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- W1964585812 abstract "Derivation of the intensity of the diffuse hydrogen Lyman-beta glow at 1025 A which is due to resonance scattering of the solar H I 1025 A line by interstellar and interplanetary hydrogen. Two sources of neutral hydrogen are considered: the local interstellar medium interacting with the solar system, and the dust deionization of the H(+) component of the solar wind. It is shown that if the dust geometrical factor is less than or equal to five quintillionths per cm, observations of backscattered Lyman-beta radiation will provide a unique determination of the density and temperature of the local interstellar medium." @default.
- W1964585812 created "2016-06-24" @default.
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- W1964585812 date "1973-12-01" @default.
- W1964585812 modified "2023-09-25" @default.
- W1964585812 title "Interplanetary Lyman-Beta Emissions" @default.
- W1964585812 doi "https://doi.org/10.1086/152573" @default.
- W1964585812 hasPublicationYear "1973" @default.
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