Solar Power Equation:
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The solar power calculation estimates the electrical power output of a solar panel based on the amount of sunlight it receives (irradiance), its physical size, and its conversion efficiency. This helps in designing solar energy systems and estimating their potential output.
The calculator uses the solar power equation:
Where:
Explanation: The equation multiplies the solar energy available (irradiance) by the panel's collection area and its efficiency at converting sunlight to electricity.
Details: Accurate solar power estimation is crucial for system sizing, energy production forecasting, and return on investment calculations for solar installations.
Tips: Enter irradiance in W/m² (typically 1000 W/m² for standard test conditions), panel area in m², and efficiency as a decimal between 0 and 1 (e.g., 0.18 for 18% efficiency).
Q1: What is typical solar panel efficiency?
A: Most commercial panels range from 15-22% efficiency, with premium models reaching up to 23-24%.
Q2: How does irradiance vary by location?
A: Annual average irradiance ranges from about 100 W/m² in cloudy regions to 250 W/m² in sunny deserts.
Q3: What affects solar panel efficiency?
A: Temperature (higher temps reduce efficiency), angle to sun, shading, dust, and panel technology (monocrystalline is most efficient).
Q4: Why calculate power output?
A: To properly size solar arrays for energy needs, calculate return on investment, and compare different panel options.
Q5: What's the difference between STC and real-world output?
A: Standard Test Conditions (STC) use 1000 W/m² at 25°C - real output is typically 10-25% lower due to temperature, angle, and other factors.