Total Solar Energy Formula:
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Total solar energy is the solar energy incident on the unit area of a horizontal surface on the ground. It represents the sum of direct solar radiation and diffuse solar radiation reaching a surface.
The calculator uses the total solar energy formula:
Where:
Explanation: The formula accounts for both direct solar radiation (adjusted by the cosine of the incidence angle) and diffuse solar radiation that reaches the horizontal surface.
Details: Accurate solar energy calculation is crucial for solar energy system design, building energy efficiency analysis, agricultural planning, and climate studies.
Tips: Enter direct solar radiation in W/m², angle of incidence in radians, and diffuse solar radiation in W/m². All values must be non-negative.
Q1: What is direct solar radiation?
A: Direct solar radiation is the part of solar radiation that reaches the earth's surface without being scattered or absorbed by the atmosphere.
Q2: What is diffuse solar radiation?
A: Diffuse solar radiation is the scattered solar radiation reaching the earth's surface uniformly from all directions.
Q3: Why is the cosine function used in the formula?
A: The cosine function adjusts the direct solar radiation component based on the angle of incidence, as the effective area receiving radiation decreases with increasing angle.
Q4: What are typical values for solar radiation components?
A: On a clear day, direct radiation can range from 600-1000 W/m², while diffuse radiation typically ranges from 50-200 W/m², depending on atmospheric conditions.
Q5: How does this calculation help in solar energy applications?
A: This calculation helps determine the total solar energy available for solar panels, heating systems, and other solar energy applications, enabling proper system sizing and efficiency analysis.