Back to Search Start Over

Contribution of EMIC and Chorus Waves to the Formation of the Three‐Belt of Ultra‐Relativistic Electrons.

Authors :
Yang, Chang
Yue, Jiaxu
Yang, Hongming
He, Zhaoguo
Xiao, Fuliang
Zhang, Sai
He, Yihua
Liu, Si
Zhou, Qinghua
Gao, Zhonglei
Jin, Yuyue
Zhao, Hui
Johnston, Archie James
Source :
Journal of Geophysical Research. Space Physics; Dec2024, Vol. 129 Issue 12, p1-11, 11p
Publication Year :
2024

Abstract

The Earth's radiation belts are usually composed of an inner and an outer zone. Previous studies have reported a third belt of ultra‐relativistic electrons, but the mechanism requires to be further clarified. Here we report a very interesting feature of 3.4−6.3 $3.4-6.3$ MeV electrons during two storms in October 2018. During the October 7 storm the electrons in the region L≈3.5−5.0 $L\approx 3.5-5.0$ were quickly scattered by EMIC waves, leading to a storage ring left between L≈3.0−3.5 $L\approx 3.0-3.5$. Over the following days, due to the chorus‐driven acceleration, electron fluxes significantly increased in the region L>4 $L > 4$, consequently allowing for a three‐belt structure. During the October 13 storm the electrons in the region L>5 $L > 5$ were swept away by EMIC waves, leaving a narrow outer radiation belt confined within the region L≈4−5 $L\approx 4-5$ for several days. Numerical calculations demonstrate that the EMIC‐driven loss and chorus‐induced acceleration can account for the formation and evolution of the third‐belt morphology. Plain Language Summary: The Earth's electron radiation belts are usually composed of two high‐flux zones called the inner and outer belts, which are separated by a low‐flux slot region. However, previous studies have found that ultra‐relativistic (kinetic energy Ek>3 ${E}_{\mathrm{k}} > 3$ MeV) electrons sometimes exhibit a three‐belt morphology. Although some theories have been proposed, the mechanism underlying this rare phenomenon still requires further elucidation. Here we report a very interesting feature of 3.4–6.3 MeV electrons during two geomagnetic storms in October 2018. Prior to the first storm on October 7, the outer belt was present between the magnetic L $L$‐shell 3.0–5.0. During the storm main phase, electrons in the region L≈3.5−5.0 $L\approx 3.5-5.0$ were quickly lost by electromagnetic ion cyclotron (EMIC) waves, leaving a high‐flux zone between L≈3.0−3.5 $L\approx 3.0-3.5$. Over the following days, electrons in the region L>4 $L > 4$ were accelerated by chorus waves, consequently allowing for a three‐belt structure. During the second storm on October 13, electrons in the region L>5 $L > 5$ were swept away by EMIC waves, leaving a narrow outer belt confined within the region L≈4−5 $L\approx 4-5$ for several days. Numerical calculations demonstrate that the EMIC‐driven loss and chorus‐induced acceleration can account for the formation and evolution of the third‐belt morphology. Key Points: Ultra‐relativistic electrons exhibited three‐belt morphologies during storms in October 2018, corresponding to enhanced EMIC/chorus wavesCalculations show that electron loss/acceleration timescales induced by EMIC/chorus are about 0.01/10 days, comparable to observationsThe combined role of electromagnetic ion cyclotron (EMIC) and chorus waves can explain the formation and evolution of the three‐belt morphology [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
21699380
Volume :
129
Issue :
12
Database :
Complementary Index
Journal :
Journal of Geophysical Research. Space Physics
Publication Type :
Academic Journal
Accession number :
181825111
Full Text :
https://doi.org/10.1029/2024JA033380