On the Importance of Using Event-Specific Wave Diffusion Rates in Modeling Diffuse Electron Precipitation

Yu, Yiqun; Hosokawa, Keisuke; Ni, Binbin; Jordanova, Vania Koleva; Miyoshi, Yoshizumi; Cao, Jinbin; Tian, Xingbin; Ma, Longxing

doi:10.1029/2021ja029918

Title: On the Importance of Using Event-Specific Wave Diffusion Rates in Modeling Diffuse Electron Precipitation

Journal Article · 31 March 2022 · Journal of Geophysical Research. Space Physics

DOI: https://doi.org/10.1029/2021ja029918 · OSTI ID:1866964

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Beihang Univ., Beijing (China); Ministry of Industry and Information Technology, Beijing (China)
Univ. of Electro-Communications, Tokyo (Japan)
Wuhan Univ. (China); CAS Center for Excellence in Comparative Planetology, Heifei (China)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Nagoya Univ. (Japan)

A few to tens of keV electron precipitation that carries substantial energy source down to the upper atmosphere to create aurora is manifested as an important magnetosphere-ionosphere coupling process. The precipitation is usually caused by scattering processes associated with plasma waves in the magnetosphere. The scattering process is often quantified by wave diffusion rates that indicate how fast an electron is scattered. Global models commonly use diffusion coefficients that are derived from statistical wave models. However, due to the statistical nature, many localized, transient features could be smeared out. In this study, we investigate electron precipitation using event-specific diffusion coefficients that are obtained based on simultaneous in-situ measured/inferred, rather than statistical, chorus wave dynamics. We find that the application of the event-specific diffusion coefficients associated with a more dynamic and intense chorus wave model leads more electrons, particularly at several to tens of keV in the dawn-to-noon sector at L > 3, to precipitate than using statistical coefficients. Here, the new simulation roughly captures both the intensity and variability of the precipitating flux as detected by the NOAA/POES satellites. Ionospheric electron density in the lower E region (100–120 km) observed by the mid-latitude Millstone Hill radar is also much better reproduced, while the case using statistical diffusion coefficients underestimates the ionization rate. This study implies the importance of using event-specific diffusion rates in simulating the diffuse electron precipitation and understanding the magnetosphere-ionosphere coupling.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE; NASA; NSFC; JSPS

Grant/Contract Number:: 89233218CNA000001

OSTI ID:: 1866964

Report Number(s):: LA-UR-21-29010

Journal Information:: Journal of Geophysical Research. Space Physics, Journal Name: Journal of Geophysical Research. Space Physics Journal Issue: 4 Vol. 127; ISSN 2169-9380

Publisher:: American Geophysical UnionCopyright Statement

Country of Publication:: United States

Language:: English

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