Solar Time Formula:
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Sunrise and sunset time calculation involves determining the exact times when the sun appears above and disappears below the horizon. This calculation uses solar position formulas and accounts for various astronomical factors including the equation of time and longitude correction.
The calculator uses the solar time formula:
Where:
Explanation: The equation converts local clock time to true solar time, which is essential for accurate sunrise and sunset calculations based on the sun's actual position.
Details: Accurate solar time calculation is crucial for astronomy, navigation, agriculture, photography, and various scientific applications. It helps determine optimal times for solar energy collection and outdoor activities.
Tips: Enter local time in HH:MM format, equation of time in minutes (can be positive or negative), and longitude correction in minutes. The calculator will compute the corresponding solar time.
Q1: What is the Equation of Time?
A: The Equation of Time represents the difference between apparent solar time (based on the sun's position) and mean solar time (based on uniform clock time), ranging from -14 to +16 minutes throughout the year.
Q2: How is Longitude Correction calculated?
A: Longitude Correction = 4 × (Time Zone Longitude - Observer's Longitude) minutes, where longitude is in degrees and positive for east longitude.
Q3: Why is solar time different from clock time?
A: Solar time varies due to Earth's elliptical orbit and axial tilt, while clock time uses uniform time zones for practical purposes.
Q4: What factors affect sunrise and sunset times?
A: Latitude, longitude, date, altitude, atmospheric refraction, and observer's elevation all influence actual sunrise and sunset times.
Q5: How accurate are these calculations?
A: For most practical purposes, these calculations provide accuracy within 1-2 minutes, though extreme atmospheric conditions can cause variations.