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The Ultraviolet Spectrum of the Sun from V-2 Rockets
Phys. Rev. 73, 877 – Published 15 April, 1948
DOI: https://doi.org/10.1103/PhysRev.73.877
Abstract
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 A, and traces are evident as far as A. A tentative list of identified lines is given. The MgII resonance doublet at A 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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