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New chorus wave properties near the equator from Van Allen Probes wave observations
Journal article   Open access   Peer reviewed

New chorus wave properties near the equator from Van Allen Probes wave observations

W Li, O Santolik, C. A Kletzing, J Bortnik, W. S Kurth, R. M Thorne and G. B Hospodarsky
Geophysical research letters, Vol.43(10), pp.4725-4735
05/28/2016
DOI: 10.1002/2016GL068780
url
https://doi.org/10.1002/2016GL068780View
Published (Version of record) Open Access

Abstract

The chorus wave properties are evaluated using Van Allen Probes data in the Earth's equatorial magnetosphere. Two distinct modes of lower band chorus are identified: a quasi‐parallel mode and a quasi‐electrostatic mode, whose wave normal direction is close to the resonance cone. Statistical results indicate that the quasi‐electrostatic (quasi‐parallel) mode preferentially occurs during relatively quiet (disturbed) geomagnetic activity at lower (higher) L shells. Although the magnetic intensity of the quasi‐electrostatic mode is considerably weaker than the quasi‐parallel mode, their electric intensities are comparable. A newly identified feature of the quasi‐electrostatic mode is that its frequency peaks at higher values compared to the quasi‐parallel mode that exhibits a broad frequency spectrum. Moreover, upper band chorus wave normal directions vary between 0° and the resonance cone and become more parallel as geomagnetic activity increases. Our new findings suggest that chorus‐driven energetic electron dynamics needs a careful examination by considering the properties of these two distinct modes. Key Points Chorus wave normal and spectral properties are evaluated using Van Allen Probes wave data Lower band chorus has two distinct modes: a quasi‐parallel mode and a quasi‐electrostatic mode Quasi‐electrostatic chorus occurs preferentially during quiet times, at lower L, and in higher frequencies
chorus wave oblique quasi‐electrostatic quasi‐parallel wave normal angles

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