Computer Science – Performance
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.0805c&link_type=abstract
American Astronomical Society, SPD meeting #42, #8.05; Bulletin of the American Astronomical Society, Vol. 43, 2011
Computer Science
Performance
Scientific paper
(this presentation is for the special ATST session of the SPD meeting)
The ViSP will be the slit-based spectro-polarimeter for the ATST. It is designed to be a wavelength versatile research instrument, multi-line capable (up to three lines simultaneously) between 380 and 900 nm, and providing high spectral, spatial, and temporal resolution, and large FOV, to satisfy the science needs of the solar community. The design effort has emphasized the high throughput of the instrument necessary for precision polarimetry science, and automated configurability, in order to increase the scientific opportunities of the instrument during daily operations. In this talk we present the design characteristics of the instrument, its expected performance, and an example of instrument configuration for a typical science case.
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