Sunrise Time Equation:
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The Sunrise Time Equation calculates the time of sunrise based on geographic latitude and solar declination. It's derived from astronomical principles and provides the local solar time of sunrise.
The calculator uses the Sunrise Time equation:
Where:
Explanation: The equation calculates the hour angle of sunrise and converts it to local solar time, with 12 representing solar noon.
Details: Accurate sunrise time calculation is important for agriculture, photography, religious observances, and various scientific applications.
Tips: Enter latitude in degrees (-90 to 90), solar declination in degrees (-23.5 to 23.5). The result is in local solar time (HH:MM format).
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 ±23.5° throughout the year.
Q2: Why does the equation use 12 as the base?
A: 12 represents solar noon (when the Sun is highest in the sky), from which we subtract the time it takes for the Sun to rise from the horizon.
Q3: How accurate is this calculation?
A: This provides theoretical sunrise time. Actual sunrise may vary due to atmospheric refraction, elevation, and local topography.
Q4: Can I use this for any date?
A: Yes, but you need to know the solar declination for your specific date (which changes throughout the year).
Q5: What about sunset time?
A: Sunset time can be calculated similarly by adding instead of subtracting the hour angle (T = 12 + (hour_angle/15)).