Daylight Length Formula:
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The Daylight Length formula calculates the number of daylight hours at a specific location on Earth based on latitude and solar declination. This astronomical formula helps determine day length for any given date and location.
The calculator uses the daylight length formula:
Where:
Explanation: The formula 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 length calculations are essential for agriculture, solar energy planning, architectural design, tourism, and understanding seasonal variations in climate and ecosystems.
Tips: Enter latitude in degrees (-90 to 90) and solar declination in degrees (-23.45 to 23.45). For accurate results, ensure inputs are within valid ranges and use appropriate declination values for specific dates.
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 do I find solar declination for a specific date?
A: Solar declination can be calculated using astronomical formulas or obtained from solar position calculators and almanacs for specific dates.
Q3: Why does daylight length vary throughout the year?
A: Daylight length varies due to Earth's 23.5° axial tilt and its revolution around the sun, causing seasonal changes in solar declination.
Q4: What are extreme cases of daylight length?
A: At polar circles (66.5° latitude), 24-hour daylight occurs at summer solstice; at poles, 6 months of continuous daylight followed by 6 months of darkness.
Q5: Is this formula accurate for all locations?
A: The formula provides theoretical daylight length; actual sunrise/sunset times may vary due to atmospheric refraction, elevation, and local topography.