through optical centre of the camera lens and the plate perpendicular meets, is known as
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α and β are the angles subtended by a point of elevation h at their air station with respective plumb points. Photo scale and focal length of the lens being S and f respectively. Parallax displacement of the point due to relief, is
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The maximum error in radial line assumption, is
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If δ is the declination of the star and φ is the latitude of the observer then the hour angle of the star at elongation is given by
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The longitudes of two places at latitude 60° N are 93° E and 97° W. Their departure is