Very Small Intensity of the Red OI Triplet during the Auroral Displays of September 14 16

Details Very Small Intensity of the Red OI Triplet during the Auroral Displays of September 14 16 Very Small Intensity of the Red OI Triplet during the Auroral Displays of September 14 16

Nov 1938

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1938natur.142..831v&link_type=abstract

Nature, Volume 142, Issue 3601, pp. 831-832 (1938).

Physics

Scientific paper

IT has been shown in previous papers1,2 that the red aurora of type A owes its redness to the enhancement of the red OI-triplet (1D2 - 3P0,1,2) and that the relative intensity of this triplet and the frequency of the red auroras of type A seem to follow the sunspot frequency2,3. This rule was found to hold for spectrograms obtained since 1923 and up to the winter season 1937-38.

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