Abstract
MANY astrophysical problems, for example, Zeeman-effect studies of the solar disk and the structure of some of the Fraunhofer lines, necessitate a very high resolving power, of the order of 106, for the spectrographic equipment.
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References
Tolansky, S., Physica, 12, 650 (1946).
Banning, M., J. Opt. Soc. Amer., 792 (1947).
Dufour, Ch., Le Vide, Nos. 16–17, 480 (1948).
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JARRETT, A. Production of a High Resolving Power by means of Multilayer Coatings. Nature 169, 790 (1952). https://doi.org/10.1038/169790a0
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DOI: https://doi.org/10.1038/169790a0
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