Abstract
BY the kindness of Mr. Todd we are enabled to give a drawing summarizing in a general way the phenomena observed during the last total eclipse. A comparison of this with the records at the two preceding sun-spot minima indicates very clearly that we have now very definite information concerning the corona of the sun as observed at the minimum period of sun-spots.
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LOCKYER, J. The Total Solar Eclipse of January 1 . Nature 39, 487–488 (1889). https://doi.org/10.1038/039487b0
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DOI: https://doi.org/10.1038/039487b0