The Ultraviolet Spectrum of the Sun from V-2 Rockets

Details The Ultraviolet Spectrum of the Sun from V-2 Rockets The Ultraviolet Spectrum of the Sun from V-2 Rockets

Apr 1948

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1948phrv...73..877h&link_type=abstract

Physical Review, vol. 73, Issue 8, pp. 877-884

Physics

14

Scientific paper

Spectra of the sun have been obtained from V-2 rockets at heights up to 155 km. A grating spectrograph was used giving a dispersion of 34A/mm. The ultraviolet spectrum of the sun obtained extends down to λ=2300A, and traces are evident as far as λ=2230A. A tentative list of identified lines is given. The MgII resonance doublet at λ=2800A is observed to have emission centers in both absorption components. The intensity of this emission is estimated as about 10 percent that of the adjacent continuum.

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