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- W2004604856 abstract "The declination results at Yerbanis showed rather large variations during the period of observation, but there was the same sharp increase in easterly declination, beginning about one hour before totality and reaching a maximum shortly after totality which was observed at Point Loma, California, by the Department of Terrestrial Magnetism.1 The apparent divergence from normal amounted to nearly five minutes of declination. This is an estimation based upon a comparison with the results at the Teoloyucan Observatory, since no comparison observations were taken at Yerbanis. Some of this large divergence may be due to the variation in temperature, which amounted to a decrease, followed by an increase, of nine degrees during the two hours of the eclipse period, due to the fact that the observations were made in the open air." @default.
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- W2004604856 date "1924-01-01" @default.
- W2004604856 modified "2023-09-25" @default.
- W2004604856 title "Note on a preliminary discussion of the magnetic observations made by the National Observatory of Mexico during the total solar eclipse of September 10, 1923" @default.
- W2004604856 doi "https://doi.org/10.1029/te029i003p00104" @default.
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