Solar Altitude Equation:
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Solar altitude (α) is the angle between the sun and the horizontal plane at a specific location and time. It represents how high the sun appears in the sky and is a crucial parameter in astronomy, solar energy, and navigation.
The calculator uses the solar altitude equation:
Where:
Explanation: The equation calculates the sun's position in the sky based on astronomical coordinates and the observer's location and time.
Details: Solar altitude is essential for solar panel positioning, architectural design, agricultural planning, and various scientific applications. It helps determine the intensity of solar radiation and optimal sun exposure.
Tips: Enter declination (δ), latitude (φ), and hour angle (H) in degrees. All values must be valid numerical inputs within appropriate ranges for accurate calculation.
Q1: What is solar declination?
A: Solar declination is the angular distance of the sun north or south of the celestial equator, varying throughout the year due to Earth's axial tilt.
Q2: How is hour angle calculated?
A: Hour angle is the angular distance between the sun's current position and its position at solar noon, measured along the celestial equator.
Q3: What are typical solar altitude values?
A: Solar altitude ranges from 0° (sunrise/sunset) to 90° (directly overhead at equator during equinoxes), varying by location, season, and time of day.
Q4: How does latitude affect solar altitude?
A: Higher latitudes generally have lower maximum solar altitudes, while equatorial regions experience higher solar altitudes throughout the year.
Q5: What applications use solar altitude calculations?
A: Solar energy systems, architecture, agriculture, photography, aviation, maritime navigation, and astronomical observations all utilize solar altitude data.