Please, though, answer this simplified version of the previous question, yes or no. The apparent angular movement of Polaris is 15 (+/-1) degrees per hour.
Polaris surely follows the 360 degrees path around the celestial pole, no matter how close.
On that path it travels 15 degrees per hour.
At one moment it will be due east, and roughly 12 hours later it will be due west, 180 degrees away.
Alpha UMI Aa sits at the declination of 89° 15' 50.8" (89,264 degrees, or 0.736 degrees away from the celestial pole).
From the point of view of some random observer anywhere at the Earth's surface the total daily movement range will cover only 1.472 degrees.
During one day speed of the apparent movement is constant.
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Now, let's try to predict the Sun's apparent traveling angles before we test them in some actual observation:
[spoiler='Sun Virtual Path Basic Data']
R: Rowbotham's model, Sun for equinoctial solar noon from 45 degrees north seen at 45 degrees elevation, which gives the height of 3110 miles = 5005 km
G: Globe model, Sun's distance from the ground 149 ± 3 million km
(the times are solar, the solar noon is at 12:00 pm)
1. England, Germany, Poland is mostly around 52 degrees north.
2. Boston, New York, Philadelphia, Washington (and Madrid, Rome, Istanbul, Beijing) are grouped around 40 degrees north.
3. Sydney, Canberra, Melbourne, Adelaide (and Santiago, Buenos Aires, Montevideo) are around 35 degrees south.
J: June solstice.
Sun's trajectory
JR: curve radius 7389 km,
center of the curve 5005 km above the North pole,
tangential speed 1934 km/h.
JG: curve radius 152 000 000 x cos(23.5) = 139 393 313 km,
center of the curve 152 000 000 x sin(23.5) = 60 609 858 km above the center of the Earth,
tangential speed 36 493 084 km/h.
S: September equinox.
Sun's trajectory
SR: curve radius 10 000 km,
center of the curve 5005 km above the North pole
tangential speed 2618 km/h.
SG: curve radius 149 000 000 km,
center of the curve in the center of the Earth,
tangential speed 39 008 109 km/h.
D: December solstice.
Sun's trajectory
DR: curve radius 12 611 km,
center of the curve 5005 km above the North pole,
tangential speed 3302 km/h.
DG: curve radius 146 000 000 x cos(23.5) = 133 890 771 km,
center of the curve 146 000 000 x sin(23.5) = 58 217 364 km below the cenetr of the Earth,
tangential speed 35 052 522 km/h.
(By now you already understood what would here be the meaning of, say, SR2: S - September Equinox, R - Rowbotham's model, 2 - observer is at 40 degrees north)
EDIT: Looks like "Spoiler" tag doesn't work on this forum.
[/spoiler]
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JR1: 6 am / 6 pm - 10.45 degrees per hour, 12 pm - 18 degrees per hour
JG1: 6 am / 6 pm - 13.5 degrees per hour, 12 pm - 13.5 degrees per hour
JR2: 6 am / 6 pm - 8.35 degrees per hour, 12 pm - 20 degrees per hour
JG2: 6 am / 6 pm - 13.5 degrees per hour, 12 pm - 13.5 degrees per hour
JR3: 6 am / 6 pm - 3.75 degrees per hour, 12 pm - 16.5 degrees per hour
JG3: 6 am / 6 pm - 13.5 degrees per hour, 12 pm - 13.5 degrees per hour
SR1: 6 am / 6 pm - 11.5 degrees per hour, 12 pm - 19 degrees per hour
SG1: 6 am / 6 pm - 14.67 degrees per hour, 12 pm - 14.67 degrees per hour
SR2: 6 am / 6 pm - 10.4 degrees per hour, 12 pm - 21.3 degrees per hour
SG2: 6 am / 6 pm - 14.67 degrees per hour, 12 pm - 14.67 degrees per hour
SR3: 6 am / 6 pm - 4.9 degrees per hour, 12 pm - 22.5 degrees per hour
SG3: 6 am / 6 pm - 14.67 degrees per hour, 12 pm - 14.67 degrees per hour
DR1: 6 am / 6 pm - 12.4 degrees per hour, 12 pm - 18.9 degrees per hour
DG1: 6 am / 6 pm - 13.5 degrees per hour, 12 pm - 13.5 degrees per hour
DR2: 6 am / 6 pm - 18.7 degrees per hour, 12 pm - 21.3 degrees per hour
DG2: 6 am / 6 pm - 13.5 degrees per hour, 12 pm - 13.5 degrees per hour
DR3: 6 am / 6 pm - 6.5 degrees per hour, 12 pm - 32.5 degrees per hour
DG3: 6 am / 6 pm - 13.5 degrees per hour, 12 pm - 13.5 degrees per hour
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Obviously (without refraction) the apparent Sun's angular speed will vary much more in Rowbotham's model than in Globe model.
In Rowbotham's model it depends on location, and can be as low as 4 degrees in the morning (in Soth pole even lower),
and as high as 32 degrees (on Equator even higher).
In Globe model varies during a year, from 13.5 to 14.67 degrees, and during a day it remains practically constant, regardless the observer's location on the Earth.
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Now, how fast is the Sun really traveling across the sky in the places where each of us lives?