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- W2071799796 abstract "It has been stated in a previous communication that a preliminary reduction of the Roman observations of prominences, observed on the sun’s limb by Tacchini, indicated that, in addition to main epochs of maxima and minima of prominences coinciding in time with those of the maxima and minima of the total spotted area, there are also prominent subsidiary maxima and minima. One of us has pointed out in a recent communication to the Académie des Sciences that a comparison of the frequency of prominences visible in each solar latitude with the frequency of the most intense magnetic storms, indicated that ( a ) magnetic storms classed as “great” by Ellis, and the greatest prominence activity near the poles of the sun occurred at the same time; and ( b ) that the curve of general magnetic activity was nearly the same as that of the prominences observed near the solar equator." @default.
- W2071799796 created "2016-06-24" @default.
- W2071799796 date "1903-06-30" @default.
- W2071799796 modified "2023-10-18" @default.
- W2071799796 title "The relation between solar prominences and terrestrial magnetism" @default.
- W2071799796 doi "https://doi.org/10.1098/rspl.1902.0093" @default.
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