Parker Solar Probe Energetic Particle Observations of the September 5, 2022 SEP Event

C. M.S. Cohen; E. R. Christian; A. C. Cummings; A. J. Davis; G. A. de Nolfo; M. I. Desai; J. Giacalone; M. E. Hill; A. W. Labrador; R. A. Leske; D. J. McComas; R. L. McNutt; R. A. Mewaldt; D. G. Mitchell; J. G. Mitchell; J. S. Rankin; N. A. Schwadron; T. Sharma; M. M. Shen; J. R. Szalay; M. E. Wiedenbeck; A. Vourlidas; S. D. Bale; M. Pulupa; J. C. Kasper; D. E. Larson; P. Whittlesey

Parker Solar Probe Energetic Particle Observations of the September 5, 2022 SEP Event

C. M.S. Cohen, E. R. Christian, A. C. Cummings, A. J. Davis, G. A. de Nolfo, M. I. Desai, J. Giacalone, M. E. Hill, A. W. Labrador, R. A. Leske, D. J. McComas, R. L. McNutt, R. A. Mewaldt, D. G. Mitchell, J. G. Mitchell, J. S. Rankin, N. A. Schwadron, T. Sharma, M. M. Shen, J. R. SzalayM. E. Wiedenbeck, A. Vourlidas, S. D. Bale, M. Pulupa, J. C. Kasper, D. E. Larson, P. Whittlesey

Research output: Contribution to journal › Conference article › peer-review

Abstract

On 5 September 2022 Parker Solar Probe (Parker) was less than 17 RS from the Sun when the Integrated Science Investigation of the Sun (IS☉IS) observed an intense solar energetic particle (SEP) event associated with a strong soft x-ray flare and a very fast coronal mass ejection (CME). The energy dependence of the particle onsets indicate shock acceleration both far and close to the spacecraft providing a unique opportunity to study the evolution of particle energization. Significant time variability of the characteristics of the energetic particle population is evident and has been examined in relation to magnetic and plasma structures and expectations from acceleration processes. We present an overview of these observations and highlight a few of the ongoing studies.

Original language	English (US)
Article number	1276
Journal	Proceedings of Science
Volume	444
State	Published - Sep 27 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: Jul 26 2023 → Aug 3 2023

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Cohen, C. M. S., Christian, E. R., Cummings, A. C., Davis, A. J., de Nolfo, G. A., Desai, M. I., Giacalone, J., Hill, M. E., Labrador, A. W., Leske, R. A., McComas, D. J., McNutt, R. L., Mewaldt, R. A., Mitchell, D. G., Mitchell, J. G., Rankin, J. S., Schwadron, N. A., Sharma, T., Shen, M. M., ... Whittlesey, P. (2024). Parker Solar Probe Energetic Particle Observations of the September 5, 2022 SEP Event. Proceedings of Science, 444, Article 1276.

Cohen, CMS, Christian, ER, Cummings, AC, Davis, AJ, de Nolfo, GA, Desai, MI, Giacalone, J, Hill, ME, Labrador, AW, Leske, RA, McComas, DJ, McNutt, RL, Mewaldt, RA, Mitchell, DG, Mitchell, JG, Rankin, JS, Schwadron, NA, Sharma, T, Shen, MM, Szalay, JR, Wiedenbeck, ME, Vourlidas, A, Bale, SD, Pulupa, M, Kasper, JC, Larson, DE & Whittlesey, P 2024, 'Parker Solar Probe Energetic Particle Observations of the September 5, 2022 SEP Event', Proceedings of Science, vol. 444, 1276.

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title = "Parker Solar Probe Energetic Particle Observations of the September 5, 2022 SEP Event",

abstract = "On 5 September 2022 Parker Solar Probe (Parker) was less than 17 RS from the Sun when the Integrated Science Investigation of the Sun (IS☉IS) observed an intense solar energetic particle (SEP) event associated with a strong soft x-ray flare and a very fast coronal mass ejection (CME). The energy dependence of the particle onsets indicate shock acceleration both far and close to the spacecraft providing a unique opportunity to study the evolution of particle energization. Significant time variability of the characteristics of the energetic particle population is evident and has been examined in relation to magnetic and plasma structures and expectations from acceleration processes. We present an overview of these observations and highlight a few of the ongoing studies.",

author = "Cohen, {C. M.S.} and Christian, {E. R.} and Cummings, {A. C.} and Davis, {A. J.} and {de Nolfo}, {G. A.} and Desai, {M. I.} and J. Giacalone and Hill, {M. E.} and Labrador, {A. W.} and Leske, {R. A.} and McComas, {D. J.} and McNutt, {R. L.} and Mewaldt, {R. A.} and Mitchell, {D. G.} and Mitchell, {J. G.} and Rankin, {J. S.} and Schwadron, {N. A.} and T. Sharma and Shen, {M. M.} and Szalay, {J. R.} and Wiedenbeck, {M. E.} and A. Vourlidas and Bale, {S. D.} and M. Pulupa and Kasper, {J. C.} and Larson, {D. E.} and P. Whittlesey",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

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AU - Cohen, C. M.S.

AU - Christian, E. R.

AU - Cummings, A. C.

AU - Davis, A. J.

AU - de Nolfo, G. A.

AU - Desai, M. I.

AU - Giacalone, J.

AU - Hill, M. E.

AU - Labrador, A. W.

AU - Leske, R. A.

AU - McComas, D. J.

AU - McNutt, R. L.

AU - Mewaldt, R. A.

AU - Mitchell, D. G.

AU - Mitchell, J. G.

AU - Rankin, J. S.

AU - Schwadron, N. A.

AU - Sharma, T.

AU - Shen, M. M.

AU - Szalay, J. R.

AU - Wiedenbeck, M. E.

AU - Vourlidas, A.

AU - Bale, S. D.

AU - Pulupa, M.

AU - Kasper, J. C.

AU - Larson, D. E.

AU - Whittlesey, P.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - On 5 September 2022 Parker Solar Probe (Parker) was less than 17 RS from the Sun when the Integrated Science Investigation of the Sun (IS☉IS) observed an intense solar energetic particle (SEP) event associated with a strong soft x-ray flare and a very fast coronal mass ejection (CME). The energy dependence of the particle onsets indicate shock acceleration both far and close to the spacecraft providing a unique opportunity to study the evolution of particle energization. Significant time variability of the characteristics of the energetic particle population is evident and has been examined in relation to magnetic and plasma structures and expectations from acceleration processes. We present an overview of these observations and highlight a few of the ongoing studies.

AB - On 5 September 2022 Parker Solar Probe (Parker) was less than 17 RS from the Sun when the Integrated Science Investigation of the Sun (IS☉IS) observed an intense solar energetic particle (SEP) event associated with a strong soft x-ray flare and a very fast coronal mass ejection (CME). The energy dependence of the particle onsets indicate shock acceleration both far and close to the spacecraft providing a unique opportunity to study the evolution of particle energization. Significant time variability of the characteristics of the energetic particle population is evident and has been examined in relation to magnetic and plasma structures and expectations from acceleration processes. We present an overview of these observations and highlight a few of the ongoing studies.

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M3 - Conference article

AN - SCOPUS:85212302426

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1276

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Parker Solar Probe Energetic Particle Observations of the September 5, 2022 SEP Event

Abstract

ASJC Scopus subject areas

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