Daylight Calculation Formula:
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The daylight calculation estimates the length of daylight (sunrise to sunset) at a given latitude on a specific date (represented by solar declination). It's based on astronomical formulas that account for Earth's axial tilt and position in its orbit.
The calculator uses the daylight formula:
Where:
Explanation: The formula calculates the hour angle of sunrise/sunset and converts it to time. The factor of 2 accounts for both sunrise and sunset angles, and the division by 15 converts degrees to hours (since Earth rotates 15° per hour).
Details: Knowing daylight duration is crucial for agriculture, solar energy planning, architectural design, and understanding seasonal variations in different geographic locations.
Tips: Enter latitude between -90° (South Pole) and 90° (North Pole). Declination ranges from -23.5° (winter solstice) to +23.5° (summer solstice), with 0° at equinoxes.
Q1: What is solar declination?
A: Solar declination is the angle between the Sun's rays and Earth's equatorial plane, varying between ±23.5° throughout the year due to Earth's axial tilt.
Q2: How accurate is this calculation?
A: It provides theoretical maximum daylight, not accounting for atmospheric refraction, terrain, or twilight periods which can add several minutes of daylight.
Q3: What's the daylight at the poles?
A: At summer solstice (δ ≈ 23.5°), polar day occurs with 24 hours of daylight. At winter solstice (δ ≈ -23.5°), polar night occurs with 0 hours of daylight.
Q4: How does latitude affect daylight?
A: Daylight variation increases with latitude. Near the equator, daylight is nearly constant (~12 hours). At higher latitudes, seasonal variation becomes extreme.
Q5: Can I calculate sunset/sunrise times with this?
A: This gives total daylight duration. For actual sunrise/sunset times, you'd need to calculate the hour angle and adjust for longitude and time zone.