Characteristics of Field‐Aligned Low‐Energy Oxygen (FALEO) Events Based on Arase LEP‐i Observations

Abstract This study investigates field‐aligned low‐energy oxygen (FALEO) ions observed by the Arase satellite during 2020–2023. Using 4 years of data from the low‐energy particle experiment ion mass analyzer and magnetic field investigation instruments, we identified 90 energy‐dispersed FALEO events and our analysis reveals several key findings: (a) FALEO ions exhibit field‐aligned motion, appearing parallel to the magnetic field below the equator and anti‐parallel above it (b) the stop energy of nightside FALEO ions increases with L ‐value but decreases at low L ‐value during the high K p values, (c) unidirectional FALEO events occur primarily between 18 magnetic local time (MLT) and 08 MLT, peaking near 00 MLT, (d) bidirectional events are found between 22 and 10 MLT, with a broad maximum around 06 MLT, (e) for the first time, using Arase bidirectional FALEO events are observed on the dawnside magnetosphere within 06–10 MLT, and (f) most of the dawnside FALEO events are associated with geomagnetic storms, indicating a strong link to enhanced geomagnetic activity. These findings suggest the existence of a previously unrecognized dawnside source of FALEO ions in addition to the well‐established nightside source. The presence of such events on the dawnside may impact dayside reconnection processes and affect the global magnetospheric convection.

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Journal
Journal of Geophysical Research Space Physics
Published
2026-02-24
DOI
https://doi.org/10.1029/2025ja034541
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
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article

Characteristics of Field‐Aligned Low‐Energy Oxygen (FALEO) Events Based on Arase LEP‐i Observations

Kazushi Asamura, Trunali Shah, Masahito Nose, N. Kitamura et al.
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
article

Characteristics of Field‐Aligned Low‐Energy Oxygen (FALEO) Events Based on Arase LEP‐i Observations

Kazushi Asamura, Trunali Shah, Masahito Nose, N. Kitamura, K. Yamamoto, A. Matsuoka, Y. Miyoshi, M. Teramoto, I. Shinohara, B. Veenadhari
article en

Abstract

Abstract This study investigates field‐aligned low‐energy oxygen (FALEO) ions observed by the Arase satellite during 2020–2023. Using 4 years of data from the low‐energy particle experiment ion mass analyzer and magnetic field investigation instruments, we identified 90 energy‐dispersed FALEO events and our analysis reveals several key findings: (a) FALEO ions exhibit field‐aligned motion, appearing parallel to the magnetic field below the equator and anti‐parallel above it (b) the stop energy of nightside FALEO ions increases with L ‐value but decreases at low L ‐value during the high K p values, (c) unidirectional FALEO events occur primarily between 18 magnetic local time (MLT) and 08 MLT, peaking near 00 MLT, (d) bidirectional events are found between 22 and 10 MLT, with a broad maximum around 06 MLT, (e) for the first time, using Arase bidirectional FALEO events are observed on the dawnside magnetosphere within 06–10 MLT, and (f) most of the dawnside FALEO events are associated with geomagnetic storms, indicating a strong link to enhanced geomagnetic activity. These findings suggest the existence of a previously unrecognized dawnside source of FALEO ions in addition to the well‐established nightside source. The presence of such events on the dawnside may impact dayside reconnection processes and affect the global magnetospheric convection.

Journal of Geophysical Research Space PhysicsVol. 131(3)
Kyushu Institute of Technology (JP), Kyoto University (JP), Japan Aerospace Exploration Agency (JP), Nagoya City University (JP), Institute of Space and Astronautical Science (JP), Nagoya University (JP)
Affordable and clean energy
Openalex Percentile: Top 32%
Ionosphere and magnetosphere dynamics
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Characteristics of Field‐Aligned Low‐Energy Oxygen (FALEO) Events Based on Arase LEP‐i Observations — Kazushi Asamura, Trunali Shah, et al. · Journal of Geophysical Research Space Physics (2026) | TGRS Research Map | TGRS