Out-of-eclipse externally occulted coronagraphs

Details Out-of-eclipse externally occulted coronagraphs Out-of-eclipse externally occulted coronagraphs

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...80l&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, May-June 1987, p. 80-87. In Russian.

Physics

Coronagraphs, Diffraction Radiation, Solar Eclipses, Solar Flux Density, Image Processing, Stellar Occultation, Stellar Spectrophotometry

Scientific paper

A theoretical estimate is made of the diffracted solar light intensity in the primary focal plane of a coronagraph externally occulted by a continuous screen. The screen has an opening (scanning aperture) that is peculiar in terms of its shape and arrangement; it views a radial portion of the solar corona. The use of this type of highly efficient external occulter makes it possible to dispense with the Lyot scheme.

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