Daylight Formula:
From: | To: |
Definition: This calculator estimates the number of daylight hours at a given latitude on a specific day of the year based on solar declination.
Purpose: It helps astronomers, meteorologists, and anyone interested in daylight patterns understand how day length varies with location and season.
The calculator uses the formula:
Where:
Explanation: The formula calculates the fraction of the day that the sun is above the horizon based on the Earth's axial tilt and the observer's latitude.
Details: Understanding daylight duration is crucial for agriculture, solar energy planning, architectural design, and understanding seasonal changes.
Tips: Enter your latitude (-90 to 90) and the solar declination (-23.45 to 23.45) for the date of interest. The calculator will compute the hours of daylight.
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 between ±23.45° throughout the year.
Q2: How do I find solar declination for a specific date?
A: Use our Solar Declination Calculator or astronomical tables. It's approximately 0° at equinoxes and ±23.45° at solstices.
Q3: What happens at extreme latitudes?
A: Near the poles, this formula accounts for midnight sun (24-hour daylight) and polar night (no daylight) when appropriate.
Q4: Does this account for atmospheric refraction?
A: No, this is a theoretical calculation. Actual daylight is slightly longer due to atmospheric effects.
Q5: What's the daylight at the equator?
A: Approximately 12 hours year-round, as the sun rises and sets nearly perpendicular to the horizon.