Sunrise Equation:
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Sunrise and sunset times represent the moments when the upper limb of the Sun appears or disappears on the horizon. These calculations are essential for astronomy, navigation, agriculture, and various cultural and religious practices.
The calculator uses the sunrise equation:
Where:
Explanation: The equation calculates the hour angle of sunrise based on latitude and solar declination, then converts this to local solar time.
Details: Accurate sunrise and sunset calculations are crucial for planning outdoor activities, agricultural operations, energy management (solar power), and understanding seasonal daylight variations.
Tips: Enter latitude in degrees (-90 to 90), solar declination in degrees (-23.5 to 23.5). For sunset calculation, use the same equation but add instead of subtract the hour angle term.
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 accurate is this calculation?
A: This provides approximate solar times. Actual sunrise/sunset times are affected by atmospheric refraction, elevation, and local topography.
Q3: What does "No sunrise/sunset" mean?
A: This occurs during polar day/night when the Sun doesn't rise or set for extended periods at high latitudes.
Q4: How to calculate sunset time?
A: Sunset = 12 + (1/15) × acos(-tan(lat)tan(decl)), using the same formula but adding the hour angle instead of subtracting.
Q5: What's the difference between solar time and local time?
A: Solar time is based on the Sun's position, while local time includes time zone adjustments and daylight saving time.