Evidence of stronger pitch angle scattering loss caused by oblique whistler-mode waves as compared with quasi-parallel waves

Wave normal distributions of lower‐band whistler‐mode waves observed outside the plasmapause exhibit two peaks: one near the parallel direction and the other at very oblique angles. We analyze a number of conjunction events between the Van Allen Probes near the equatorial plane and Polar Orbiting En...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Geophysical research letters 2014-09, Vol.41 (17), p.6063-6070
Hauptverfasser: Li, W., Mourenas, D., Artemyev, A. V., Agapitov, O. V., Bortnik, J., Albert, J. M., Thorne, R. M., Ni, B., Kletzing, C. A., Kurth, W. S., Hospodarsky, G. B.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:Wave normal distributions of lower‐band whistler‐mode waves observed outside the plasmapause exhibit two peaks: one near the parallel direction and the other at very oblique angles. We analyze a number of conjunction events between the Van Allen Probes near the equatorial plane and Polar Orbiting Environmental Satellites (POES) at conjugate low altitudes, where lower‐band whistler‐mode wave amplitudes were inferred from the two‐directional POES electron measurements over 30–100 keV, assuming that these waves were quasi‐parallel. For conjunction events, the wave amplitudes inferred from the POES electron measurements were found to be overestimated as compared with the Van Allen Probes measurements primarily for oblique waves and quasi‐parallel waves with small wave amplitudes (< ~20 pT) measured at low latitudes. This provides plausible experimental evidence of stronger pitch angle scattering loss caused by oblique waves than by quasi‐parallel waves with the same magnetic wave amplitudes, as predicted by numerical calculations. Key Points Oblique waves cause stronger pitch angle scattering than parallel waves with the same BwWe provide the evidence using conjunction events between Radiation Belt Storm Probes (RBSP) and POESBoth observational and numerical results support this scenario
ISSN:0094-8276
1944-8007
DOI:10.1002/2014GL061260