apparent solar time sentence in Hindi
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- "' Mean solar time "'was originally apparent solar time corrected by the equation of time.
- :The solar time article, specifically the section on apparent solar time gets at the reasons for this.
- Of course, the equation of time can still be used, when required, to obtain apparent solar time from clock time.
- Times in the Almanac were in apparent solar time, because time aboard ship was most often determined by observing the Sun.
- Two types of solar time are apparent solar time ( sundial time ) and mean solar time ( clock time ).
- An analemma may be added to many types of sundials to correct apparent solar time to mean solar time or another standard time.
- From 1767 to 1833, the British " Nautical Almanac and Astronomical Ephemeris " tabulated the equation of time in the sense'mean minus apparent solar time '.
- The start of each year was determined according to the day of the autumnal equinox, in relation to true or apparent solar time at the Paris Observatory.
- The apparent solar time is a measure of the Earth's rotation and the difference between it and the mean solar time is known as the equation of time.
- Divided into 12 equal parts, sundials tell apparent solar time by measuring the visible passage of the sun through its daily course in the sky, from east to west.
- Decimal time would also have been reckoned according to apparent solar time, depending on the location it was observed, as was already the practice generally for the setting of clocks.
- Gerald J . Toomer uses the medieval term " equation " from the Latin " aequtiM ", for Ptolemy's difference between the mean solar time and the apparent solar time.
- I think " local solar time " is what I usually see for it, although Wikipedia's Solar time article goes with " apparent solar time " .-- Anon, July 11.22 : 30 ( UTC ).
- The two times that differ are the " apparent solar time ", which directly tracks the motion of the sun, and " mean solar time ", which tracks a theoretical " mean " sun with noons 24 hours apart.
- Solar time is measured by the apparent diurnal motion of the Sun, and local noon in apparent solar time is the moment when the Sun is exactly due south or north ( depending on the observer's latitude and the season ).
- In the unusual case that the apparent solar time of an observation was needed, one would apply the equation of time to " mean " solar time, requiring all differences in the equation of time to have the opposite sign than before.
- When the apparent solar time that corresponds to a given civil time is to be found, the difference in longitude between the site of interest and the time zone meridian, daylight saving time, and the equation of time must all be considered.
- I noticed an interesting citation of Wikipedia about the definition of one form of time ( apparent solar time ) in a presentation to a BIPM / ITU meeting that will influence the possible redefinition of another form of time ( UTC ).
- This may be due to imprecision in the ephemeris data used by JPL Horizons; also the JPL Horizons data gives local apparent solar time while the times reported above are probably some form of mean solar time ( and therefore some of the discrepancy would be due to the Martian equivalent of the equation of time ).
- Apparent solar time can be obtained by measurement of the current position ( hour angle ) of the Sun, as indicated ( with limited accuracy ) by a sundial . " Mean " solar time, for the same place, would be the time indicated by a steady clock set so that over the year its differences from apparent solar time would resolve to zero.
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