Calculation of the intensity of light diffracted by outer eclipsing disks of a coronograph

Details Calculation of the intensity of light diffracted by outer eclipsing disks of a coronograph Calculation of the intensity of light diffracted by outer eclipsing disks of a coronograph

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977opsp...42..559l&link_type=abstract

Optika i Spektroskopiia, vol. 42, Mar. 1977, p. 559-561. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Photography, Coronagraphs, Luminous Intensity, Solar Instruments, Wave Diffraction, Balloon-Borne Instruments, Disks (Shapes), Monochromatic Radiation, Point Sources, Satellite-Borne Instruments, Screen Effect

Scientific paper

Eclipsing disks are generally used to reduce the amount of scattered
light in a satellite- or balloon-borne solar coronograph. The paper
presents a method for calculating the intensity of light difracted by
the disks of a coronograph, based on the use of the Kirchhoff integral
in the Rubinovich representation.

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