PSP Bibliography



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Found 4 entries in the Bibliography.


Showing entries from 1 through 4


2023

A Living Catalog of Parker Solar Probe IS\ensuremath\odotIS Energetic Particle Enhancements

Energetic charged particles are pervasive throughout the heliosphere with contributions from solar energetic particle events, stream and corotating interaction regions, galactic cosmic rays, anomalous cosmic rays, and suprathermal ions. The Integrated Science Investigation of the Sun (IS\ensuremath\odotIS) on board the Parker Solar Probe is a suite of energetic particle detectors covering the energy range \raisebox-0.5ex\textasciitilde20 keV-200 MeV nuc$^-1$. IS\ensuremath\odotIS measures energetic particles closer to the Su ...

Mitchell, J.~G.; Cohen, C.~M.~S.; Eddy, T.~J.; Joyce, C.~J.; Rankin, J.~S.; Shen, M.~M.; De Nolfo, G.~A.; Christian, E.~R.; McComas, D.~J.; McNutt, R.~L.; Wiedenbeck, M.~E.; Schwadron, N.~A.; Hill, M.~E.; Labrador, A.~W.; Leske, R.~A.; Mewaldt, R.~A.; Mitchell, D.~G.; Szalay, J.~R.;

Published by: \apjs      Published on: feb

YEAR: 2023     DOI: 10.3847/1538-4365/aca4c8

Parker Data Used; solar flares; Solar energetic particles; Interplanetary physics; Solar particle emission; Solar coronal mass ejection shocks; 1496; 1491; 827; 1517; 1997

Simulation of the Solar Energetic Particle Event on 2020 May 29 Observed by Parker Solar Probe

This paper presents a stochastic three-dimensional focused transport simulation of solar energetic particles (SEPs) produced by a data-driven coronal mass ejection (CME) shock propagating through a data-driven model of coronal and heliospheric magnetic fields. The injection of SEPs at the CME shock is treated using diffusive shock acceleration of post-shock suprathermal solar wind ions. A time-backward stochastic simulation is employed to solve the transport equation to obtain the SEP time-intensity profile at any location, ...

Cheng, Lei; Zhang, Ming; Lario, David; Balmaceda, Laura; Kwon, Ryun; Cohen, Christina;

Published by: \apj      Published on: feb

YEAR: 2023     DOI: 10.3847/1538-4357/acac21

Parker Data Used; Solar energetic particles; Solar particle emission; Solar coronal mass ejection shocks; 1491; 1517; 1997; Astrophysics - Solar and Stellar Astrophysics; Physics - Space Physics

2022

Double-power-law Feature of Energetic Particles Accelerated at Coronal Shocks

Recent observations have shown that in many large solar energetic particle (SEP) events the event-integrated differential spectra resemble double power laws. We perform numerical modeling of particle acceleration at coronal shocks propagating through a streamer-like magnetic field by solving the Parker transport equation, including protons and heavier ions. We find that for all ion species the energy spectra integrated over the simulation domain can be described by a double power law, and the break energy depends on the ion ...

Yu, Feiyu; Kong, Xiangliang; Guo, Fan; Liu, Wenlong; Jiang, Zelong; Chen, Yao; Giacalone, Joe;

Published by: \apjl      Published on: feb

YEAR: 2022     DOI: 10.3847/2041-8213/ac4cb3

1491; 1517; 1997; 1486; Astrophysics - Solar and Stellar Astrophysics

2021

Energetic Electron Observations by Parker Solar Probe/IS\ensuremath\odotIS during the First Widespread SEP Event of Solar Cycle 25 on 2020 November 29

At the end of 2020 November, two coronal mass ejections (CMEs) erupted from the Sun and propagated through the interplanetary medium in the direction of Parker Solar Probe while the spacecraft was located at \raisebox-0.5ex\textasciitilde0.81 au. The passage of these interplanetary CMEs (ICMEs) starting on November 29 (DOY 334) produced the largest enhancement of energetic ions and electrons observed by the Integrated Science Investigation of the Sun (IS\ensuremath\odotIS) energetic particle instrument suite on board Parker ...

Mitchell, J.~G.; De Nolfo, G.~A.; Hill, M.~E.; Christian, E.~R.; Richardson, I.~G.; McComas, D.~J.; McNutt, R.~L.; Mitchell, D.~G.; Schwadron, N.~A.; Bale, S.~D.; Giacalone, J.; Joyce, C.~J.; Niehof, J.~T.; Szalay, J.~R.;

Published by: \apj      Published on: oct

YEAR: 2021     DOI: 10.3847/1538-4357/ac110e

Parker Data Used; solar flares; Solar activity; Solar coronal mass ejection shocks; Interplanetary shocks; Solar energetic particles; Solar particle emission; 1496; 1475; 1997; 829; 1491; 1517



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