Non‐storm erosion of MeV electron outer radiation belt down to L* < 4.0 associated with successive enhancements of solar wind density. Issue 6 (21st December 2021)

• Record Type: Journal Article
• Authors: Xiong, Ying; Xie, Lun; Fu, SuiYan; Ni, BinBin; Pu, ZuYin
• Is Part Of: Earth and planetary physics. Volume 5:Issue 6(2021)
• Page Start: 581
• Page End: 591
• Publication Date: 2021-12-21
• Subjects: solar wind density enhancement -- outer radiation belt -- MeV electrons -- outward radial diffusion -- EMIC wave scattering loss; Geophysics -- Periodicals; Earth sciences -- Periodicals; Planets -- Geology -- Periodicals; 550.5
• DOI: 10.26464/epp2021051
• Languages: English
• ISSNs: 2096-3955

Abstract

Abstract: We report an unusual non‐storm erosion event of outer zone MeV electron distribution during three successive solar wind number density enhancements (SWDEs) on November 27−30, 2015. Loss of MeV electrons and energy‐dependent narrowing of electron pitch angle distributions (PAD) first developed at L * = 5.5 and then moved down to L * &lt; 4. According to the evolution of the electron phase space density (PSD) profile, losses of electrons with small pitch angles at L * &gt; 4 during SWDE1 are mainly due to outward radial diffusion. However during SWDE2&amp;3, scattering loss due to EMIC waves is dominant at 4 &lt; L * &lt; 5. As for electrons with large pitch angles, outward radial diffusion is the primary loss mechanism throughout all SWDEs which is consistent with the incursion of the Last Closed Drift Shell (LCDS). The inner edge of EMIC wave activity moved from L * ~5 to L * ~4 and from L ~6.4 to L ~4.2 from SWDE1 to SWDE2&amp;3, respectively, observed by Van Allen Probes and by ground stations. This is consistent with the inward penetration of anisotropic energetic protons from L * = 4.5 to L * = 3.5, suggesting that the inward extension of EMIC waves may be driven by the inward injection of anisotropic energetic protons from the dense plasma sheet. Key Points: The non‐storm loss mechanisms of MeV electrons in the outer radiation belt during three successive solar wind density enhancements are investigated. The losses of electrons with small pitch angles are first controlled by outward radial diffusion at L * &gt; 4, then by EMIC‐wave‐driven pitch angle scattering at 4 &lt; L * &lt; 5. Outward radial diffusion is the primary loss mechanism for large pitch angle electrons.