The Multi-Spectral Solar Telescope Array: Observations of Loop Structures in the Solar Atmosphere.

Physics – Optics

Scientific paper

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Scientific paper

The emergence of multilayer coated optics technology has offered solar physics an unprecedented opportunity to obtain images of the corona at spatial resolutions previously unattainable. A previous demonstration of the efficacy of this technique, the Stanford/Marshall Space Flight Center (NASA) Rocket X-ray Spectroheliograph, rendered full disk images of the solar corona between 1 and 2 arc seconds spatial resolution and spanning more than 3 solar radii. Further images were obtained during the 1991 flight of the Multi -Spectral Solar Telescope Array (MSSTA) at comparable or higher resolutions (<=q1 arc second) and spanning a broader range of the Soft X-ray/EUV spectrum. This thesis describes the development of the MSSTA and presents a preliminary analysis of some plasma loops observed in the corona.

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