Using MEPED observations to infer plasma density and chorus intensity in the radiation belts

Longley, William J.; Chan, Anthony A.; Jaynes, Allison N.; Elkington, Scot R.; Pettit, Joshua M.; Ross, Johnathan P. ORCID: https://orcid.org/0000-0001-5282-3293; Glauert, Sarah A. ORCID: https://orcid.org/0000-0003-0149-8608; Horne, Richard B. ORCID: https://orcid.org/0000-0002-0412-6407. 2022 Using MEPED observations to infer plasma density and chorus intensity in the radiation belts. Frontiers in Astronomy and Space Sciences, 9, 1063329. 15, pp. https://doi.org/10.3389/fspas.2022.1063329

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© 2022 Longley, Chan, Jaynes, Elkington, Pettit, Ross, Glauert and Horne. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
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Official URL: https://www.frontiersin.org/articles/10.3389/fspas...

Abstract/Summary

Efforts to model and predict energetic electron fluxes in the radiation belts are highly sensitive to local wave-particle interactions. In this study, we use multi-point measurements of precipitating and trapped electron fluxes to investigate the dynamic variation of chorus wave-particle interactions during the 17 March 2013 storm. Quasilinear theory characterizes the chorus wave-particle interaction as a diffusive process, with the diffusion coefficients depending on the particle energy and pitch angle, as well as the background plasma parameters such as the wave intensity and plasma density. These plasma parameters in the radiation belts are spatially localized and time-varying, so we construct event-specific diffusion coefficients using MEPED (onboard POES/MetOp) measurements of electron fluxes at low Earth orbit. This new method provides realistic diffusion coefficients for chorus waves that account for changes in the wave intensity, the plasma density, and the magnetic field strength in the outer radiation belt. We show that the inferred chorus intensity is significantly lower than previous estimates that use MEPED observations since the same amount of increased precipitation by 30–300 keV electrons can be explained by a change in the plasma density. This technique therefore allows for us to create time varying, global maps of the plasma-gyrofrequency ratio (fpe/fce), and therefore plasma density, in the outer radiation belts using the MEPED measurements. The global density estimates compare reasonably well to in situ density measurements from RBSP-B.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	https://doi.org/10.3389/fspas.2022.1063329
ISSN:	2296-987X
Additional Keywords:	Radiation Belts, wave-particle interaction, Quasilinear diffusion, SDE modeling, chorus waves, density measurements, POES/MetOp, Van Allen Probes
Date made live:	21 Nov 2022 09:28 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/533551

Item Type:

Publication - Article

Digital Object Identifier (DOI):

https://doi.org/10.3389/fspas.2022.1063329

ISSN:

2296-987X

Additional Keywords:

Radiation Belts, wave-particle interaction, Quasilinear diffusion, SDE modeling, chorus waves, density measurements, POES/MetOp, Van Allen Probes

Date made live:

21 Nov 2022 09:28 +0 (UTC)

URI:

https://nora.nerc.ac.uk/id/eprint/533551