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- W2004187408 abstract "A Fabry-Perot instrument has been used as a spectrometer with a resolving power of about 10,000 to identify the twilight helium emission at 10,830 Å. Photometric measurements of the atmospheric helium emission were also obtained with the Fabry-Perot. Large fluctuating enhancements were recorded in the zenith while visible aurora was present in the sky. The twilight emission intensities are consistent with previous measurements and the rate at which the emission intensity decays during twilight is consistent with the excitation of triplet helium atoms by collision of photoelectrons with ground state helium atoms, followed by resonance scattering." @default.
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- W2004187408 date "1969-04-01" @default.
- W2004187408 modified "2023-09-26" @default.
- W2004187408 title "An identification of twilight helium 10,830 Å emission with increased resolution and preliminary photometric measurements" @default.
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- W2004187408 doi "https://doi.org/10.1016/0032-0633(69)90191-3" @default.
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