A comprehensive overview is presented of recent observational and theoretical results on
solar wind structures and fluctuations and magnetohydrodynamic waves and turbulence …

In situ measurements of the solar wind and remote observations of coronal holes have
strongly implicated the resonant interaction with ion cyclotron waves as the responsible …

Electron density power spectrum in the local interstellar medium ADS Classic is now
deprecated. It will be completely retired in October 2019. This page will automatically redirect to …

This paper presents a theoretical framework for understanding plasma turbulence in
astrophysical plasmas. It is motivated by observations of electromagnetic and density …

Solar wind fluctuations are commonly regarded as a superposition of MHD waves, primarily
in the Alfvén mode. These MHD fluctuations are frequently assumed to possess “slab” or …

An extended random medium is modeled by a set of 2-D thin Gaussian phase-changing
screens with phase power spectral densities appropriate to the natural medium being …

The Mars gravity field resolution is mostly determined by the lower altitude Mars
Reconnaissance Orbiter (MRO) tracking data. With nearly four years of additional MRO and …

Radio Doppler data from four encounters of the Galileo spacecraft with the jovian moon
Europa have been used to refine models of Europa's interior. Europa is most likely …

The theory of nearly incompressible (NI) fluid dynamics developed previously for
hydrodynamics is extended to magnetohydrodynamics (MHD). On the basis of a singular …

The physical processes involved in diffusion of Galactic cosmic rays in the interstellar
medium are addressed. We study the possibility that the nonlinear MHD cascade sets the …