REFOS:纳米卫星上的太阳软x射线分光光度计

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Anton Reva, Sergey Kuzin, Andrey Pertsov, Alexey Kirichenko, Sergey Dyatkov, Ivan Loboda, Viktor Chervinsky, Anton Kholodilov, Alexey Trifonov, Sergey Bogachev, Sergei Chumak
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引用次数: 0

摘要

在这项工作中,我们描述了REFOS仪器的设计和飞行性能(来自俄罗斯REntgenovskiy FOto Spectrometer;英文“x射线光光谱仪”)。REFOS是一种软x射线分光光度计,可记录全盘集成太阳光谱(“太阳作为恒星”)。它在脉冲-1纳米卫星上运行,该卫星于2023年6月24日发射。REFOS具有1.2 - 30 keV的光谱范围,5.9 keV时半最大(FWHM)分辨率为0.123 keV的标称全宽度,16秒的节奏。我们使用2023年12月31日21:55 UT发生的X5.0耀斑的光谱来说明仪器的飞行性能。对于这次耀斑,REFOS在其所有能量箱中都记录了一个有意义的信号。通过对GOES和REFOS通量的比较,修正了REFOS的光谱灵敏度。此外,我们根据连续体的形状评估校准的质量。观测到的连续谱可以用来诊断等离子体温度,观测到的光谱线可以用来研究镁、硅、硫、氩、钙、铁和镍的丰度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
REFOS: Solar Soft X-ray Spectrophotometer on Board Nanosatellite

In this work, we describe the design and flight performance of the REFOS instrument (from Russian REntgenovskiy FOto Spektrometr; in English “X-ray Photo Spectrometer”). REFOS is a soft X-ray spectrophotometer that registers full-disk integrated solar spectra (“Sun as a star”). It operates on board the Impulse-1 nanosatellite, which was launched on 24 June 2023. REFOS has a 1.2 – 30 keV spectral range, a 0.123 keV nominal full width at half-maximum (FWHM) resolution at 5.9 keV, and a cadence of 16 s. We illustrate the instrument flight performance using the spectra of the X5.0 flare that occurred on 31 December 2023 at 21:55 UT. For this flare, REFOS registered a meaningful signal in all of its energy bins. Based on a comparison between the GOES and REFOS fluxes, we corrected the REFOS spectral sensitivity. Additionally, we assessed the quality of the calibration based on the shape of the continuum. The observed continuum allows diagnosing the plasma temperature, and the observed spectral lines allow studying abundances of the Mg, Si, S, Ar, Ca, Fe, and Ni.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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