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Sun Elevation Angle at Noon & Solar Declination

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Understanding the noon sun elevation and solar declination calculator — concept and principle

This calculator gives two numbers for any latitude and date: the solar declination (the latitude where the Sun is directly overhead at noon) and the Sun's elevation above the horizon at local solar noon, its highest point of the day. People use it to estimate solar panel tilt, shadow lengths, sunlight in rooms and gardens, and in geography lessons on the seasons.

Noon sun elevation in summer and winterAt latitude 37.57° the noon Sun is 75.9° high on 21 June (declination 23.44°) and about 29° on 21 December.How high the Sun climbs at noon21 Jun: 75.9°21 Dec: ≈ 29.0°elevation = 90° − |latitude − declination|June: 90 − |37.57 − 23.44| = 75.87°Dec: 90 − |37.57 + 23.44| ≈ 28.99°
The Sun’s declination swings ±23.44°, so Seoul’s noon Sun climbs about 47° higher in June than in December.

How it is calculated

The day number uses the year you enter (default 2026), so leap years are counted correctly.

The principle

Earth's axis is tilted about 23.44° to its orbit. As Earth goes around the Sun, the point directly beneath the Sun moves between 23.44° N (June solstice) and 23.44° S (December solstice), tracing roughly a sine wave over the year; that is the declination. At solar noon the Sun lies on your meridian. If it were overhead at latitude δ and you stand at latitude φ, the angle between the zenith and the Sun is simply the difference in latitude |φ − δ|, so its elevation is 90° minus that difference.

Worked example

  1. Inputs: latitude 37.57° (Seoul), 21 June, so N = 172.
  2. 360/365 × (172 − 81) = 89.75°, and sin 89.75° = 0.99999, so δ = 23.43978294°.
  3. |37.57 − 23.44| = 14.13°.
  4. Elevation = 90 − 14.13 = 75.86978294°.
  5. A 1 m pole would cast a noon shadow of 1 ÷ tan 75.87° ≈ 0.25 m.
How Noon elevation (°) changes with Latitude (°)How Noon elevation changes with Latitude304050607080909.3918.828.237.64756.475.1Example: 75.86978294Latitude (°)
Each point is the calculator re-run with only “Latitude (°)” changed; the gold point is the default example. Change the inputs above and this chart follows your numbers.
Latitude (°)Noon elevation (°)
9.3975.95271706
18.885.34521706
28.285.26228294
37.675.86978294
4766.47728294
56.457.08478294
75.138.29978294

How to read the result

For Seoul the noon elevation ranges from about 75.9° at the June solstice to 52.4° at the equinoxes and only about 29.0° at the December solstice, when a 1 m pole casts a shadow about 1.8 m long. If the elevation comes out negative, the Sun stays below the horizon all day (polar night). Within the tropics the Sun can be overhead (90°) on two days a year. A fixed solar panel facing south is often tilted near the latitude angle as a year-round compromise, though the best tilt depends on climate and local guidance.

Common mistakes

Keep in mind: The simple sine formula for declination can differ from precise values by up to about 1.4° on some dates, and refraction is ignored. Use an almanac or a full solar position algorithm when accuracy matters.

Frequently asked questions

Why is the hottest month not June if the Sun is highest then?

Land and oceans take weeks to warm up, so peak temperatures lag the solstice; in Korea the hottest period is usually late July to August.

What latitude has the Sun overhead at the June solstice?

The Tropic of Cancer, at about 23.44° N, which equals the axial tilt.

How do I get the shadow length?

Shadow length = object height ÷ tan(elevation).

Sources: J. Meeus, Astronomical Algorithms, 2nd ed., Willmann-Bell, 1998, Chapter 25 · J. A. Duffie and W. A. Beckman, Solar Engineering of Thermal Processes, 4th ed., Wiley, 2013

Checked 8 Nov 2026. Standard textbook formulas in SI units, computed in your browser. For learning and estimates — real designs must follow your local codes and be checked by a qualified engineer.

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