SO/PHI-HRT Polarimetry
SO/PHI is the Polarimetric Helioseismic Imager on board the Solar Orbiter; one of the 6 remote sensing instruments. It is a spectropolarimeter: it takes images of the Sun at very distinct wavelengths and different polarisations. From these images, the full vector magnetic field at the solar surface,...
Main Authors: | , |
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Format: | Still Image |
Language: | unknown |
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Zenodo
2021
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Subjects: | |
Online Access: | https://dx.doi.org/10.5281/zenodo.4663705 https://zenodo.org/record/4663705 |
Summary: | SO/PHI is the Polarimetric Helioseismic Imager on board the Solar Orbiter; one of the 6 remote sensing instruments. It is a spectropolarimeter: it takes images of the Sun at very distinct wavelengths and different polarisations. From these images, the full vector magnetic field at the solar surface, as well as the LOS (Line Of Sight) velocity, can be inferred. To produce reliable magnetograms and dopplergrams the polarimetry of SO/PHI-HRT has to be calibrated. This poster describes the preliminary results that characterise its polarimetric properties. : {"references": ["Rodr\u00edguez, J. Blanco, et al. \"SOPHISM: an end-to-end software instrument simulator.\" The Astrophysical Journal Supplement Series 237.2 (2018): 35.", "Solanki, Sami K., et al. \"The polarimetric and helioseismic imager on solar orbiter.\" Astronomy & Astrophysics 642 (2020): A11.", "Su\u00e1rez, D. Orozco, and J. C. Del Toro Iniesta. \"The usefulness of analytic response functions.\" Astronomy & Astrophysics 462.3 (2007): 1137-1145."]} |
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