电离层-磁层系统N+观测综述

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Frontiers in Astronomy and Space Sciences Pub Date : 2023-10-04 DOI:10.3389/fspas.2023.1224659
Raluca Ilie, Mei-Yun Lin, Muhammad Fraz Bashir, Abhiraj Majumder
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引用次数: 0

摘要

除了O +和其他重离子外,大多数研究还没有考虑和评估整个电离层-磁层系统中N +离子的输运和通电。近地等离子体中N +存在的有限观测记录,部分原因是由于仪器在区分相似质量的离子种类方面的限制,掩盖了它对近地等离子体的重要贡献。这封信回顾了最值得注意的N +离子观测,从Sputnik III在电离层的早期低空测量到增强型极流探测器(e-POP)任务报告的测量。现有的观测资料表明,氮离子是氧离子外流的恒定伴侣,其丰度随季节、太阳周期、一天中的时间和地磁活动而变化。电离层-磁层系统中氮存在的有力记录提出了离子组成的问题,并且在解释当前任务中的O +测量值时需要谨慎。
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A review of N+ observations in the ionosphere-magnetosphere system
Most studies have yet to consider and assess the transport and energization of N + ions throughout the ionosphere-magnetosphere system, in addition to that of O + and other heavy ion species. The limited observational record of N + presence in near-Earth plasma, partly due to instrument limitations to distinguish ion species of similar masses, has obscured its significant contribution to the near-Earth plasma. This letter reviews the most notable observations of N + ions, starting from the early low altitude measurements from Sputnik III in the ionosphere to the measurements reported by the Enhanced Polar Outflow Probe (e-POP) mission. The available observational data set suggests that nitrogen ions are constant companions of outflowing oxygen ions, and their abundances vary with season, solar cycle, time of day, and geomagnetic activity. This strong record of nitrogen presence in the ionosphere-magnetosphere system raises the question of ionic composition and the need for caution when interpreting O + measurements from current missions.
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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