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- W2103697400 abstract "Examination of a relationship found between intense (3 +) solar flares within the central zone of the Sun's disk and subsequent geomagnetic activity has been extended to less intense flares (3 and 2). With flares of intensity 3 there is a small statistical rise of geomagnetic activity within a few days of the mean flare; in individual cases the disturbance is generally less intense and is certainly less probable than for flares 3 +. There is no perceptible rise of geomagnetic activity after the mean flare of intensity 2. Some distinctive flares 3 are tabulated for comparison with the most intense flares dealt with in the first paper. Radio fade-out data confirm in a general way a small statistical rise of geomagnetic activity within a few days after the mean fade-out, but the results are less definitive than those from the solar flare data." @default.
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- W2103697400 date "1944-02-01" @default.
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- W2103697400 title "Solar Flares and Magnetic Storms (Second Paper)" @default.
- W2103697400 doi "https://doi.org/10.1093/mnras/104.1.4" @default.
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