18 August 2005 The visible spectro-polarimeter for the advanced technology solar telescope
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The mission of the ATST visible spectro-polarimeter (ViSP) is to provide precision measurements of the full state of polarization (Stokes parameters) simultaneously at diverse wavelengths in the visible spectrum and fully resolve (or nearly so) the profiles of spectrum lines originating in the solar atmosphere. We present the instrument science requirements, their flow down to instrument specifications, and a preliminary ViSP design. The ViSP spectrograph allows for reconfiguration while maintaining an immediately selectable configuration. We describe how the ViSP will utilize the ATST polarimetry facility.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
D. F. Elmore, D. F. Elmore, H. Socas-Navarro, H. Socas-Navarro, G. L. Card, G. L. Card, K. V. Streander, K. V. Streander, "The visible spectro-polarimeter for the advanced technology solar telescope", Proc. SPIE 5901, Solar Physics and Space Weather Instrumentation, 590106 (18 August 2005); doi: 10.1117/12.618459; https://doi.org/10.1117/12.618459


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