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The last observable line in hydrogen emission spectrum

โœ Scribed by L. N. Kurochka; L. B. Ribko

Publisher
Springer
Year
1978
Tongue
English
Weight
480 KB
Volume
57
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis

It is shown that outside continuous solar spectrum or diffused solar light in the Earth's atmosphere substantially reduces the contrast and quality of observable emission lines in the hydrogen spectrum..A formula is obtained which enables the electron concentration in hydrogen plasma to be determined by the last observable line with due account for outside (spurious) continuous spectrum.

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