Nonstorm time dropout of radiation belt electron fluxes on 24 September 2013

Su, Zhenpeng; Gao, Zhonglei; Reeves, Geoffrey D.; Funsten, Herbert O.; Zhu, Hui; Li, Wen; Zheng, Huinan; Wang, Yuming; Wang, Shui; Spence, H. E.; Baker, D. N.; Blake, J. B.; Wygant, J. R.

doi:10.1002/2016JA022546

Title: Nonstorm time dropout of radiation belt electron fluxes on 24 September 2013

Journal Article · Fri Jul 01 00:00:00 EDT 2016 · Journal of Geophysical Research. Space Physics

DOI:https://doi.org/10.1002/2016JA022546· OSTI ID:1291235

Su, Zhenpeng ^[1]; Gao, Zhonglei ^[1]; Reeves, Geoffrey D. ^[2]; Funsten, Herbert O. ^[3]; Zhu, Hui ^[4]; Li, Wen ^[4]; Zheng, Huinan ^[1]; Wang, Yuming ^[1]; Wang, Shui ^[1]; Spence, H. E. ^[5]; Baker, D. N. ^[6]; Blake, J. B. ^[7]; Wygant, J. R. ^[8]

Univ. of Science and Technology of China, Hefei (China)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States); New Mexico Consortium, Los Alamos, NM (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Univ. of California, Los Angeles, CA (United States)
Univ. of New Hampshire, Durham, NH (United States). Dept. of Physics
Univ. of Colorado, Boulder, CO (United States)
The Aerospace Corp., Los Angeles, CA (United States)
Univ. of Minnesota, Minneapolis, MN (United States)

Radiation belt electron flux dropouts during the main phase of geomagnetic storms have received increasing attention in recent years. Here we focus on a rarely reported nonstorm time dropout event observed by Van Allen Probes on 24 September 2013. Within several hours, the radiation belt electron fluxes exhibited a significant (up to 2 orders of magnitude) depletion over a wide range of radial distances (L > 4.5), energies (~500 keV to several MeV) and equatorial pitch angles (0° ≤ α_e ≤ 180°). STEERB simulations show that the relativistic electron loss in the region L = 4.5–6.0 was primarily caused by the pitch angle scattering of observed plasmaspheric hiss and electromagnetic ion cyclotron waves. Furthermore, our results emphasize the complexity of radiation belt dynamics and the importance of wave-driven precipitation loss even during nonstorm times.

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Research Organization:: Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: National Aeronautics and Space Administration (NASA); USDOE

Grant/Contract Number:: AC52-06NA25396

OSTI ID:: 1291235

Report Number(s):: LA-UR-16-23140

Journal Information:: Journal of Geophysical Research. Space Physics, Journal Name: Journal of Geophysical Research. Space Physics; ISSN 2169-9380

Publisher:: American Geophysical UnionCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 44 works

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Energetic Electron Precipitation: Multievent Analysis of Its Spatial Extent During EMIC Wave Activity Capannolo, L.; Li, W.; Ma, Q. Journal of Geophysical Research: Space Physics https://doi.org/10.1029/2018ja026291	journal	April 2019
Direct Observation of Subrelativistic Electron Precipitation Potentially Driven by EMIC Waves Capannolo, L.; Li, W.; Ma, Q. Geophysical Research Letters, Vol. 46, Issue 22 https://doi.org/10.1029/2019gl084202	journal	November 2019
Impact of Significant Time‐Integrated Geomagnetic Activity on 2‐MeV Electron Flux Mourenas, D.; Artemyev, A. V.; Zhang, X. ‐J. Journal of Geophysical Research: Space Physics, Vol. 124, Issue 6 https://doi.org/10.1029/2019ja026659	journal	June 2019
Propagation of EMIC Waves Inside the Plasmasphere: A Two‐Event Study Wang, G.; Zhang, T. L.; Gao, Z. L. Journal of Geophysical Research: Space Physics, Vol. 124, Issue 11 https://doi.org/10.1029/2019ja027055	journal	November 2019

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