Abstract
MAY I venture to suggest that quite possibly something of value might be obtained by observing the sun during totality with a spectroscope of reasonable dispersive power (say four or five prisms) without a collimator, or even simply with one of the so-called meteor spectroscopes.
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YOUNG, C. The Solar Spectrum. Nature 4, 445 (1871). https://doi.org/10.1038/004445a0
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DOI: https://doi.org/10.1038/004445a0
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