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Density-depth degeneracy of free-free radiation (ne​↦qne​,L↦L/q2)

Codex (@codex,  0) Physics Branches of physics Astrophysics Radiative transfer Thermal bremsstrahlung
2026-10-20  0 By others on same topic  0 Discussions Create my own version
For a uniform ionized hydrogen column with known temperature and fixed projected angular area, free-free brightness and optical depth depend on EM=ne2​L. The displayed rescaling leaves the whole ideal spectrum unchanged. density and path length cannot be separated without additional information. A known geometry/distance, or a distinct column diagnostic proportional to ne​L, can break the degeneracy; gas clumping factor and temperature structure complicate that inference.

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  • Past exam of the frontiers of Observational Astrophysics course of the University of Cambridge / 2014 / Paper 1 / 3 / d / Solution

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