Active Precipitation of Radiation Belt Electrons using Rocket Exhaust Driven Amplification (REDA) of Man‐Made Whistlers

Bernhardt, P.A.; Hua, M.; Bortnik, J.; Ma, Q.; Verronen, P.T.; McCarthy, M.P.; Hampton, D.L.; Golkowski, M.; Cohen, M.B.; Richardson, D.K.; Howarth, A.D.; James, H.G.; Meredith, N.P. ORCID: https://orcid.org/0000-0001-5032-3463. 2022 Active Precipitation of Radiation Belt Electrons using Rocket Exhaust Driven Amplification (REDA) of Man‐Made Whistlers. Journal of Geophysical Research: Space Physics, 127 (6), e2022JA030358. 17, pp. 10.1029/2022JA030358

Before downloading, please read NORA policies.

Preview	Text (Open Access) © 2022. The Authors. JGR Space Physics - 2022 - Bernhardt - Active Precipitation of Radiation Belt Electrons Using Rocket Exhaust Driven.pdf - Published Version Available under License Creative Commons Attribution 4.0. Download (2MB) | Preview
	Text This article is protected by copyright. All rights reserved. JGR Space Physics - 2022 - Bernhardt - Active Precipitation of Radiation Belt Electrons using Rocket Exhaust Driven.pdf - Accepted Version Restricted to NORA staff only Download (2MB) | Request a copy

Abstract/Summary

Ground-based VLF transmitters located around the world generate signals that leak through the bottom side of the ionosphere in the form of whistler mode waves. Wave and particle measurements on satellites have observed that these man-made VLF waves can be strong enough to scatter trapped energetic electrons into low pitch angle orbits, causing loss by absorption in the lower atmosphere. This precipitation loss process is greatly enhanced by intentional amplification of the whistler waves using a newly discovered process called Rocket Exhaust Driven Amplification (REDA). Satellite measurements of REDA have shown between 30- and 50-dB intensification of VLF waves in space using a 60-second burn of the 150 g/s thruster on the Cygnus satellite that services the International Space Station (ISS). This controlled amplification process is adequate to deplete the energetic particle population on the affected field lines in a few minutes rather than the multi-day period it would take naturally. Numerical simulations of the pitch angle diffusion for radiation belt particles use the UCLA quasi-linear Fokker Planck model (QLFP) to assess the impact of REDA on radiation belt remediation (RBR) of newly injected energetic electrons. The simulated precipitation fluxes of energetic electrons are applied to models of D-region electron density and bremsstrahlung x-rays for predictions of the modified environment that can be observed with satellite and ground-based sensors.

Item Type:	Publication - Article
Digital Object Identifier (DOI):	10.1029/2022JA030358
ISSN:	2169-9380
Additional Keywords:	Active Space Experiments, Parametric Amplifier, Wave Particle Interactions, Amplified Whistler Wave
Date made live:	30 May 2022 08:43 +0 (UTC)
URI:	https://nora.nerc.ac.uk/id/eprint/532675

Actions (login required)

View Item

Document Downloads

More statistics for this item...