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,...

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