activity
20102024
most citedMagnetic Reconnection and Intermittent Turbulence in the Solar Wind

174 citations · 808 across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2024

Variation in Path Lengths of Turbulent Magnetic Field Lines and Solar Energetic Particles

Wirin Sonsrettee, Piyanate Chuychai, Achara Seripienlert +5

Modeling of time profiles of solar energetic particle (SEP) observations often considers transport along a large-scale magnetic field with a fixed path length from the source to th…

physics.plasm-ph20241 cited

Scale Separation Effects on Simulations of Plasma Turbulence

Jago Edyvean, Tulasi N. Parashar, Tom Simpson +7

Understanding plasma turbulence requires a synthesis of experiments, observations, theory, and simulations. In the case of kinetic plasmas such as the solar wind, the lack of colli…

physics.space-ph2024

Anisotropy of Density Fluctuations in the Solar Wind at 1 au

Jiaming Wang, Rohit Chhiber, Sohom Roy +6

A well-known property of solar wind plasma turbulence is the observed anisotropy of the autocorrelations, or equivalently the spectra, of velocity and magnetic field fluctuations.…

physics.space-ph2024

Correlation of Coronal Mass Ejection Shock Temperature with Solar Energetic Particle Intensity

Manuel Enrique Cuesta, D. J. McComas, L. Y. Khoo +13

Solar energetic particle (SEP) events have been observed by the Parker Solar Probe (PSP) spacecraft since its launch in 2018. These events include sources from solar flares and cor…

physics.space-ph2023

Unveiling plasma energization and energy transport in the Earth Magnetospheric System: the need for future coordinated multiscale observations

A. Retino, L. Kepko, H. Kucharek +31

Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in…

physics.plasm-ph2023

Scale Filtering Analysis of Kinetic Reconnection and its Associated Turbulence

Subash Adhikari, Yan Yang, William H. Matthaeus +3

Previously, using an incompressible von Kármán-Howarth formalism, the behavior of cross-scale energy transfer in magnetic reconnection and turbulence was found to be essentially id…