2021
DOI: 10.1029/2020ja028477
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Energy‐Resolved Detection of Precipitating Electrons of 30–100 keV by a Sounding Rocket Associated With Dayside Chorus Waves

Abstract: Precipitating electrons from the magnetosphere have been measured by balloons, sounding rockets, and low-altitude satellites to investigate auroral zone phenomenology (e.g.

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Cited by 2 publications
(2 citation statements)
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“…It carried eight observation packages. One of the packages is called PARM (Pulsating AuroRa and Microburst) (Sugo et al., 2021) which includes a high‐energy electron detector (HEP: High Energy Particle detector) and a magnetometer (AFG: ASIC‐based FluxGate magnetometer). Pitch angles of observed electrons were calculated by using AFG data in this study.…”
Section: Instrumentationmentioning
confidence: 99%
“…It carried eight observation packages. One of the packages is called PARM (Pulsating AuroRa and Microburst) (Sugo et al., 2021) which includes a high‐energy electron detector (HEP: High Energy Particle detector) and a magnetometer (AFG: ASIC‐based FluxGate magnetometer). Pitch angles of observed electrons were calculated by using AFG data in this study.…”
Section: Instrumentationmentioning
confidence: 99%
“…For more detailed information, please refer to previous studies (e.g., Kennel, 1969; Summers et al., 1998; Storey, 1953). Previous observations have shown that in the plasma trough, where the electron density is low, whistler‐mode chorus waves (Nishimura et al., 2010; Sugo et al., 2021; Miyoshi et al., 2015a, 2015b, 2021), electromagnetic ion cyclotron (EMIC) waves (Jordanova et al., 2008; Miyoshi et al., 2008), electron cyclotron harmonic (ECH) waves (Zhang et al., 2015; Fukizawa et al., 2018), time domain structures consisting of complicated electrostatic fluctuations and kinetic Alfven waves (Khazanov et al., 2021) cause electron precipitation in a wide energy range.…”
Section: Introductionmentioning
confidence: 97%