Parker Solar Probe observations of solar energetic particle events with inverse-velocity-arrival features

In solar energetic particle (SEP) events, velocity dispersion (VD) is characterized by the earlier arrival of faster, higher energy particles relative to slower ones, assuming negligible acceleration time and scattering effects. This characteristic enables estimation of the time of particle release...

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Autores principales:	Xu Zigong, Cohen C. M. S., Leske R. A., Muro G. D., Cummings A. C., Romeo O. M., Lario D., McComas D. J., Cuesta M. E., Pak S., Khoo L. Y., Farooki H. A., Shen M. M., Kasapis S., Christian E. R., Grant Mitchell J., Mitchell D. G., McNutt R. L., Kouloumvakos A., Berland G. D., Schwadron N. A., Wiedenbeck M. E., Stevens M. L., Allen R. C.
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	EDP Sciences 2026-06-01
Colección:	Astronomy & Astrophysics
Materias:	sun: activity sun: coronal mass ejections (cmes) sun: general sun: heliosphere sun: particle emission solar-terrestrial relations
Acceso en línea:	https://www.aanda.org/articles/aa/full_html/2026/06/aa60274-26/aa60274-26.html
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