SunPositionby SHIFT64
Latitude & Location
Select a preset city, reference point, or set precise coordinates using the slider
Automatic Daily Maxima (Solar Noon)
Automatically determines solar culmination (solar noon), where sun elevation is highest and incidence angle is smallest
Comparison of Two Dates Across the Year
Select any dates to immediately contrast solar radiation parameters and angles of incidence
2026-06-21
June 21, 20262026-12-21
December 21, 2026Comparative Overview (2026-06-21 vs 2026-12-21)
Direct differences in incidence angles, shadow geometry, and daylight duration
| Solar Parameter | 2026-06-21 | 2026-12-21 | Difference (Δ) |
|---|---|---|---|
| Maximum sun elevation (α_max at noon) | 61.2° | 14.4° | -46.8° |
| Angle of incidence on ground (zenith at noon) | 28.8° | 75.6° | +46.8° (shallower on 2026-12-21) |
| 1 m pole shadow length at noon | 0.55 m | 3.90 m | +3.35 m (609% longer) |
| Culmination time (clock noon) | 10:37 (UTC+2) | 10:34 (UTC+1) | Timezone shift of 1h (DST) |
| Day length (sunrise – sunset) | 16h 47m | 7h 42m | Difference: 9h 5m |
Sun Position on Celestial Dome & Elevation Angles
Astrometric celestial sphere: elevation angle (α) from 0° horizon to 90° zenith for both dates
24-Hour Solar Elevation Profile (00:00 – 24:00)
Solar altitude curve above the horizon throughout the full 24h day for both dates
Timezone & Clock Offset (Winter vs Summer)
Analysis of official CET / CEST differences and the equation of time effect on solar noon
Daylight Saving Time UTC+2 (CEST) applies in summer – clocks are shifted +1 hour forward, causing solar noon to occur around 12:30–13:00 clock time.
Standard Time UTC+1 (CET) applies in winter – the sun culminates (reaches maximum altitude) around 11:30–12:00 clock time.
- Daylight Saving Time (DST): In Europe from the last Sunday in March to the last Sunday in October, Daylight Saving Time (UTC+2) is observed. Clocks are moved +1h forward, causing solar noon in June to occur around 12:30–13:00. In December, on standard time (UTC+1), culmination occurs around 11:30–12:00.
- Longitude (21.01° E): Zone time UTC+1 is synchronized with the 15° E meridian. Every degree to the east shifts the solar culmination 4 minutes earlier.
- Equation of Time: Earth's elliptical orbit and axial tilt introduce natural variations in true solar time ranging from -14 to +16 minutes throughout the year.