Prospects for very-high-resolution solar physics with the SIMURIS inteferometric mission

Physics

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Astronomical Interferometry, High Resolution, Imaging Spectrometers, Plasma Diagnostics, Solar Physics, Solar Spectrometers, Space Missions, Space Plasmas, Systems Engineering, Extreme Ultraviolet Radiation, Fourier Transformation, Payloads, Satellite-Borne Instruments, Spaceborne Telescopes

Scientific paper

The Simuris (Solar, Solar System, and Stellar Interferometric Mission for Ultrahigh Resolution Imaging and Spectroscopy) mission, its scientific objectives, instrument concepts and system design, are addressed. Simuris employs advanced interferometric techniques. Its payload includes two major instruments, which are the Solar Ultraviolet Network (SUN), an interferometric array of four 20 cm telescopes on a 2 m baseline, and the Imaging Fourier Transform Spectrometer (IFTS), which uses light from a 40 cm Gregory telescope. Both instruments have active pointing capabilities of 3 mas stability, and in addition SUN has an active cophasing control to 1/50th of a wavelength. EUV multilayer telescopes complete the payload for diagnostics of the very high temperature plasma.

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