Formula Used:
| From: | To: | 
Mean Hemi-Spherical Candle Power is a measurement that represents the average intensity of light emitted by a source in all directions within a hemisphere. It quantifies the overall luminous intensity distribution of a light source.
The calculator uses the formula:
Where:
Explanation: This formula calculates the average candle power over a hemisphere by dividing the total luminous flux by 2π, which represents the solid angle of a hemisphere.
Details: Calculating Mean Hemi-Spherical Candle Power is crucial for lighting design, photometric analysis, and evaluating the efficiency and performance of light sources in various applications.
Tips: Enter the luminous flux value in lumens. The value must be greater than zero for accurate calculation.
                    Q1: What is the difference between candle power and luminous flux?
                    A: Candle power measures luminous intensity in a specific direction, while luminous flux measures the total light output in all directions.
                
                    Q2: Why is the hemisphere used in this calculation?
                    A: The hemisphere represents the typical lighting environment where light is emitted in the downward direction, making it relevant for most practical lighting applications.
                
                    Q3: What are typical M.H.S.C.P. values for common light sources?
                    A: Values vary significantly depending on the light source type and wattage. For example, a 60W incandescent bulb might have M.H.S.C.P. around 70-80 candela.
                
                    Q4: How does M.H.S.C.P. relate to illuminance?
                    A: M.H.S.C.P. represents the light source's intensity, while illuminance measures the amount of light falling on a surface. They are related through the inverse square law and cosine law.
                
                    Q5: Are there limitations to this calculation method?
                    A: This calculation assumes uniform light distribution. For sources with non-uniform distribution patterns, more complex photometric analysis may be required.