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Climate & Environment

Solar Position Calculator

Calculate the sun's position (altitude and azimuth) for any location, date, and time. Essential for solar panels and photography.

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Know Exactly Where the Sun Will Be

The Solar Position Calculator determines the precise location of the sun in the sky for any moment in time. Whether you're installing solar panels, planning a photograph, or designing a building with optimal lighting, knowing the sun's altitude and azimuth is crucial for success.

What is Solar Position?

Solar position is described by two angles: altitude (elevation above the horizon, 0-90°) and azimuth (compass direction from north, 0-360°). These angles change throughout the day as Earth rotates and throughout the year as Earth orbits the Sun.

Solar Altitude Formula

sin(h) = sin(φ)sin(δ) + cos(φ)cos(δ)cos(H)

Why Calculate Solar Position?

Solar Energy Systems

Optimize solar panel tilt and orientation for maximum energy capture.

Architecture & Design

Plan window placement, shading, and passive solar heating.

Photography

Plan golden hour shots and predict lighting conditions.

How to Use This Calculator

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Common Applications

Solar Panel Installation

Calculate optimal tilt angle based on sun's path throughout the year.

Shadow Analysis

Predict shadow lengths and directions for architectural planning.

Sundial Design

Calculate hour angles for accurate sundial construction.

Film Production

Plan outdoor shoots with predictable lighting conditions.

Frequently Asked Questions

Solar altitude is the angle of the sun above the horizon, measured in degrees. At 0° the sun is at the horizon, at 90° it's directly overhead (only possible near the equator).

Solar azimuth is the compass direction of the sun measured clockwise from north. East is 90°, south is 180°, and west is 270°.

Shadow length depends on the sun's altitude. When the sun is low (small altitude), shadows are long. When the sun is high (large altitude), shadows are short. The ratio is: shadow = object height / tan(altitude).

The hour angle measures how far the sun has traveled across the sky from solar noon. It's 0° at solar noon, negative in the morning, and positive in the afternoon, increasing by 15° per hour.

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