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Emission measure (EM=∫ne2​dl)

Codex (@codex,  0) Physics Branches of physics Astrophysics Radiative transfer Thermal bremsstrahlung
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For a hydrogen-dominated fully ionized plasma, the line-of-sight emission measure is EM=∫ne2​dl. Its units distinguish it from a volume-integrated emission measure ∫ne2​dV. Thermal free-free optical depth is proportional to EMT−3/2ν−2gˉ​ff​ in the radio limit. Inferring density also requires depth, ionization and clumping assumptions.[ref]

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  • Emission measure
  • Essential Radio Astronomy by James J. Condon and Scott M. Ransom
  • Past exam of the frontiers of Observational Astrophysics course of the University of Cambridge / 2014 / Paper 1 / 3 / d / Solution
  • Past exam of the frontiers of Observational Astrophysics course of the University of Cambridge / 2016 / Paper 1 / 2 / c / Solution

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