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- W2036554002 abstract "A novel design of a rf afterglow source of the oxygen forbidden lines at 630.0 and 557.7 nm for use in thermospheric dynamics studies is presented. With a repetitive discharge-afterglow excitation cycle, the source yields adequate afterglow intensities of the OI lines that are sufficiently free of background continuum for use in Fabry-Perot interferometer measurements of spectral line profiles. These lines provide accurate zero-velocity references in Fabry-Perot determinations of Doppler shifts in the OI thermospheric lines. The design considerations for the rf source are described, together with its preparation and filling by an ultrahigh-vacuum gas-handling system. Examples are given of the source's output spectrum, as measured by a grating spectrometer, and its spectral line profiles, as determined by a Fabry-Perot interferometer. Comparative interferometry between the OI afterglow source lines and nearby (within approximately 0.01-0.02-nm) lines from hollow-cathode sources illustrates the means of establishing secondary reference sources in cases in which the primary OI afterglow source is not available." @default.
- W2036554002 created "2016-06-24" @default.
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- W2036554002 date "2002-10-20" @default.
- W2036554002 modified "2023-09-23" @default.
- W2036554002 title "Oxygen 6300- and 5577-nm line source for thermospheric dynamics studies" @default.
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- W2036554002 doi "https://doi.org/10.1364/ao.41.006499" @default.
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