Radiation Processes in Astronomy: L9b - Spectral line scattering (classic), Lorentz profile, Q-value
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Radiation Processes in Astronomy: L9b - Spectral line scattering (classic), Lorentz profile, Q-value
A personal little favorite in lecture series. 🔹 We describe elastic scattering as classic, driven, weakly damped oscillator. First part on Thomson and Rayleigh (“why is the sky blue?”) limits and second, linked here, on resonance line scattering. 🔹 Among many other things, it gives underlying reason to the enormous power tapped in ...
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