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ICON极紫外光谱仪的飞行性能。

In-Flight Performance of the ICON EUV Spectrograph.

作者信息

Korpela Eric J, Sirk Martin M, Edelstein Jerry, McPhate Jason B, Tuminello Richard M, Stephan Andrew W, England Scott L, Immel Thomas J

机构信息

Space Sciences Laboratory, University of California, Berkeley, CA USA.

Aerospace & Ocean Engineering, Virginia Tech, Blacksburg, VA USA.

出版信息

Space Sci Rev. 2023;219(3):24. doi: 10.1007/s11214-023-00963-1. Epub 2023 Mar 28.

Abstract

We present in-flight performance measurements of the Ionospheric Connection Explorer EUV spectrometer, , a wide field ( ) extreme ultraviolet (EUV) imaging spectrograph designed to observe the lower ionosphere at tangent altitudes between 100 and 500 km. The primary targets of the spectrometer, which has a spectral range of 54-88 nm, are the Oii emission lines at 61.6 nmand 83.4 nm. In flight calibration and performance measurement has shown that the instrument has met all of the science performance requirements. We discuss the observed and expected changes in the instrument performance due to microchannel plate charge depletion, and how these changes were tracked over the first two years of flight. This paper shows raw data products from this instrument. A parallel paper (Stephan et al. in Space Sci. Rev. 218:63, 2022) in this volume discusses the use of these raw products to determine O density profiles versus altitude.

摘要

我们展示了电离层连接探测器极紫外光谱仪的飞行性能测量结果,这是一台宽视场( )极紫外(EUV)成像光谱仪,旨在观测100至500千米切向高度处的低层电离层。该光谱仪的光谱范围为54 - 88纳米,主要目标是61.6纳米和83.4纳米处的氧离子发射线。飞行校准和性能测量表明,该仪器已满足所有科学性能要求。我们讨论了由于微通道板电荷耗尽导致的仪器性能观测到的和预期的变化,以及在飞行的头两年中如何跟踪这些变化。本文展示了该仪器的原始数据产品。本卷中的一篇平行论文(Stephan等人,《空间科学评论》218:63,2022)讨论了如何使用这些原始产品来确定氧密度随高度的分布。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e1a9/10050024/81ed5a781f67/11214_2023_963_Fig1_HTML.jpg

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