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Spectral Flux

/ˈspɛk.trəl flʌks/noun
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Spectral flux is the measure of electromagnetic energy or photons received per unit area per unit time, distributed across different wavelengths or frequencies, making it a cornerstone of spectroscopic analysis. This concept helps scientists decode the composition, temperature, and motion of celestial bodies, and in modern applications, it's used to study everything from distant galaxies to atmospheric phenomena on Earth.

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