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Global Model of Whistler Mode Chorus in the Near-Equatorial Region (|λm|<  18°)


AuthorMeredith, Nigel; Horne, Richard; Shen, Xiao-Chen; Li, Wen; Bortnik, Jacob;
Keywordswhistler mode chorus; wave-particle interactions; Radiation belts; Van Allen Probes
AbstractWe extend our database of whistler mode chorus, based on data from seven satellites, by including ∼3 years of data from Radiation Belt Storm Probes (RBSP)-A and RBSP-B and an additional ∼6 years of data from Time History of Events and Macroscale Interactions during Substorms (THEMIS)-A, THEMIS-D, and THEMIS-E. The new database allows us to probe the near-equatorial region in detail, revealing new features. In the equatorial source region, |λm|<6°, strong wave power is most extensive in the 0.1–0.4fce bands in the region 21–11 magnetic local time (MLT) from the plasmapause out to L∗ = 8 and beyond, especially near dawn. At higher frequencies, in the 0.4–0.6fce frequency bands, strong wave power is more tightly confined, typically being restricted to the postmidnight sector in the region 4
Year of Publication2020
JournalGeophysical Research Letters
Volume47
Number of Pagese2020GL087311
Section
Date Published05/2020
ISBN
URLhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2020GL087311
DOIhttps://doi.org/10.1029/2020GL087311