The nature of the magnetic field fluctuations in the solar wind between the ion and electron
scales is still under debate. Using the Cluster/STAFF instrument, we make a survey of the …

Whistler waves are intermittently present in the solar wind, while their origin and effects are
not entirely understood. We present a statistical analysis of magnetic field fluctuations in the …

We use the one-dimensional TRISTAN-MP particle-in-cell code to model the nonlinear
evolution of the whistler heat flux instability (WHFI) that was proposed by Gary et al. and …

We present results of a two-dimensional fully kinetic particle-in-cell simulation in order to
shed light on the role of whistler waves in the scattering of strahl electrons and in the heat …

At electron scales, the power spectrum of solar-wind magnetic fluctuations can be highly
variable and the dissipation mechanisms of the magnetic energy into the various particle …

The origins and properties of large-amplitude whistler wavepackets in the solar wind are still
unclear. In this Letter, we utilize single spacecraft electric and magnetic field waveform …

We present an analysis of simultaneous particle and field measurements from the ARTEMIS
spacecraft, which demonstrates that quasi-parallel whistler waves in the solar wind can be …

We present a theoretical analysis of electron heat flux inhibition in the solar wind when a
significant portion of the heat flux is carried by strahl electrons. We adopt core-strahl velocity …

The role of solar wind expansion in generating whistler waves is investigated using the EB-
iPic3D code, which models solar wind expansion self-consistently within a fully kinetic semi …

Abstract Using the Parker Solar Probe FIELDS bandpass-filter data and SWEAP electron
data from Encounters 1 through 9, we show statistical properties of narrowband whistlers …