Global and Sequential Imaging Observation of the Earth's Plasmasphere by PHOENIX Onboard EQUULEUS

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Masaki Kuwabara, Kazuo Yoshioka, Reina Hikida, Go Murakami, Ichiro Yoshikawa, Shintaro Nakajima, Ryota Fuse, Yosuke Kawabata, Ryu Funase
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Abstract

The Plasmaspheric Helium ion Observation by Enhanced New Imager in eXtreme ultraviolet (PHOENIX) onboard EQUilibriUm Lunar-Earth point 6U Spacecraft (EQUULEUS) performed global imaging observations of the Earth's plasmasphere from a meridian view. PHOENIX is a normal-incidence telescope designed to observe He II emission at 30.4 nm, consisting of a mirror coated with molybdenum and silicon multilayers, a thin metallic filter made of aluminum and carbon, and a microchannel plate detector. This paper provides an overview of the PHOENIX instrument, its in-flight calibration, and initial results of Earth observations. During in-flight calibration, it was found that stray light affected the data when the phase angle between the line of sight and the Sun was small, but a method for its removal was developed using stray light observations. The calibration results confirmed that PHOENIX is optimized for He II observation, with a sensitivity of 1.45 × 10 2 $1.45\times {10}^{-2}$ cts/s/pix/Rayleigh for He II. It was also demonstrated that PHOENIX is capable of capturing global images of the Earth's plasmasphere with an angular resolution of less than 0.19° and a temporal resolution of less than 1.5 hr. In May 2023, PHOENIX successfully conducted imaging observations of the Earth's plasmasphere while EQUULEUS was on its way to the Earth-Moon Lagrange point 2, revealing the density structure along the dipole-shaped magnetic field lines. Furthermore, the shrinkage of the plasmasphere due to geomagnetic disturbances was captured. This marks the first global imaging of the Earth's plasmasphere using an ultra-small instrument.

Abstract Image

利用EQUULEUS上的PHOENIX对地球等离子层进行全球和序列成像观测
EQUilibriUm Lunar-Earth point 6U Spacecraft(EQUULEUS)上的等离子体氦离子极紫外增强新成像仪(PHOENIX)对地球等离子体进行了子午线全球成像观测。PHOENIX 是一台正常入射望远镜,设计用于观测波长为 30.4 纳米的 He II 发射,它由一面镀有钼和硅多层膜的镜子、一个由铝和碳制成的薄金属滤光片以及一个微通道板探测器组成。本文概述了 PHOENIX 仪器、其飞行中校准以及地球观测的初步结果。在飞行校准过程中发现,当视线与太阳之间的相位角较小时,杂散光会对数据产生影响,但利用杂散光观测结果开发出了去除杂散光的方法。校准结果证实,PHOENIX 是观测 He II 的最佳选择,对 He II 的灵敏度为 1.45 × 10 - 2 1.45times {10}^{-2}$ cts/s/pix/Rayleigh。此外还证明 PHOENIX 能够捕捉地球等离子体的全球图像,其角度分辨率小于 0.19°,时间分辨率小于 1.5 小时。2023 年 5 月,当 EQUULEUS 正在前往地月拉格朗日点 2 的途中时,PHOENIX 成功地对地球质球进行了成像观测,揭示了沿偶极子形磁场线的密度结构。此外,还捕捉到了地磁扰动导致的质球收缩。这标志着首次使用超小型仪器对地球质球进行全球成像。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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