Direct Observation of Subrelativistic Electron Precipitation Potentially Driven by EMIC Waves
Supporting Files
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2019
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Details
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Journal Title:Geophysical Research Letters
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Personal Author:Capannolo, L.
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Li, W.
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Ma, Q.
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Chen, L.
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Shen, X.‐C.
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Spence, H. E.
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Sample, J.
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Johnson, A.
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Shumko, M.
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Klumpar, D. M.
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Redmon, R. J.
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NOAA Program & Office:
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Description:Electromagnetic ion cyclotron (EMIC) waves are known to typically cause electron losses into Earth's upper atmosphere at >~1 MeV, while the minimum energy of electrons subject to efficient EMIC-driven precipitation loss is unresolved. This letter reports electron precipitation from subrelativistic energies of ~250 keV up to ~1 MeV observed by the Focused Investigations of Relativistic Electron Burst Intensity, Range and Dynamics (FIREBIRD-II) CubeSats, while two Polar Operational Environmental Satellites (POES) observed proton precipitation nearby. Van Allen Probe A detected EMIC waves (~0.7–2.0 nT) over the similar L shell extent of electron precipitation observed by FIREBIRD-II, albeit with a ~1.6 magnetic local time (MLT) difference. Although plasmaspheric hiss and magnetosonic waves were also observed, quasi-linear calculations indicate that EMIC waves were the most efficient in driving the electron precipitation. Quasi-linear theory predicts efficient precipitation at >0.8–1 MeV (due to H-band EMIC waves), suggesting that other mechanisms are required to explain the observed subrelativistic electron precipitation.
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Keywords:
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Source:Geophysical Research Letters, 46(22), 12711-12721
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DOI:
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Document Type:
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Rights Information:Other
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Compliance:Submitted
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Main Document Checksum:urn:sha256:ca7cf377639cc68b1f19e1321b0d7fd412f535c8381776e8024f2e06b1a19554
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