One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

The near-Earth space is a unique laboratory to explore turbulence and energy dissipation
processes in magnetized plasmas thanks to the availability of high-quality data from various …

In particular during the descending phase of the solar cycle, Alfvén waves in the high-speed
solar wind streams are a major form of interplanetary disturbances. The fluctuating …

The first complete estimation of the compressible energy cascade rate| ϵ C| at
magnetohydrodynamic (MHD) and subion scales is obtained in Earth's magnetosheath …

The first estimation of the energy cascade rate| ε C| of magnetosheath turbulence is obtained
using the Cluster and THEMIS spacecraft data and an exact law of compressible isothermal …

Heliospheric plasma turbulence plays a key role in transferring the energy of large‐scale
magnetic field and plasma flow fluctuations to smaller scales where the energy can be …

High‐resolution multispacecraft magnetic field measurements from the Magnetospheric
Multiscale mission's flux‐gate magnetometer are employed to examine statistical properties …

The dual spacecraft mission BepiColombo is the first joint mission between the European
Space Agency (ESA) and the Japanese Aerospace Exploration Agency (JAXA) to explore …

On the 1/f Spectrum in the Solar Wind and Its Connection with Magnetic Compressibility -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

In the solar wind, power spectral density (PSD) of the magnetic field fluctuations generally
follow the so-called Kolmogorov spectrum f− 5/3 in the inertial range, where the dynamics is …