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Spectral Imager of the Solar Atmosphere: the First Extreme-Ultraviolet Solar Integral Field Spectrograph Using Slicers

Aerospace(2024)

Univ Durham | Univ Paris Saclay | Natl Res Council Italy | Univ Cambridge | Czech Acad Sci | Royal Observ Belgium | European Space Agcy | NASA Goddard Space Flight Ctr | Univ Liege ULiege | Univ Coll London | Spanish Space Solar Phys Consortium S3PC | Lockheed Martin Solar & Astrophys Lab | Univ Appl Sci & Arts Northwestern Switzerland

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Abstract
Particle acceleration, and the thermalisation of energetic particles, are fundamental processes across the universe. Whilst the Sun is an excellent object to study this phenomenon, since it is the most energetic particle accelerator in the Solar System, this phenomenon arises in many other astrophysical objects, such as active galactic nuclei, black holes, neutron stars, gamma ray bursts, solar and stellar coronae, accretion disks and planetary magnetospheres. Observations in the Extreme Ultraviolet (EUV) are essential for these studies but can only be made from space. Current spectrographs operating in the EUV use an entrance slit and cover the required field of view using a scanning mechanism. This results in a relatively slow image cadence in the order of minutes to capture inherently rapid and transient processes, and/or in the spectrograph slit ‘missing the action’. The application of image slicers for EUV integral field spectrographs is therefore revolutionary. The development of this technology will enable the observations of EUV spectra from an entire 2D field of view in seconds, over two orders of magnitude faster than what is currently possible. The Spectral Imaging of the Solar Atmosphere (SISA) instrument is the first integral field spectrograph proposed for observations at ∼180 Å combining the image slicer technology and curved diffraction gratings in a highly efficient and compact layout, while providing important spectroscopic diagnostics for the characterisation of solar coronal and flare plasmas. SISA’s characteristics, main challenges, and the on-going activities to enable the image slicer technology for EUV applications are presented in this paper.
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EUV spectroscopy,solar IFS,EUV slicers,image slicers,solar space mission,particle acceleration
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要点】:本文介绍了Spectral Imager of the Solar Atmosphere (SISA)——一种利用图像切片技术的首款极端紫外线太阳积分视场光谱仪,能够显著提高观测速度,实现对太阳大气中粒子加速和热化过程的快速、全面观测。

方法】:作者提出将图像切片技术与弯曲衍射光栅结合,设计出高效紧凑的布局,实现极端紫外线下的积分视场光谱观测。

实验】:SISA仪器的设计和开发正在进行中,旨在通过空间观测,利用图像切片技术提高EUV光谱观测的速度,当前实验的具体数据集名称未在摘要中提及。