collaborators

11 papers

physics.space-ph2026

Wave Activity at MHD-ion Scales Associated with Switchbacks

Kyung-Eun Choi, Oleksiy V. Agapitov, Forrest Mozer +9

Magnetic switchbacks (SB) -- the localized magnetic structures with magnetic field direction inclined at an angle relative to the background -- in the young solar wind h…

astro-ph.SR2026

Direct Evidence of Non-Ideal Dissipative Dynamics in Solar Wind Magnetic Switchbacks

Forrest Mozer, Oleksiy Agapitov, Kyung-Eun Choi +1

Magnetic switchbacks, large-amplitude, localized Alfvenic like rotations of the solar wind magnetic field, have been the subject of intensive investigation, with approximately 200…

astro-ph.SR2026

Measurements on the kinetic physics in streamer dynamics

Forrest Mozer, Kyungeun Choi, Richard Sydora +1

A major goal of solar physics is understanding the transition of the medium from the closed-loop magnetic configuration of the corona to the open structure of the heliospheric curr…

physics.space-ph2026

On flying near the base of a pseudo-streamer

Forrest Mozer, Oleksiy Agapitov, Kyungeun Choi +1

Near the 10 solar radius perihelion of Parker Solar Probe encounter 24, a confined region containing an enhanced plasma density (25,000 per cubic centimeter) and broadband electros…

astro-ph.SR2025

On the origin of the dominant waves in the extended solar corona

Forrest Mozer, Oleksiy Agapitov, Orlando Romeo +2

The extended solar corona at 10-30 solar radii is essentially devoid of all waves below 100 kHz other than triggered ion acoustic waves (TIAW), which consist of a low frequency ele…

astro-ph.SR2025

Plasma instability in the front of ejected energetic electrons and Type III solar radiobursts

Vladimir Krasnoselskikh, Immanuel Christopher Jebaraj, Tom Robert Franck Cooper +7

Type III radio bursts are a signature of the flux of near-relativistic electrons ejected during solar flares. These bursts are frequently observed by spacecraft such as the Parker…