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First evidence for chorus at a large geocentric distance as a source of plasmaspheric hiss: Coordinated THEMIS and Van Allen Probes observation
Journal article   Open access   Peer reviewed

First evidence for chorus at a large geocentric distance as a source of plasmaspheric hiss: Coordinated THEMIS and Van Allen Probes observation

W Li, C. A Kletzing, L Chen, W. S Kurth, J Bortnik, G. B Hospodarsky, R. M Thorne and V Angelopoulos
Geophysical research letters, Vol.42(2), pp.241-248
01/28/2015
DOI: 10.1002/2014GL062832
url
https://doi.org/10.1002/2014GL062832View
Published (Version of record) Open Access

Abstract

Recent ray tracing suggests that plasmaspheric hiss can originate from chorus observed outside of the plasmapause. Although a few individual events have been reported to support this mechanism, the number of reported conjugate events is still very limited. Using coordinated observations between Time History of Events and Macroscale Interactions during Substorms (THEMIS) and Van Allen Probes, we report on an interesting event, where chorus was observed at a large L shell (~9.8), different from previously reported events at L < 6, but still exhibited a remarkable correlation with hiss observed in the outer plasmasphere (L ~ 5.5). Ray tracing indicates that a subset of chorus can propagate into the observed location of hiss on a timescale of ~5–6 s, in excellent agreement with the observed time lag between chorus and hiss. This provides quantitative support that chorus from large L shells, where it was previously considered unable to propagate into the plasmasphere, can in fact be the source of hiss. Key Points Chorus excited at large L can propagate into the plasmasphere and form hiss Conjugate observation shows excellent correlation between chorus and hiss Propagation time from source region of chorus to hiss agrees with observation
chorus hiss wave propagation

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