EUV complementary instrumentation for SIMURIS

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Extreme Ultraviolet Radiation, High Resolution, High Temperature, Solar Atmosphere, Solar Corona, Solar Instruments, Spaceborne Telescopes, Ultraviolet Telescopes, X Ray Telescopes, Imaging Spectrometers, Interferometry, Mission Planning, Requirements, Spatial Resolution, X Ray Imagery

Scientific paper

The design, instrument requirements, and scientific objectives of the X-ray Ultraviolet Imager, a normal incidence telescope with mirrors coated with multilayers, designed to provide observations at the sub arcsecond spatial resolution in the X-ray/XUV domain are considered. The instrument could provide high resolution imaging of the high temperature solar atmosphere. The X-ray Ultraviolet Imager is a multimirror telescope with a number of independent channels imaging at different wavelengths. Each channel is optimized to select a narrow spectroscopic band in the 40 to 400 A region, which is rich in diagnostic lines formed at quite different temperatures. The number of channels is chosen in such a way to cover the entire temperature range observed on the solar outer atmosphere, from 100,000 to about 10(exp 7) K. The instrument consists of two complementary imaging systems: a high resolution telescope with subarcsecond resolution on a limited field of view; and a wide field telescope imaging the whole Sun within 2.5 solar radii from Sun center.

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