papers

Publications (42)

physics.space-ph2019

Time domain structures and dust in the solar vicinity: Parker Solar Probe observations

F. S. Mozer, O. V. Agapitov, S. D. Bale +9

On April 5, 2019, while the Parker Solar Probe was at its 35 solar radius perihelion, the data set collected at 293 samples/sec contained more than 10,000 examples of spiky electri…

astro-ph.SR2020

Detection of small magnetic flux ropes from the third and fourth Parker Solar Probe encounters

L. -L. Zhao, G. P. Zank, Q. Hu +22

We systematically search for magnetic flux rope structures in the solar wind to within the closest distance to the Sun of 0.13 AU, using data from the third and fourth orbits of th…

physics.space-ph2019

Identification of Magnetic Flux Ropes from Parker Solar Probe Observations during the First Encounter

L. -L. Zhao, G. P. Zank, L. Adhikari +17

The Parker Solar Probe (PSP) observed an interplanetary coronal mass ejection (ICME) event during its first orbit around the sun, among many other events. This event is analyzed by…

astro-ph.SR2023

Whistler waves generated inside magnetic dips in the young solar wind: observations of the Search-Coil Magnetometer on board Parker Solar Probe

C. Froment, O. V. Agapitov, V. Krasnoselskikh +11

Context. Whistler waves are electromagnetic waves produced by electron-driven instabilities, that in turn can reshape the electron distributions via wave-particle interactions. In…

astro-ph.SR2025

Energy-dependent SEP Fe/O abundances during the May 2024 superstorm

G. D. Muro, C. M. S. Cohen, Z. Xu +16

During mid-May 2024, active region (AR) 13664 produced a series of M- and X-class flares along with several coronal mass ejections (CMEs) that resulted in exceptionally strong auro…

astro-ph.SR2021

Solar wind energy flux observations in the inner heliosphere: First results from Parker Solar Probe

M. Liu, K. Issautier, N. Meyer-Vernet +15

We investigate the solar wind energy flux in the inner heliosphere using 12-day observations around each perihelion of Encounter One (E01), Two (E02), Four (E04), and Five (E05) of…