A nonstorm time enhancement of relativistic electrons in the outer radiation belt. Issue 1 (15th January 2014)

• Record Type: Journal Article
• Authors: Schiller, Quintin; Li, Xinlin; Blum, Lauren; Tu, Weichao; Turner, Drew L.; Blake, J. B.
• Is Part Of: Geophysical research letters. Volume 41:Issue 1(2014:Jan.)
• Page Start: 7
• Page End: 12
• Publication Date: 2014-01-15
• Subjects: Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2013GL058485
• Languages: English
• ISSNs: 0094-8276

Abstract

<abstract abstract-type="main"> <title>Abstract</title> <p>[1] Despite the lack of a geomagnetic storm (based on the <italic>Dst</italic> index), relativistic electron fluxes were enhanced over 2.5 orders of magnitude in the outer radiation belt in 13 h on 13–14 January 2013. The unusual enhancement was observed by Magnetic Electron Ion Spectrometer (MagEIS), onboard the Van Allen Probes; Relativistic Electron and Proton Telescope Integrated Little Experiment, onboard the Colorado Student Space Weather Experiment; and Solid State Telescope, onboard Time History of Events and Macroscale Interactions during Substorms (THEMIS). Analyses of MagEIS phase space density (PSD) profiles show a positive outward radial gradient from 4 &lt; <italic>L</italic> &lt; 5.5. However, THEMIS observations show a peak in PSD outside of the Van Allen Probes' apogee, which suggest a very interesting scenario: wave‐particle interactions causing a PSD peak at ~ <italic>L</italic>* = 5.5 from where the electrons are then rapidly transported radially inward. This letter demonstrates, for the first time in detail, that geomagnetic storms are not necessary for causing dramatic enhancements in the outer radiation belt.</p> </abstract>