The visible spectro-polarimeter for the advanced technology solar telescope

Bibcode
2005SPIE.5901...60E
DOI
10.1117/12.618459
Elmore, D. F.; Socas-Navarro, H.; Card, G. L.; Streander, K. V.
Bibliographical reference

Solar Physics and Space Weather Instrumentation. Edited by Fineschi, Silvano; Viereck, Rodney A. Proceedings of the SPIE, Volume 5901, pp. 60-66 (2005).

Advertised on:
8
2005
Number of authors
4
IAC number of authors
0
Citations
9
Refereed citations
8
Description
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.
Type
Non-refereed

It may interest you

  • Non-refereed
    An overview of the preliminary optical design of the European Solar Telescope (EST)
    The European Solar Telescope (EST) is a 4-m class-solar telescope that will become part of the next generation of groundbased facilities. Located at the "Observatorio del Roque de los Muchachos" in La Palma (Spain), it will be aimed to study the magnetic connectivity of the solar atmosphere with high spatial and temporal resolution. The EST optical
    Belío-Asin, Marta et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..2GB
    Citations
    0
  • Non-refereed
    ANDES, the high resolution spectrograph for the ELT: science goals, project overview, and future developments
    The first generation of ELT instruments includes an optical-infrared high resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion Echelle Spectrograph). ANDES consists of three fibre-fed spectrographs ([U]BV, RIZ, YJH) providing a spectral resolution of ∼100,000 with a minimum simultaneous wavelength
    Marconi, A. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..13M
    Citations
    1
  • Non-refereed
    Shape and Mutual Orbit Modeling of Binary Near-Earth Asteroid 2020 BX<SUB>12</SUB>
    Approximately 15% of the near-Earth asteroid (NEA) population are estimated to be binary systems. 54 binaries have Arecibo radar observations; 2020 BX 12 is one of them. Discovered on January 27, 2020, by the Asteroid Terrestrial-impact Last Alert System (ATLAS) survey at Mauna Loa Observatory, 2020 BX 12 has an absolute magnitude of 20.6 and an
    Zambrano-Marin, Luisa Fernanda et al.

    Advertised on:

    10
    2024
    Bibcode
    2024DPS....5631203Z
    Citations
    0