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).
Apparent solar time is ahead of clock time in the UK during the winter and spring seasons. This is due to the equation of time, which accounts for the variation in the Earth's orbit and axial tilt throughout the year.
It is called "solar time" or "apparent solar time." This method of timekeeping is based on the position of the sun in the sky, with noon defined as when the sun is at its highest point.
apparent solar time
Time is based on the average length of the apparent solar day, which is the time it takes for the Sun to return to the same position in the sky, as observed on Earth. This forms the basis for the 24-hour day cycle that we use to structure our activities.
An apparent solar day is the time it takes for the Earth to complete one full rotation based on the position of the sun in the sky. It can vary slightly each day due to the Earth's elliptical orbit and axial tilt. This is different from a mean solar day, which is a consistent 24-hour period averaged over a year.
Apparent solar time is ahead of clock time in the UK during the winter and spring seasons. This is due to the equation of time, which accounts for the variation in the Earth's orbit and axial tilt throughout the year.
Because, when using "apparent solar time", the length of a "solar day" varies slightly during the year. (This is because the Earth's orbit isn't exactly circular and the Earth's axis is tilted.) "Clock time" is based on an average (or "mean") of these day lengths, called the "mean solar day". So clocks use "mean solar time". (By coincidence, on the date the question was answered (14th April) "apparent solar time" and 'clock' time are synchronised.) There's another reason for apparent solar time being different from clock time. "Clock time" uses time zones. So, over a wide area, the time on a clock equals the "mean solar time" at a particular, defining, longitude.
It very much depends on what is meant by solar time. Not really, it's fairly clear. There are 2 types of solar time: 1) "Apparent solar time". At any particular place this is called the "local apparent solar time", because it depends on longitude. 2) "Mean solar time". This averages out the natural variations of "apparent solar time". (The word "mean" is just a way of saying "average".) This too is depends on longitude of course, but time zones are used to cover a wide area, for convenience.
Because, when using "apparent solar time", the length of a "solar day" varies slightly during the year. (This is because the Earth's orbit isn't exactly circular and the Earth's axis is tilted.) "Clock time" is based on an average (or "mean") of these day lengths, called the "mean solar day". So clocks use "mean solar time". (By coincidence, on the date the question was answered (14th April) "apparent solar time" and 'clock' time are synchronised.) There's another reason for apparent solar time being different from clock time. "Clock time" uses time zones. So, over a wide area, the time on a clock equals the "mean solar time" at a particular, defining, longitude.
the distance between the solar time i.e Mean time apparent solar time is stated as equation of time. M.t-A.t=equation of time
It is called "solar time" or "apparent solar time." This method of timekeeping is based on the position of the sun in the sky, with noon defined as when the sun is at its highest point.
Time based on the sun is called solar time. It is measured using the position of the sun in the sky.
The Sun
The apparent solar day is longer in January due to the tilt of the Earth's axis and its elliptical orbit around the Sun. During this time, the Earth moves more slowly in its orbit, which affects the Sun's position in the sky. As a result, the time from one solar noon to the next is slightly extended, leading to longer apparent solar days. This phenomenon is part of the equation of time, which accounts for variations in the solar day throughout the year.
apparent solar time
Time is based on the average length of the apparent solar day, which is the time it takes for the Sun to return to the same position in the sky, as observed on Earth. This forms the basis for the 24-hour day cycle that we use to structure our activities.
Apparent solar time