I'm not sure how the term solar south is defined, but if it means the time when the sun crosses the meridian of the site's local longitude, that is, when the azimuth angle of the sun at a location is 180 degrees, that time will vary for each day of the year and can be conceptualized or graphed as something called the analemma of the sun. It's that funny looking figure 8 you used to see on some globes. Also check out "analemma + Stanford Solar Center" on Google for some neat pictures and some text.
One common term in use for that time is "solar noon".
Relative to civil clock time (and leaving D.S.T. adjustments out of it for this discussion) which is partially based on based on each day being exactly 24 hours in length, and a non elliptical orbit, the variation in the time when solar noon occurs is mostly caused by the slightly elliptical nature of the earth's orbit, and to a lesser degree by the wobbling of the earth on its axis (like a top) called precession, and some gravitational effects from the moon and the sun.
The magnitude of the annual variation of solar noon is about 30 minutes or so, from earliest to latest, with the variation being asymmetrical about civil clock mid day (noon) time and the degree of asymmetry f(longitude). The actual daily change is of the order of a few seconds/day.
Example: yesterday (12/16/2017) at my location, solar noon was at 11:44:17 P.S.T. and some fraction of a second. Today it was at 11:44:45 P.S.T.and some fraction of a second.
The earliest solar noon at my location occurs at 11:31:54 P.S.T. on 11/01 to 11/03.
The latest solar noon at my location occurs at 12:02:37 P.S.T.on 01/10/ to 02/02.
Those dates also wobble around by less than about 24 hours or so over a few years +/- some. .
Consult the nautical almanac for details.
All that and 5 bucks or more will get you a Starbucks.
One common term in use for that time is "solar noon".
Relative to civil clock time (and leaving D.S.T. adjustments out of it for this discussion) which is partially based on based on each day being exactly 24 hours in length, and a non elliptical orbit, the variation in the time when solar noon occurs is mostly caused by the slightly elliptical nature of the earth's orbit, and to a lesser degree by the wobbling of the earth on its axis (like a top) called precession, and some gravitational effects from the moon and the sun.
The magnitude of the annual variation of solar noon is about 30 minutes or so, from earliest to latest, with the variation being asymmetrical about civil clock mid day (noon) time and the degree of asymmetry f(longitude). The actual daily change is of the order of a few seconds/day.
Example: yesterday (12/16/2017) at my location, solar noon was at 11:44:17 P.S.T. and some fraction of a second. Today it was at 11:44:45 P.S.T.and some fraction of a second.
The earliest solar noon at my location occurs at 11:31:54 P.S.T. on 11/01 to 11/03.
The latest solar noon at my location occurs at 12:02:37 P.S.T.on 01/10/ to 02/02.
Those dates also wobble around by less than about 24 hours or so over a few years +/- some. .
Consult the nautical almanac for details.
All that and 5 bucks or more will get you a Starbucks.
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