Daylight Equation:
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The Daylight Equation calculates the number of daylight hours at a given latitude and solar declination angle. It's based on astronomical principles and provides accurate daylight duration for any location on Earth.
The calculator uses the daylight equation:
Where:
Explanation: The equation calculates the hour angle of sunrise/sunset and converts it to daylight hours, accounting for the Earth's spherical geometry and axial tilt.
Details: Daylight duration affects agriculture, energy consumption, human circadian rhythms, tourism planning, and solar energy production. Accurate daylight prediction is essential for various scientific and practical applications.
Tips: Enter latitude between -90° (South Pole) and 90° (North Pole), and solar declination between -23.5° (winter solstice) and 23.5° (summer solstice). All values must be within valid ranges.
Q1: What is solar declination?
A: Solar declination is the angle between the rays of the sun and the plane of the Earth's equator. It varies throughout the year due to Earth's axial tilt.
Q2: How does latitude affect daylight hours?
A: Higher latitudes experience greater variation in daylight hours throughout the year, with polar regions having 24 hours of daylight or darkness during solstices.
Q3: What are typical daylight hours at the equator?
A: At the equator, daylight hours remain relatively constant at approximately 12 hours throughout the year, with minor variations.
Q4: Why does the equation use trigonometric functions?
A: Trigonometric functions accurately model the spherical geometry of Earth and the relationship between latitude, declination, and sun position.
Q5: Can this calculate daylight for any date?
A: Yes, when provided with the correct solar declination for that date. Solar declination can be calculated or looked up in astronomical tables.