Van Allen Probes: Perigee ~1.1Re, Apogee ~5.8Re, Inclination 10 degrees THEMIS: Apogee above 10Re, Perigee below 2Re Polar Data Centre,Natural Environment Research Council,UK Research & InnovationĭE1: Perigee 568km, Apogee 23,289 km, Inclination 89.9 degreesĭouble Star TC1: Perigee 562km, Apogee 78,790km, Inclination 28.2 degrees Global model of Whistler Mode Chorus in the Near-Equatorial Region (|λ|m<18o) Meredith, Nigel Horne, Richard Shen, Xiao-Chen Li, Wen Bortnik, Jacob
Full details of the subsequent analysis are given in Meredith et al. The AE indices used in this study are available from the NSSDC Omniweb. The Van Allen Probes plasma wave data are available at.
#Cdaweb vs omniweb archive#
The Double Star TC1 data are available at the Cluster Science Archive (). The DE1 wave data are available from the CDAWeb ().
The plasma wave data used in this study come from Dynamics Explorer 1 (DE1), Double Star TC1, THEMIS-A, THEMIS-D, THEMIS-E, RBSP-A and RBSP-B. The wave data have been calibrated and quality-controlled prior to release. Sun-earth Interactions > Ionosphere/Magnetosphere Dynamics > Plasma Waves.In this study we extend our existing database of whistler mode chorus by including ~3 years of data from RBSP-A and RBSP-B and an additional ~6 years of data from THEMIS A, D, and E, greatly improving the statistics and coverage in the near-equatorial region (|MLAT| Ionosphere/Magnetosphere Dynamics Whistler mode chorus is an important magnetospheric emission, playing fundamental roles in the dynamics of the Earth's outer radiation belt and the production of the Earth's diffuse and pulsating aurora.
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