Dissipative anomaly states that ε, the rate of turbulent energy dissipation away from boundaries, remains finite as viscosity tends to zero. As a basi...

The upper atmosphere of the Sun, the solar corona, is expanding outward forming the solar wind and creating a bubble in the local interstellar medium,...

The 1/f spectrum, otherwise referred to as flicker noise, is a notable feature of solar wind observations. It often spans several orders of magnitude ...

Pressure-strain interaction has emerged as an important channel of energy conversion in collisionless plasma. On the one hand, it describes the pathwa...

The NASA Magnetospheric Multiscale (MMS) mission explores the boundary regions of the Earth's magnetosphere with high-accuracy measurements of charged...

Observations indicate that helical magnetic flux tubes are present in the solar corona and solar wind [eg, 1,2,3]. In the solar wind there is some que...

Turbulence is an inherently multiscale phenomenon. It is characterized by cross-scale energy transfer, along with the formation of intermittent struct...

The 1/f spectrum, otherwise referred to as flicker noise, is an observed feature of the of solar wind, spanning several orders of magnitude in frequen...