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      Towards imaging-spectro-polarimetry of solar flares in the X-rays

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          Abstract

          X-ray polarimetry of solar flares is still a not well established field of observation of our star. Past polarimeters were not able to measure with a high significance the polarization in X-rays from solar flares. Moreover, they had no imaging capabilities and measured only the polarization by integrating on all the image of the source. We propose a mission concept based on a gas photoelectric polarimeter, coupled with multilayer lobster-eye optics, to perform imaging-spectro-polarimetry of solar flares while monitoring the entire solar disc.

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          Author and article information

          Journal
          04 July 2024
          Article
          2407.04749
          0b757b3b-86bc-4619-bcc0-34017abe6d2a

          http://creativecommons.org/licenses/by-nc-sa/4.0/

          History
          Custom metadata
          Paper No. 13093-311
          Proceeding of SPIE Conference "Astronomical Telescopes+ Instrumentation", Yokohama (Japan), 16-21 June 2024
          astro-ph.IM astro-ph.SR

          Instrumentation & Methods for astrophysics,Solar & Stellar astrophysics

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