The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

The dissipation of magnetized turbulence is an important paradigm for describing heating
and energy transfer in astrophysical environments such as the solar corona and wind; …

The fluctuating magnetic helicity is considered an important parameter in diagnosing the
characteristic modes of solar wind turbulence. Among them is the Alfvén-cyclotron wave …

Magnetic field data acquired by the Ulysses spacecraft in high-speed streams over the poles
of the Sun are used to investigate the normalized magnetic helicity spectrum σ m as a …

We use magnetic field and ion moment data from the MFI and SWE instruments on board the
Wind spacecraft to study the nature of solar wind turbulence at ion-kinetic scales. We …

Intervals of enhanced magnetic fluctuations have been frequently observed in the solar
wind. But it remains an open question as to whether these waves are generated at the Sun …

Abstract Parker Solar Probe (PSP) observed predominately Alfvénic fluctuations in the solar
wind near the Sun where the magnetic field tends to be radially aligned. In this paper, two …

This review paper compiles recent results obtained by the present group of authors
describing the effects of suprathermal populations present in space plasmas (up to a few …

Transverse, near-circularly polarized, parallel-propagating electromagnetic waves around
the proton cyclotron frequency were found sporadically in the solar wind throughout the …