Coronal Photopolarimetry with the LASCO-C2 Coronagraph over 24 Years [1996-2019] -- Application to the K/F Separation and to the Determination of the Electron Density

Abstract

We present an in-depth characterization of the polarimetric channel of the Large-Angle Spectrometric COronagraph LASCO-C2 onboard the Solar and Heliospheric Observatory (SoHO). The polarimetric analysis of the white-light images makes use of polarized sequences composed of three images obtained though three polarizers oriented at +60°, 0° and -60°, complemented by a neighboring unpolarized image, and relies on the formalism of Mueller. The Mueller matrix characterizing the C2 instrument was obtained through extensive ground-based calibrations of the optical components and global laboratory tests. Additional critical corrections were derived from in-flight tests relying prominently on roll sequences and on consistency criteria, mainly the tangential direction of polarization. Our final results encompass the characterization of the polarization of the white-light corona, of its polarized radiance, of the two-dimensional electron density, and of the K-corona over two solar cycles. They are in excellent agreement with measurements obtained at several solar eclipses except for slight discrepancies affecting the innermost part of the C2 field-of-view, probably resulting from an imperfect removal of the bright diffraction fringe surrounding the occulter.

72 pages, 51 figures

References in corpus (2)

• Time-Dependent Tomographic Reconstruction of the Solar Corona
• Imaging Polarimetry of the 2017 Solar Eclipse with the RIT Polarization Imaging Camera

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• Restitution of the K and F Components of the Solar Corona from LASCO-C2 Images over 24 Years [1996--2019]
• Polarimetric Studies of a Fast Coronal Mass Ejection
• Polarization of the Corona Observed During the 2017 and 2019 Total Solar Eclipses
• A Simple Radial Gradient Filter for Batch-Processing of Coronagraph Images