Observations of High Energy Electrons during the 5 September 2022 Solar Energetic Particle Event with the Parker Solar Probe EPI-Hi Instrument

A. W. Labrador, J. G. Mitchell, E. R. Christian, C. M.S. Cohen, A. C. Cummings, G. A. de Nolfo, R. A. Leske, David J. McComas, R. A. Mewaldt, J. S. Rankin, N. Schwadron, E. C. Stone, J. Szalay, M. E. Wiedenbeck

Research output: Contribution to journalConference articlepeer-review

Abstract

The 5 September 2022 SEP event observed by Parker Solar Probe yielded some of the highest intensities in high energy electrons observed at the instrument since its launch in 2018. For this paper, we will examine the high energy electron signals detected by the EPI-Hi HET instrument to measure the spectra, the time-evolution of the spectra, and anisotropies in electrons during the event. We will examine the HET electron measurements and compare them with the proton measurements. We will also explain in detail the calculation of the electron spectra during periods of very high count rate.

Original languageEnglish (US)
Article number1315
JournalProceedings of Science
Volume444
StatePublished - Sep 27 2024
Event38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan
Duration: Jul 26 2023Aug 3 2023

All Science Journal Classification (ASJC) codes

  • General

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