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Current Affairs January 2024

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4

The true and mean suns occupy the same meridian at the same time on

A. April 15

B. June 14

C. September 1

D. All the above

Correct Answer :

D. All the above


Related Questions

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4

Homologous points are

A. Opposite corners of a photograph

B. Nodal points of the camera lens

C. Corresponding points on the ground and photograph

D. Plumb points of stereo pair of photographs

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4

To obtain photographs of an area of 1000 m average elevation, on scale 1 : 30, 000, with a camera of 30 cm focal length, the flying height is

A. 4000 m

B. 5000 m

C. 6000 m

D. 7000 m

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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 great circle which passes through the zenith, nadir and the poles, is known as

A. Meridian

B. Vertical circle

C. Prime vertical

D. None of these

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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

The scale of a vertical photograph of focal length f taken from height of H metres above M.S.L., at a point of reduced level h, is

A. f/H

B. f/(H + h)

C. f/(H - h)

D. (H - h)/f

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4

The great circle whose plane is perpendicular to the axis of rotation of the earth, is called

A. Equator

B. Terrestrial equator

C. 0° latitude

D. All the above

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4

Pick up the correct statement from the following:

A. The principal point coincides with plumb point on a true vertical photograph

B. The top of a hill appears on a truly vertical photograph at greater distance than its bottom from the principal point

C. The top of a hill is represented on a vertical photograph at larger scale than the area of a nearby valley

D. All the above

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4

The declination and right ascension of the sun becomes 23° 27' S and 270° respectively on

A. March 21

B. June 21

C. September 21

D. December 22

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4

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

A. sin H = tan φ . cot δ

B. cos H = tan φ . cot δ

C. tan H = tan φ . cot δ

D. None of these

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4

If δ is the declination of the star and φ is the latitude of the observer, then the azimuth of the star at elongation is given by

A. sin z = sec φ . cos δ

B. cos z = sec φ . cos δ

C. tan z = sec φ . cos δ

D. None of these

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4

At western elongation, the pole star moves

A. Eastward

B. Westward

C. Northward

D. Southward

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4

A star may culminate at zenith if its declination is

A. Greater than the longitude of the place

B. Less than the latitude of the place

C. Equal to the latitude of the place

D. None of these

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4

Pick up the incorrect statement from the following. High oblique photographs

A. May have tilt up to 30°

B. May include the image of the horizon

C. May not include the image of the horizon

D. None of these

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4

The parallax of a point on the photograph is due to

A. Ground elevation

B. Flying height

C. Length of air base

D. All the above

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4

Parallax bar measures

A. Parallax

B. Height

C. Parallax difference

D. Height difference

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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

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4

The latitude of a place was obtained by subtracting the zenith distance of a star from its declination, the observed star was between

A. Horizon and equator

B. Equator and zenith

C. Zenith and pole

D. Pole and horizon

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4

From the principal point the horizon point lies on the principal line at a distance of

A. f tan θ

B. f sin θ

C. f cot θ

D. f cos θ

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4

The principal line is the line joining the principal point and

A. Nadir

B. Isocenter

C. Perspective centre

D. None of these

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4

The normal longitudinal overlap is generally kept

A. 50 %

B. 60 %

C. 70 %

D. 75 %

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4

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

A. 80°

B. 70°

C. 60°

D. 50°

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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 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

If two points differing by 1° of latitude and of the same longitude is 110 km apart on the earth, then two astronomical positions on the moon is about

A. 10 km

B. 25 km

C. 30 km

D. 50 km

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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

D. None of these

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4

The displacement of the pictured position of a point of h elevation on a vertical photograph taken with a camera of 30 cm focal length, from an altitude of 3000 m, is

A. 4.4 mm

B. 5.5 mm

C. 6.5 mm

D. 7.5 mm

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4

Pick up the correct statement from the following:

A. The measured stereoscopic base of photographs is obtained by dividing the air base in metres by the mean scale of the photograph

B. The difference between the absolute parallax of two points depends upon the difference in their elevations

C. The line joining the principal point of a photograph and the transferred principal point of the adjoining photograph, is called stereoscopic base

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

If v, t and f/H are the ground speed of the aircraft, the shutter speed of the camera and the scale of the photograph respectively, then the amount of image displacement

A. i = v. t. H/f

B. i = v. f/t. H

C. i = v. t. (f/H)

D. i = t. H/v. f