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Apparent solar time
At mid-day or when the sun is as close to overhead of you as possible. At this time, your shadow will be directly below you and not long, as it is at sunrise or sunset. If you want which day in a year the Shadow likely to be smallest than it is June 22
Godfather 405 days...(95 days as regular show and rest as noon show) Chitram (366 days regular show)
the tilt goes towards the sun, the seasons chang from winter to summer
sunset comes first and then noon.
The same as local apparent noon. When the sun is the highest in the sky. This is true. However; to be more specific solar noon is half way between sunrise and sunset. It's at solar noon that a point gets the most direct sunlight of the day. To calculate solar noon you find out how many hours of daylight there are between sunrise and sunset and divide by 2. Add the quotient to the sunrise time and that will give you the solar noon time.
In France, noon is typically referred to as "midi."
Solar radiation is most intense at noon.
Solar noon is the time when the Sun appears to contact the local celestial meridian. This is when the Sun apparently reaches its highest point in the sky, at 12 noon apparent solar time and can be observed using a sundial. The local or clock time of solar noon depends on the longitude and date.
the answer would be Solar TIme
After you.
A Solar Day.
A Solar Day.
Solar Noon is when the sun is highest in the sky, or closest to zenith, so there would be no direction of shadow, it would be under your feet. To test this yourself on Nov. 22 the solar noon in NYC will be at 11:42:15, go find out for yourself.
Its position and apparent movement around the sky. "Apparent solar time" is based on the "apparent solar day", reckoned by defining as 'solar noon' the moment of the Sun's highest altitude above the horizon on any given day. (That's when the Sun crosses the observer's meridian.) Apparent solar days do not have the exact same length (from one solar noon to the next) throughout the year, which is surprising to some at first. This is why the first approaches to creating a solid "standard time" involved determining the length of the 'mean solar day' (average solar day).
at each place ,whenever the sun was directly overhead , it was considered noon this was called solar time.
at each place ,whenever the sun was directly overhead , it was considered noon this was called solar time.