Electron precipitation from EMIC waves: A case study from 31 May 2013

On 31 May 2013 several rising tone electromagnetic ion cyclotron (EMIC) waves with intervals of pulsations of diminishing periods were observed in the magnetic local time afternoon and evening sectors during the onset of a moderate/large geomagnetic storm. The waves were sequentially observed in Fin...

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Veröffentlicht in:Journal of geophysical research. Space physics 2015-05, Vol.120 (5), p.3618-3631
Hauptverfasser: Clilverd, Mark A., Duthie, Roger, Hardman, Rachael, Hendry, Aaron T., Rodger, Craig J., Raita, Tero, Engebretson, Mark, Lessard, Marc R., Danskin, Donald, Milling, David K.
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container_end_page 3631
container_issue 5
container_start_page 3618
container_title Journal of geophysical research. Space physics
container_volume 120
creator Clilverd, Mark A.
Duthie, Roger
Hardman, Rachael
Hendry, Aaron T.
Rodger, Craig J.
Raita, Tero
Engebretson, Mark
Lessard, Marc R.
Danskin, Donald
Milling, David K.
description On 31 May 2013 several rising tone electromagnetic ion cyclotron (EMIC) waves with intervals of pulsations of diminishing periods were observed in the magnetic local time afternoon and evening sectors during the onset of a moderate/large geomagnetic storm. The waves were sequentially observed in Finland, Antarctica, and western Canada. Coincident electron precipitation by a network of ground‐based Antarctic Arctic Radiation‐belt Dynamic Deposition VLF Atmospheric Research Konsortia and riometer instruments, as well as the Polar‐orbiting Operational Environmental Satellite (POES) electron telescopes, was also observed. At the same time, POES detected 30–80 keV proton precipitation drifting westward at locations that were consistent with the ground‐based observations, indicating substorm injection. Through detailed modeling of the combination of ground and satellite observations, the characteristics of the EMIC‐induced electron precipitation were identified as latitudinal width of 2–3° or ΔL = 1 Re, longitudinal width ~50° or 3 h magnetic local time, lower cutoff energy 280 keV, typical flux 1 × 104 el cm−2 sr−1 s−1 > 300 keV. The lower cutoff energy of the most clearly defined EMIC rising tone in this study confirms the identification of a class of EMIC‐induced precipitation events with unexpectedly low‐energy cutoffs of
doi_str_mv 10.1002/2015JA021090
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The waves were sequentially observed in Finland, Antarctica, and western Canada. Coincident electron precipitation by a network of ground‐based Antarctic Arctic Radiation‐belt Dynamic Deposition VLF Atmospheric Research Konsortia and riometer instruments, as well as the Polar‐orbiting Operational Environmental Satellite (POES) electron telescopes, was also observed. At the same time, POES detected 30–80 keV proton precipitation drifting westward at locations that were consistent with the ground‐based observations, indicating substorm injection. Through detailed modeling of the combination of ground and satellite observations, the characteristics of the EMIC‐induced electron precipitation were identified as latitudinal width of 2–3° or ΔL = 1 Re, longitudinal width ~50° or 3 h magnetic local time, lower cutoff energy 280 keV, typical flux 1 × 104 el cm−2 sr−1 s−1 &gt; 300 keV. The lower cutoff energy of the most clearly defined EMIC rising tone in this study confirms the identification of a class of EMIC‐induced precipitation events with unexpectedly low‐energy cutoffs of &lt;400 keV. Key Points EMIC induced electron precipitation with latitudinal width of 2–3° EMIC induced electron precipitation with lower cutoff energy of 280 keV Oxygen band EMIC induced electron precipitation driven by substorm</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1002/2015JA021090</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Antarctica ; Atmospheric research ; Atmospherics ; Cyclotrons ; electromagnetic ion cyclotron ; Electron precipitation ; Electrons ; Energy ; Geophysics ; Ground-based observation ; Low energy ; Magnetic fields ; Networks ; radio propagation ; satellite</subject><ispartof>Journal of geophysical research. 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Space physics</title><addtitle>J. Geophys. Res. Space Physics</addtitle><description>On 31 May 2013 several rising tone electromagnetic ion cyclotron (EMIC) waves with intervals of pulsations of diminishing periods were observed in the magnetic local time afternoon and evening sectors during the onset of a moderate/large geomagnetic storm. The waves were sequentially observed in Finland, Antarctica, and western Canada. Coincident electron precipitation by a network of ground‐based Antarctic Arctic Radiation‐belt Dynamic Deposition VLF Atmospheric Research Konsortia and riometer instruments, as well as the Polar‐orbiting Operational Environmental Satellite (POES) electron telescopes, was also observed. At the same time, POES detected 30–80 keV proton precipitation drifting westward at locations that were consistent with the ground‐based observations, indicating substorm injection. Through detailed modeling of the combination of ground and satellite observations, the characteristics of the EMIC‐induced electron precipitation were identified as latitudinal width of 2–3° or ΔL = 1 Re, longitudinal width ~50° or 3 h magnetic local time, lower cutoff energy 280 keV, typical flux 1 × 104 el cm−2 sr−1 s−1 &gt; 300 keV. The lower cutoff energy of the most clearly defined EMIC rising tone in this study confirms the identification of a class of EMIC‐induced precipitation events with unexpectedly low‐energy cutoffs of &lt;400 keV. 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subjects Antarctica
Atmospheric research
Atmospherics
Cyclotrons
electromagnetic ion cyclotron
Electron precipitation
Electrons
Energy
Geophysics
Ground-based observation
Low energy
Magnetic fields
Networks
radio propagation
satellite
title Electron precipitation from EMIC waves: A case study from 31 May 2013
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