Surveying The latitude of the observer's position, is Angular distance along the observer's meridian between equator and the observer Declination of the observer's zenith All listed here Elevation of the elevated pole Angular distance along the observer's meridian between equator and the observer Declination of the observer's zenith All listed here Elevation of the elevated pole ANSWER DOWNLOAD EXAMIANS APP
Surveying If the staff is not held vertical at a level¬ling station, the reduced level calculated from the observation would be less than true R.L. None of these more than true R.L. true R.L. less than true R.L. None of these more than true R.L. true R.L. ANSWER DOWNLOAD EXAMIANS APP
Surveying At the first point of Aeries, the sun moves From north to south of the equator From south to north of the equator Southward Northward From north to south of the equator From south to north of the equator Southward Northward ANSWER DOWNLOAD EXAMIANS APP
Surveying The cross hairs in the surveying telescope are placed much closer to the objective lens than to the eye piece much closer to the eye-piece than to the objective lens midway between eye piece and objec-tive lens anywhere between eye-piece and objective lens much closer to the objective lens than to the eye piece much closer to the eye-piece than to the objective lens midway between eye piece and objec-tive lens anywhere between eye-piece and objective lens ANSWER DOWNLOAD EXAMIANS APP
Surveying The most convenient co-ordinate system for specifying the relative positions of heavenly bodies on the celestial sphere, is Altitude and azimuth system Declination and hour angle system Declination and right ascension system Declination and altitude system Altitude and azimuth system Declination and hour angle system Declination and right ascension system Declination and altitude system ANSWER DOWNLOAD EXAMIANS APP
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