Energization of Outflowing O <sup>+</sup> by Double‐Pickup in Earthward Plasma Jets From Lobe Reconnection and in Magnetosheath Flow

Abstract This study reports a case of energetic oxygen ions (O + ) with energies around 20 keV, observed at the high‐latitude magnetopause during lobe reconnection. In the adjacent lobe/mantle region, another O + beam, outflowing directly from the ionosphere, was observed with energies of approximately 1 keV. The energies and velocity distribution functions of O + indicate that the observed 20 keV O + are accelerated through double pickup processes. A test particle simulation shows that the outflowing O + ions are first picked up by an earthward plasma jet from lobe reconnection and energized up to ∼3 keV. Subsequently, they are picked up by the tailward magnetosheath flow and further energized up to ∼15 keV. A strong gradient in the convection electric field at the magnetopause current layer, which tends to form during lobe reconnection, is likely to play an important role in the generation of energetic O + .

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Journal
Geophysical Research Letters
Published
2025-08-04
DOI
https://doi.org/10.1029/2025gl115236
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

Energization of Outflowing O + by Double‐Pickup in Earthward Plasma Jets From Lobe Reconnection and in Magnetosheath Flow

Iannis S Dandouras, S. Taguchi, H. Nilsson, Haruto Koike et al.
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
article

Energization of Outflowing O + by Double‐Pickup in Earthward Plasma Jets From Lobe Reconnection and in Magnetosheath Flow

Iannis S Dandouras, S. Taguchi, H. Nilsson, Haruto Koike, M. Yamauchi
article en

Abstract

Abstract This study reports a case of energetic oxygen ions (O + ) with energies around 20 keV, observed at the high‐latitude magnetopause during lobe reconnection. In the adjacent lobe/mantle region, another O + beam, outflowing directly from the ionosphere, was observed with energies of approximately 1 keV. The energies and velocity distribution functions of O + indicate that the observed 20 keV O + are accelerated through double pickup processes. A test particle simulation shows that the outflowing O + ions are first picked up by an earthward plasma jet from lobe reconnection and energized up to ∼3 keV. Subsequently, they are picked up by the tailward magnetosheath flow and further energized up to ∼15 keV. A strong gradient in the convection electric field at the magnetopause current layer, which tends to form during lobe reconnection, is likely to play an important role in the generation of energetic O + .

Geophysical Research LettersVol. 52(15)
Centre National de la Recherche Scientifique (FR), Swedish Institute of Space Physics (SE), Kyoto University (JP), Centre National d'Études Spatiales (FR), Institut de Recherche en Astrophysique et Planétologie (FR)
Centre National d’Etudes Spatiales, Japan Society for the Promotion of Science
Openalex Percentile: Top 86%
Ionosphere and magnetosphere dynamics
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