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- W1988777725 abstract "It is believed that spectroheliograms taken in the center of the Hα-line show us the solar atmosphere at the highest level observable. On such exposures the chromosphere has a fine granular structure resembling the skin of an orange. Near large spot-groups, however, it is drawn out into long filaments, indicating the presence of an extensive field of force. These filaments often remind us strongly of the arrangement of iron filings around a bar-magnet, or the lines of flow in a vortex." @default.
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- W1988777725 date "1940-08-01" @default.
- W1988777725 modified "2023-10-17" @default.
- W1988777725 title "The Nature of Solar Hydrogen Vortices" @default.
- W1988777725 doi "https://doi.org/10.1086/125190" @default.
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