Physics
Scientist
Geneve, Observatoire, Sauverny, Switzerland
Geneva Observatory, Sauverny, Switzerland
A comparison between the observed and predicted UV line blocking for blanketed model atmospheres of early type stars
Far-infrared solar brightness measured with a balloon-borne lamellar-grating interferometer
Far-infrared-solar imaging from a balloon-borne platform
Line blocking in the near ultraviolet spectrum of early type stars. I - Observed line blocking factors for 132 stars
On asymmetries of solar spectral lines
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