A Generation Mechanism of Banded Plasmaspheric Hiss

Abstract As a unique structure of plasmaspheric hiss emissions, banded hiss waves generally consist of an upper band above ∼200 Hz, a lower band below ∼100 Hz and a power gap in between. However, the generation mechanism of banded hiss remains unclear. Here we present a representative event of bande...

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Main Authors: Junhu Dong, Binbin Ni, Zheng Xiang, Zhiyong Wu
Format: Article
Language:English
Published: Wiley 2025-04-01
Series:Geophysical Research Letters
Online Access:https://doi.org/10.1029/2024GL113809
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author Junhu Dong
Binbin Ni
Zheng Xiang
Zhiyong Wu
author_facet Junhu Dong
Binbin Ni
Zheng Xiang
Zhiyong Wu
author_sort Junhu Dong
collection DOAJ
description Abstract As a unique structure of plasmaspheric hiss emissions, banded hiss waves generally consist of an upper band above ∼200 Hz, a lower band below ∼100 Hz and a power gap in between. However, the generation mechanism of banded hiss remains unclear. Here we present a representative event of banded hiss co‐existing in both the plasmaspheric plume structure and the plasmasphere. The wave Poynting flux measurements and linear instability analysis suggest that banded hiss can be generated in the equatorial plume region. The ray tracing simulations further show that the plume structure enables banded hiss to propagate along the plasma density crest to higher latitudes, followed by the penetration into the plasmasphere. Our data analysis and modeling efforts provide a plausible mechanism for the generation of banded hiss, and also highlight the significant role of plume structure in the generation and propagation of magnetospheric whistler‐mode waves.
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publishDate 2025-04-01
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series Geophysical Research Letters
spelling doaj-art-ca47fbbd04cb45768a5d15a14ad19aca2025-08-20T03:44:25ZengWileyGeophysical Research Letters0094-82761944-80072025-04-01528n/an/a10.1029/2024GL113809A Generation Mechanism of Banded Plasmaspheric HissJunhu Dong0Binbin Ni1Zheng Xiang2Zhiyong Wu3School of Earth and Space Science and Technology Wuhan University Wuhan ChinaSchool of Earth and Space Science and Technology Wuhan University Wuhan ChinaSchool of Earth and Space Science and Technology Wuhan University Wuhan ChinaNational Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences University of Science and Technology of China Hefei ChinaAbstract As a unique structure of plasmaspheric hiss emissions, banded hiss waves generally consist of an upper band above ∼200 Hz, a lower band below ∼100 Hz and a power gap in between. However, the generation mechanism of banded hiss remains unclear. Here we present a representative event of banded hiss co‐existing in both the plasmaspheric plume structure and the plasmasphere. The wave Poynting flux measurements and linear instability analysis suggest that banded hiss can be generated in the equatorial plume region. The ray tracing simulations further show that the plume structure enables banded hiss to propagate along the plasma density crest to higher latitudes, followed by the penetration into the plasmasphere. Our data analysis and modeling efforts provide a plausible mechanism for the generation of banded hiss, and also highlight the significant role of plume structure in the generation and propagation of magnetospheric whistler‐mode waves.https://doi.org/10.1029/2024GL113809
spellingShingle Junhu Dong
Binbin Ni
Zheng Xiang
Zhiyong Wu
A Generation Mechanism of Banded Plasmaspheric Hiss
Geophysical Research Letters
title A Generation Mechanism of Banded Plasmaspheric Hiss
title_full A Generation Mechanism of Banded Plasmaspheric Hiss
title_fullStr A Generation Mechanism of Banded Plasmaspheric Hiss
title_full_unstemmed A Generation Mechanism of Banded Plasmaspheric Hiss
title_short A Generation Mechanism of Banded Plasmaspheric Hiss
title_sort generation mechanism of banded plasmaspheric hiss
url https://doi.org/10.1029/2024GL113809
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