Investigating energetic electron precipitation through combining ground-based and balloon observations
Clilverd, Mark A. ORCID: https://orcid.org/0000-0002-7388-1529; Rodger, Craig J.; McCarthy, Michael; Millan, Robyn; Blum, Lauren W.; Cobbett, Neil; Brundell, James B.; Danskin, Donald; Halford, Alexa J.. 2017 Investigating energetic electron precipitation through combining ground-based and balloon observations. Journal of Geophysical Research: Space Physics, 122 (1). 534-546. https://doi.org/10.1002/2016JA022812
Before downloading, please read NORA policies.
|
Text
© 2017. American Geophysical Union. All Rights Reserved. Clilverd_et_al-2017-Journal_of_Geophysical_Research__Space_Physics.pdf - Published Version Download (1MB) | Preview |
Abstract/Summary
A detailed comparison is undertaken of the energetic electron spectra and fluxes of two precipitation events that were observed in 18/19 January 2013. A novel but powerful technique of combining simultaneous ground-based subionospheric radio wave data and riometer absorption measurements with X-ray fluxes from a Balloon Array for Relativistic Radiation-belt Electron Losses (BARREL) balloon is used for the first time as an example of the analysis procedure. The two precipitation events are observed by all three instruments, and the relative timing is used to provide information/insight into the spatial extent and evolution of the precipitation regions. The two regions were found to be moving westward with drift periods of 5–11 h and with longitudinal dimensions of ~20° and ~70° (1.5–3.5 h of magnetic local time). The electron precipitation spectra during the events can be best represented by a peaked energy spectrum, with the peak in flux occurring at ~1–1.2 MeV. This suggests that the radiation belt loss mechanism occurring is an energy-selective process, rather than one that precipitates the ambient trapped population. The motion, size, and energy spectra of the patches are consistent with electromagnetic ion cyclotron-induced electron precipitation driven by injected 10–100 keV protons. Radio wave modeling calculations applying the balloon-based fluxes were used for the first time and successfully reproduced the ground-based subionospheric radio wave and riometer observations, thus finding strong agreement between the observations and the BARREL measurements.
Item Type: | Publication - Article |
---|---|
Digital Object Identifier (DOI): | https://doi.org/10.1002/2016JA022812 |
Programmes: | BAS Programmes > BAS Programmes 2015 > Space Weather and Atmosphere |
ISSN: | 0148-0227 |
Additional Keywords: | electron precipitation, AARDDVARK, BARREL, EMIc waves |
Date made live: | 18 Apr 2017 13:29 +0 (UTC) |
URI: | https://nora.nerc.ac.uk/id/eprint/513482 |
Actions (login required)
View Item |
Document Downloads
Downloads for past 30 days
Downloads per month over past year