Development of Solar Flare X-ray Polarimeter with Micro-Pixel CMOS Sensors
Abstract
We are developing an X-ray polarimeter using micro-pixel CMOS sensors for solar flare X-ray polarimetry. The system consists of a 2.5-m pixel CMOS image sensor with a 12.812.8 mm imaging area and a readout system based on a Zynq System-on-Chip. While previous studies have validated this concept, no realistic feasibility studies have been conducted for the solar flare X-ray polarization observation. In this work, we performed polarization sensitivity measurements at synchrotron facilities. The results show that our polarimeter is sensitive to the X-ray polarization, exhibiting a modulation factor of 5-15% at an energy range of 6-22 keV. The measurements also determined the thickness of the sensitive layer to be approximately 5 m, and the thicknesses of the insensitive layers to be 0.8 m (Si), 2.1 m (SiO2), and 0.24 m (Cu). These measured thicknesses lead to a quantum efficiency of 3-4% at 10 keV. Based on these experimental evaluations, we estimated the sensitivity of the micro-pixel CMOS polarimeter system. We found that, when combined with a telescope with an effective area of 10 cm, this system can detect X-ray polarization with a polarization degree of a few percent for M-class flares.
Keywords
Cite
@article{arxiv.2509.03914,
title = {Development of Solar Flare X-ray Polarimeter with Micro-Pixel CMOS Sensors},
author = {Kouichi Hagino and Tatsuaki Kato and Toshiya Iwata and Masahiro Ichihashi and Hiroumi Matsuhashi and Gen Fujimoto and Riki Sato and Hirokazu Odaka and Noriyuki Narukage and Shota Arai and Takahiro Minami and Satoshi Takashima and Aya Bamba},
journal= {arXiv preprint arXiv:2509.03914},
year = {2025}
}
Comments
9 pages, 5 figures, Proceedings of SPIE 2025 Optics + Photonics, Astronomical Applications, Paper number 13625-43