Contribution of Cyclotron-resonant Damping to Kinetic Dissipation of Interplanetary Turbulence [PDF]
With 1 figure; accepted by Astrophys. J.
Leamon, Robert J. +3 more
openaire +2 more sources
Observations of Waves and Structures by Frequency–Wavenumber Spectrum in Solar Wind Turbulence
A well-known shortcoming of single-spacecraft spectral analysis is that only the 1D wavenumber spectrum can be observed, assuming the characteristic wave propagation speed is much smaller than the solar wind flow speed.
L.-L. Zhao +3 more
doaj +1 more source
Solar cycle changes of large-scale solar wind structure
In this paper, I present the results on large-scale evolution of density turbulence of solar wind in the inner heliosphere during 1985 - 2009. At a given distance from the Sun, the density turbulence is maximum around the maximum phase of the solar cycle
Manoharan, P. K. Manoharan
core +1 more source
One-point statistics and intermittency of induced electric field in the solar wind
The interplanetary induced electric field e=vxb is studied, using solar wind time series. The probability distribution functions (PDFs) of the electric field components are measured from the data and their non-gaussianity is discussed.
Bruno, Roberto +2 more
core +1 more source
The Influence of Magnetic Turbulence on the Energetic Particle Transport Upstream of Shock Waves
Energetic particles are ubiquitous in the interplanetary space and their transport properties are strongly influenced by the interaction with magnetic field fluctuations.
Silvia Perri +4 more
doaj +1 more source
Sunward-propagating Alfv\'enic fluctuations observed in the heliosphere [PDF]
The mixture/interaction of anti-sunward-propagating Alfv\'enic fluctuations (AFs) and sunward-propagating Alfv\'enic fluctuations (SAFs) is believed to result in the decrease of the Alfv\'enicity of solar wind fluctuations with increasing heliocentric ...
Belcher, J. W. +4 more
core +3 more sources
A nonextensive entropy approach to solar wind intermittency
The probability distributions (PDFs) of the differences of any physical variable in the intermittent, turbulent interplanetary medium are scale dependent.
Baumjohann W. +20 more
core +1 more source
Abstract Based on 2‐year magnetic data from the Macau science satellite, we investigate the compressional Pc3‐4 pulsations (between 16 and 100 mHz) driven by upstream waves (UWs). Our results confirm larger UWs amplitudes in the South Atlantic Anomaly (SAA) longitudes, agreeing with previous missions.
Chao Xiong +3 more
wiley +1 more source
Characterization of the Transmission and Generation of Turbulence at Interplanetary Shocks
We study the transmission and characteristics of turbulent magnetohydrodynamic (MHD) fluctuations from upstream to downstream regions of interplanetary (IP) shocks using the linear mode decomposition (LMD) technique of G. P. Zank et al.
Sujan Prasad Gautam +10 more
doaj +1 more source
INFLUENCE OF THE SOLAR WIND ON INTERFEROMETRIC OBSERVATIONS AT THE DECAMETER WAVELENGTHS [PDF]
Purpose: The effect of the Earth’s ionosphere and interplanetary plasma on the radio astronomy observations, in particular, interferometric ones, at decameter waves has been investigated.
V. O. Shepelev +3 more
doaj +1 more source

