Solar Luminance Formula:
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Solar luminance refers to the luminous intensity per unit area of the sun's surface. It measures how much light the sun emits in a given direction per unit area, typically expressed in candelas per square meter (cd/m²).
The calculator uses the fundamental luminance formula:
Where:
Explanation: For the sun, the standard luminance value is approximately 1.6×10⁹ cd/m², which represents the intense brightness of the solar surface.
Details: Understanding solar luminance is crucial for astronomy, solar energy research, atmospheric studies, and designing optical systems that interact with sunlight. It helps in calculating solar radiation intensity and understanding the sun's energy output.
Tips: Choose between custom calculation (enter illuminance and area values) or use the standard solar value. For custom calculations, enter illuminance in lux and area in square meters. The standard solar luminance is approximately 1.6 billion cd/m².
Q1: What is the difference between luminance and illuminance?
A: Luminance measures the light emitted or reflected from a surface (cd/m²), while illuminance measures the light falling on a surface (lux).
Q2: Why is the sun's luminance so high?
A: The sun's extreme luminance results from its high surface temperature (about 5,778 K) and nuclear fusion processes that generate immense amounts of light energy.
Q3: How does solar luminance affect Earth?
A: Solar luminance determines the intensity of sunlight reaching Earth, influencing climate, weather patterns, and the amount of solar energy available for power generation.
Q4: Can I measure solar luminance directly?
A: Direct measurement requires specialized equipment like photometers or luminance meters with appropriate filters to handle the sun's intense brightness safely.
Q5: How does atmospheric conditions affect solar luminance?
A: Atmospheric scattering, absorption, and cloud cover can significantly reduce the apparent luminance of the sun as seen from Earth's surface compared to measurements in space.