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Interferometer Measurements of the Red Auroral Line 6300

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Abstract

WE know that considerable interest is attached to certain auroral lines in the region 6300–6400 A. Thus the enhancement of one or more of these lines is responsible for a particular type of red-coloured auroræ1,3 and, according to the interpretation of the strong green line by McLennan and his collaborators, the OI-triplet (1D23P0,1,2) should appear in this region.

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References

  1. L. Vegard, NATURE, 117, 356; 1926.

    Article  Google Scholar 

  2. L. Vegard, Geophys. Publ., 9, No. 11; 1932.

  3. L. Vegard, Z. Phys., 75, 30; 1932.

    Article  CAS  ADS  Google Scholar 

  4. L. Vegard, Geophys. Publ., 10, No. 4; 1933.

  5. L. Vegard and L. Harang, Geophys. Publ., 10, No. 5; 1933.

  6. L. Vegard and L. Harang, Geophys. Publ., 11, No. 1; 1934.

  7. J. J. Hopfield, Phys. Rev., 37, 160; 1931.

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HARANG, L., VEGARD, L. Interferometer Measurements of the Red Auroral Line 6300. Nature 135, 542–543 (1935). https://doi.org/10.1038/135542b0

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