activity
20152026
most citedMagnetic Field Rotations in the Solar Wind at Kinetic Scales

25 citations · 27 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Spatially Coherent and Intermittent Alfvénic Fluctuations in Solar Polar Spicules

Edris Tajfirouze, Christopher H. K. Chen, Richard J. Morton +1

Alfvénic fluctuations are considered a key mechanism for transporting energy from the lower solar atmosphere into the corona, with spicules acting as dynamic conduits for this tran…

physics.space-ph2025

The Nature of Turbulence at Sub-Electron Scales in the Solar Wind

Shiladittya Mondal, Christopher H. K. Chen, Davide Manzini

The nature of turbulence at sub-electron scales has remained an open question, central to understanding how electrons are heated in the solar wind. This is primarily because spacec…

physics.space-ph2025★ 1 cited

Analog ensemble forecasts of solar wind parameters: Quantification of the predictability and time-domain spectral performance

Pauline A. Simon, Christopher H. K. Chen, Mathew J. Owens +1

Forecasting multiscale properties of the solar wind is one of the important aspects of space weather prediction as mesoscales, larger than one minute, can affect the magnetosphere.…

astro-ph.SR2023★ 1 cited

Properties underlying the variation of the magnetic field spectral index in the inner solar wind

J. R. McIntyre, C. H. K. Chen, A. Larosa

Using data from orbits one to eleven of the Parker Solar Probe (PSP) mission, the magnetic field spectral index was measured across a range of heliocentric distances. The previousl…

physics.space-ph2015★ 25 cited

Magnetic Field Rotations in the Solar Wind at Kinetic Scales

C. H. K. Chen, L. Matteini, D. Burgess +1

The solar wind magnetic field contains rotations at a broad range of scales, which have been extensively studied in the MHD range. Here we present an extension of this analysis to…