Solar Hour Angle Formula:
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The Solar Hour Angle formula calculates the angular displacement of the sun east or west of the local meridian due to the Earth's rotation. It is a fundamental parameter in solar position calculations and astronomy.
The calculator uses the Solar Hour Angle formula:
Where:
Explanation: The Earth rotates 15 degrees per hour (360°/24h), so the hour angle changes by 15 degrees for each hour difference from solar noon.
Details: Hour angle is crucial for determining solar position, calculating sunrise/sunset times, designing solar energy systems, and in astronomical observations.
Tips: Enter Local Solar Time and Solar Noon in hours (0-24 format). Positive results indicate afternoon hours, negative results indicate morning hours.
Q1: What is the range of hour angle values?
A: Hour angle ranges from -180° to +180°, with negative values before solar noon and positive values after solar noon.
Q2: How is solar noon determined?
A: Solar noon is when the sun reaches its highest point in the sky, which varies by location and date due to longitude and equation of time.
Q3: What's the difference between solar time and standard time?
A: Solar time is based on the sun's position, while standard time uses time zones. They can differ by up to 30 minutes due to longitude and daylight saving.
Q4: How accurate is this calculation?
A: The formula provides theoretical hour angle. For precise calculations, factors like atmospheric refraction and equation of time should be considered.
Q5: What are practical applications of hour angle?
A: Solar tracking systems, architectural design, agricultural planning, photography, and astronomical observations all use hour angle calculations.