We present here experimental evidence of the filling in of Fraunhofer lines at 5893 and 7699 Å by scattering from terrestrial surfaces. This effect is shown to vary with the scattering angle and with the nature of the surfaces involved. Consequences on dayglow data and on lunar luminescence studies will be considered in future publications.
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Marie‐Lise Chanin (1975) studied this question.
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