For a hydrogen-dominated fully ionized plasma, the line-of-sight emission measure is . Its units distinguish it from a volume-integrated emission measure . Thermal free-free optical depth is proportional to in the radio limit. Inferring density also requires depth, ionization and clumping assumptions.[ref]
Essential Radio Astronomy by James J. Condon and Scott M. Ransom. chapter 4, equations (4.57)–(4.58)
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