Day Length Equation:
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The day length calculation determines the number of daylight hours at a given latitude for a specific date (represented by solar declination). It's important for agriculture, ecology, and understanding seasonal variations in sunlight.
The calculator uses the day length equation:
Where:
Explanation: The equation calculates the time between sunrise and sunset based on the angle of the sun relative to the Earth's surface at a given latitude.
Details: Day length affects plant growth, animal behavior, energy consumption patterns, and has cultural significance in many societies. Accurate calculation is essential for agricultural planning and solar energy projects.
Tips: Enter latitude between -90° (South Pole) and 90° (North Pole). Solar declination ranges from -23.45° (December solstice) to +23.45° (June solstice). Values outside these ranges will be automatically adjusted.
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 between ±23.45° throughout the year.
Q2: How do I find the solar declination for a specific date?
A: Solar declination can be calculated using specialized formulas or found in astronomical tables. Common values: 0° at equinoxes, +23.45° at June solstice, -23.45° at December solstice.
Q3: Why does day length change with latitude?
A: The Earth's axial tilt causes different latitudes to receive sunlight for different durations as the Earth orbits the Sun.
Q4: What happens at extreme latitudes?
A: Near the poles, day length can be 24 hours (midnight sun) or 0 hours (polar night) during solstices. The equation handles these cases mathematically.
Q5: Can this calculate twilight durations?
A: No, this calculates only the time between sunrise and sunset. Twilight calculations require additional parameters for different definitions of twilight.