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4

The station pointer is generally used in

A. Triangulation surveying

B. Astronomical surveying

C. Hydrographical surveying

D. Photogrammetric surveying

Correct Answer :

C. Hydrographical surveying


Related Questions

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4

The declination and right ascension of the sun becomes 23° 27' N and 90° respectively on

A. March 21

B. June 21

C. September 21

D. December 22

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4

Pick up the incorrect statement from the following:

A. Latitudes north of the equator are taken as positive

B. Latitudes south of the equator are taken as negative

C. Longitudes east of Greenwich are taken as negative

D. Longitudes west of Greenwich are taken as positive

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4

In field astronomy, the quantities observed are entirely

A. Lengths

B. Angles

C. Heights

D. All of these

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4

The angle between the observer's meridian and declination circle of a heavenly body, is known as

A. Hour angle

B. Azimuth

C. Right ascension

D. Declination

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4

Polaris is usually observed for the determination of the azimuth when it is

A. At culmination

B. At elongation

C. Neither at culmination nor at elongation

D. Either at culmination or at elongation

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4

The value of geo-centric parallax to be added to the observed altitude of sun is

A. 9 cos α

B. 9 sin α

C. 9 tan α

D. 9 cot α

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4

If the image of a triangulation station of R.L. 500 m is 4 cm from the principal point of a vertical photo taken from an altitude of 2000 m, above datum, the height displacement will be

A. 2 mm

B. 4 mm

C. 6 mm

D. 10 mm

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4

The negative sign is assigned to

A. Reduction to mean sea level

B. Correction for horizontal alignment

C. Correction for slope

D. All the above

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4

The net ground area of a vertical photograph 20 cm × 20 cm on scale 1 : 10,000 having overlaps 60% and 30%, is

A. 0.50 sq km

B. 0.56 sq km

C. 0.60 sq km

D. 0.64 sq km

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4

The nearest star is so far away from the earth that the directions to it from two diametrically opposite points on the earth differs less than

A. 0.01 second

B. 0.001 second

C. 0.0001 second

D. None of these

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4

Longitudes are measured from 0° to

A. 180° eastward

B. 180° westward

C. 180° east or westward

D. 360° eastward

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4

The nautical mile is the length of

A. 1 minute of latitude

B. 1 minute of longitude

C. 1 degree of latitude

D. 1 degree of longitude

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4

The difference in longitude of two places expressed in time is equal to the difference in their

A. Sidereal time

B. Apparent solar time

C. Mean solar time

D. All the above

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4

The coverage is least if photography is

A. High oblique

B. Low oblique

C. Vertical

D. None of these

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4

The meridian of a place is

A. A great circle passing through the place and the poles

B. A great circle whose plane is perpendicular to the axis of rotation and it also passes through the place

C. A semi-circle which passes through the place and is terminated at the poles

D. An arc of the great circle which passes through the place and is perpendicular to the equator

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4

The hour angle of the heavenly body for Greenwich meridian equals the hour angle of the body for any other meridian + longitude:

A. Mean sun

B. True sun

C. Vernal equinox

D. All the above

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4

In a spherical triangle ABC, right angled at C, sin b equals

A. sin a cos A

B. cos a sin A

C. tan a cot A

D. cot A tan a

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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

D. All the above

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4

Latitude of the observer's position is equal to altitude of

A. North pole

B. Pole star

C. Celestial pole

D. All the above

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4

H is the flying height above mean ground level and f is the principal distance of a vertical photograph. The mean scale of the photographs is

A. H. f

B. H/f

C. f/H

D. H + f

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4

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

A. Principal point

B. Isocenter

C. Plumb point

D. Perspective centre

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4

The want of correspondence in stereo-photographs

A. Is a good property

B. Is a function of tilt

C. Is not affected by the change of flying height between photographs

D. Is minimum when θ is 3°

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4

Longitude of a place is the angular distance between the meridian of the place and

A. The standard meridian

B. The international date line

C. That of Greenwich

D. Both (a) and (c) of above

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4

The position of a heavenly body on the celestial sphere can be completely specified by

A. Its altitude and azimuth

B. Its declination and hour angle

C. Its declination and right ascension

D. All the above

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4

For mapping any country

A. Geodetic triangulation of greatest possible sides and accuracy is carried out

B. Primary triangles are broken down into secondary triangles of somewhat lesser accuracy

C. Secondary triangles are further broken into third and fourth order triangles, the points of which are used for detail surveys

D. All the above

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4

At lower culmination, the pole star moves

A. Eastward

B. Westward

C. Northward

D. Southward

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4

Parallax bar measures

A. Parallax

B. Height

C. Parallax difference

D. Height difference

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4

International Date Line is located along

A. Standard meridian

B. Greenwich meridian

C. Equator

D. 180° longitude

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4

The angular distance of a heavenly body from the equator, measured along its meridian, is called

A. Declination

B. Altitude

C. Zenith distance

D. Co-latitude

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4

At upper culmination, the pole star moves

A. Eastward

B. Westward

C. Northward

D. Southward