Design of narrow band XUV and EUV coronagraphs using multilayer optics

Details Design of narrow band XUV and EUV coronagraphs using multilayer optics Design of narrow band XUV and EUV coronagraphs using multilayer optics

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991spie.1343..415w&link_type=abstract

IN: X-ray/EUV optics for astronomy, microscopy, polarimetry, and projection lithography; Proceedings of the Meeting, San Diego,

Astronomy and Astrophysics

Astronomy

Coronagraphs, Extreme Ultraviolet Radiation, Narrowband, Solar Corona, Solar Spectra, Emission Spectra, Imaging Techniques, Line Spectra, Ultraviolet Astronomy

Scientific paper

A novel approach to the study of the solar corona is described, which enables observation of the soft X-ray (XUV), EUV, and FUV emission of the highly ionized ions present in the corona. The principal advantage of this approach is a relatively low contrast between the innner corona and the solar disk at the wavelengths involved; the contrast between coronal visible light and the XUV or EUV light is about 1. The design and the anticipated performances of the XUV and EUV coronagraphs using normal incidence multilayer optics are described.

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