Sunlight Hours Formula:
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The Sunlight Hours calculation estimates the number of daylight hours at a specific latitude and solar declination angle. This formula is based on astronomical principles and helps determine day length for any location on Earth throughout the year.
The calculator uses the sunlight hours formula:
Where:
Explanation: The formula calculates the hour angle of sunrise/sunset and converts it to daylight hours, accounting for the Earth's axial tilt and geographic position.
Details: Accurate sunlight hours calculation is crucial for agriculture, solar energy planning, architectural design, climate studies, and understanding seasonal variations in daylight.
Tips: Enter latitude between -90° and +90° (negative for Southern Hemisphere), and declination between -23.45° and +23.45°. The calculator handles trigonometric calculations automatically.
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, varying throughout the year due to Earth's axial tilt.
Q2: How does latitude affect sunlight hours?
A: Higher latitudes experience greater seasonal variation in daylight hours, with extreme cases of midnight sun and polar nights near the poles.
Q3: What are typical declination values?
A: Declination ranges from approximately -23.45° (December solstice) to +23.45° (June solstice), with 0° at equinoxes.
Q4: Why does the formula return errors for some inputs?
A: When the product of tangents exceeds ±1, it indicates polar night (24-hour darkness) or midnight sun (24-hour daylight) conditions.
Q5: Can this be used for any date?
A: Yes, by using the appropriate solar declination for the specific date. Declination can be calculated or obtained from astronomical tables.