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- W2054061673 abstract "The observed optimum frequency $f$ for long distance daylight communication averaged over the year during the period from 1923 to 1936 was found to vary with the yearly average relative sunspot number $s$ according to the relation $f=7.8{(s+12)}^{frac{1}{4}}$. The march of the sunspot curve from 1749 to 1935 suggests the possibility of greater sunspot numbers in coming solar cycles than the value $s=78$ which occurred at the 1928 maximum. By means of the $f$, $s$ relation, radio conditions for sunspot numbers from 100 to 160 are calculated." @default.
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- W2054061673 date "1936-07-01" @default.
- W2054061673 modified "2023-09-25" @default.
- W2054061673 title "Radio and the Sunspot Cycle" @default.
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- W2054061673 doi "https://doi.org/10.1103/physrev.50.45" @default.
- W2054061673 hasPublicationYear "1936" @default.
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