The Repetition Period of MeV Electron Microbursts as Measured by SAMPEX/HILT

Hamdan Kandar, Lauren Blum, Mykhaylo Shumko, Lunjin Chen, Jih Hong Shue

研究成果: 雜誌貢獻期刊論文同行評審

摘要

Here we examine properties of MeV electron microbursts to better understand their generation mechanisms. Using 15 years of data from Solar, Anomalous, Magnetospheric Particles Explorer/Heavy Ion Large Telescope, >1 MeV microburst repetition periods (time spacing between bursts) are examined and clear dependencies on Auroral Electrojet (AE), L shell, and magnetic local time (MLT) are discovered. Microburst repetition periods are shortest around 0–6 hr MLT and 4–5 L shell, and grow longer toward the day and afternoon sectors and larger L shells. Shorter repetition periods (<1 s) are also found to be more common during higher AE, while longer periods (>10 s) more common during quiet times. The microburst repetition period distributions are compared directly to those of rising tone chorus wave elements and found to be similar in the night, dawn and day MLT sectors, suggesting chorus wave repetition periods are likely directly controlling those of microburst precipitation. However, dusk-side distributions differ, indicating that the dusk-side microbursts properties may be controlled by other processes.

原文???core.languages.en_GB???
文章編號e2023GL104663
期刊Geophysical Research Letters
50
發行號22
DOIs
出版狀態已出版 - 28 11月 2023

指紋

深入研究「The Repetition Period of MeV Electron Microbursts as Measured by SAMPEX/HILT」主題。共同形成了獨特的指紋。

引用此