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- W2058474008 abstract "Wild (1952) and Kardaschev (1959) noted that atomic transitions between levels of very high quantum number, n , may give lines in the radio region, if the source has sufficiently low density. Gaseous nebulae or H II regions prove to be strong sources of such radiation and a number of the predicted lines have already been found, superposed on a background of continuous emission. Relativistic effects prove to be negligible. Doppler broadening must eventually include macroscopic motions as well as temperature effects. H. R. Griem (1966, unpublished) has shown that a proper treatment of ion and electron collisions replaces the linear Stark effect. However, a broadening still remains as the result of departure of the potential of the atom from a Coulomb field because of surrounding ions. The theory follows lines similar to those laid down by Debye and Huckel in their study of dilute electrolytes." @default.
- W2058474008 created "2016-06-24" @default.
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- W2058474008 date "1969-04-24" @default.
- W2058474008 modified "2023-09-27" @default.
- W2058474008 title "A discussion on infared astronomy - Radio emission from high-level transitions in hydrogen" @default.
- W2058474008 doi "https://doi.org/10.1098/rsta.1969.0020" @default.
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