Measuring Low Plasma Density in the Earth's Equatorial Magnetosphere From Magnetosonic Waves

Horne, Richard ORCID: https://orcid.org/0000-0002-0412-6407; Daggitt, Thomas ORCID: https://orcid.org/0000-0002-3021-8890; Meredith, Nigel ORCID: https://orcid.org/0000-0001-5032-3463; Glauert, Sarah ORCID: https://orcid.org/0000-0003-0149-8608; Liu, Xu; Chen, Lunjin. 2024 Measuring Low Plasma Density in the Earth's Equatorial Magnetosphere From Magnetosonic Waves. Geophysical Research Letters, 51 (12), e2024GL108407. 7, pp. https://doi.org/10.1029/2024GL108407

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Text (Open Access) © 2024. The Authors. Geophysical Research Letters published by Wiley Periodicals LLC on behalf of American Geophysical Union. Geophysical Research Letters - 2024 - Horne - Measuring Low Plasma Density in the Earth s Equatorial Magnetosphere From.pdf - Published Version Available under License Creative Commons Attribution 4.0. Download (1MB) | Preview

Abstract/Summary

The plasma density is one of the most fundamental quantities of any plasma yet measuring it in space is exceptionally difficult when the density is low. Measurements from particle detectors are contaminated by spacecraft photoelectrons and methods using plasma wave emissions are hampered by natural plasma instabilities which dominate the wave spectrum. Here we present a new method which calculates the density from magnetosonic waves near the lower hybrid resonance frequency. The method works most effectively when the ratio of the plasma to cyclotron frequency is fpe/fce < 3.5. The method provides a lower bound on the plasma density. Using the new method we show that wave acceleration of electrons to relativistic energies is increased by orders of magnitude. The method enables years of satellite data to be re-analyzed for the Earth and the effectiveness of wave acceleration at the Earth, Jupiter and Saturn to be re-assessed.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	https://doi.org/10.1029/2024GL108407
ISSN:	0094-8276
Date made live:	17 Jun 2024 08:55 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/536768

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