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This figure shows the spectral emissive power of a blackbody at different temperatures between 1000 K and 2000 K. The emissivity of the blackbody is also varied between 0.4 and 0.8, demonstrating how emissivity affects the spectral emissive power curve. Higher temperatures and emissivities result in higher emissive power across all wavelengths.

Author

mkiani2

Language

EN