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4

The parallax equation Δp = BmΔh/H - h is applicable to entire overlap of the photographs only if parallax is measured

A. Normal to base line

B. Parallel to base line

C. Both (a) and (b)

D. Neither (a) nor (b)

Correct Answer :

B. Parallel to base line


Related Questions

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4

If a star whose declination is 60° N culminates at zenith, its altitude at the lower culmination, is

A. 10°

B. 20°

C. 30°

D. 40°

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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 incorrect statement from the following. In a spherical triangle

A. Every angle is less than two right angles

B. Sum of the three angles is equal to two right angles

C. Sum of the three angles less than six right angles and greater than two right angles

D. Sum of any two sides is greater than the third

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4

The Polaris remains below horizon at

A. 10° N

B. 50° N Latitude

C. Equator

D. 5° S latitude

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4

The distance between the minor control point and the principal point should be equal to

A. Base line of the left photograph of stereo pair

B. Base line of the right photograph of stereo pair

C. Sum of the base lines of stereo pair

D. Mean of the base lines of the stereo pair

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4

An aerial photograph may be assumed as

A. Parallel projection

B. Orthogonal projection

C. Central projection

D. None of these

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4

The altitudes of a circumpolar star at culminations are 70° and 10°, both culminations being north of zenith. The latitude of the place, is

A. 80°

B. 70°

C. 60°

D. 40°

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4

Latitude of a place is the angular distance from

A. Greenwich to the place

B. Equator to the poles

C. Equator to the nearer pole

D. None of these

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4

The distance between the projection centre and the photograph, is called

A. Principal distance

B. Principal line

C. Isocentric distance

D. Focal length

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4

If the distance between the projectors is altered by a movement along X-axis of one projector,

A. The length of the air base is increased

B. The scale of the model is altered

C. y-parallax is not affected

D. All the above

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4

The longitudes of two places at latitude 60° N are 93° E and 97° W. Their departure is

A. 5100 nautical miles

B. 5700 nautical miles

C. 120 nautical miles

D. 500 nautical miles

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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

Pick up the correct statement from the following:

A. One degree of longitude has greatest value at the equator

B. One degree of longitude has greatest value at the poles

C. One degree of longitude has the same value everywhere

D. One degree of latitude decreases from the equator to the poles

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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

Perspective centre relates to

A. Parallel projection

B. Orthogonal projection

C. Central projection

D. None of these

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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

In a truly vertical photograph,

A. Principal point coincides the isocenter

B. Iso-centre coincides the plumb point

C. Plumb point coincides the principal point

D. All the above

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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

D. None of these

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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

If θ and δ be the latitude of an observer and declination of a heavenly body respectively, the upper culmination of the body will be south of zenith if its zenith distance, is

A. δ - θ

B. θ - δ

C. θ + δ

D. ½ (θ - δ)

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4

The main object of the astronomer to obtain

A. Astronomical latitude

B. Astronomical longitude

C. Astronomical bearing

D. All of these

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4

Right ascension of a heavenly body is its equatorial angular distance measured

A. Westward from the first point of Libra

B. Eastward from the first point of Aeries

C. Westward from the first point of Aeries

D. Eastward from the first point of Libra

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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

The station pointer is generally used in

A. Triangulation surveying

B. Astronomical surveying

C. Hydrographical surveying

D. Photogrammetric surveying

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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

The method of surveying by triangulation was first introduced by the Dutchman Snell in

A. 1600

B. 1615

C. 1630

D. 1650

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4

Systematic errors

A. Always follow some definite mathematical law

B. Can be removed by applying corrections to the observed values

C. Are also known as cumulative errors

D. All the above

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4

Triangulation surveys are carried out for providing

A. Planimetric control

B. Height control

C. Both planimetric and height control

D. None of these

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4

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

D. All the above

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4

The station where observations are not made, but the angles at the station are used in triangulation series, is known as

A. Satellite station

B. Subsidiary station

C. Pivot station

D. Main station