44 citations · 135 across the 7 of their papers we have counts for
7 papers
Observation of Chaotic fluctuations in Turbulent Plasma
Riddi Bandyopadhyay, Nicolas V. Sarlis, James M. Weygand +3
Turbulence is a prevalent phenomenon in space and astrophysical plasmas, often characterized by stochastic fluctuations. While laboratory experiments and numerical simulations have…
Tens to hundreds of keV electron precipitation driven by kinetic Alfvén waves during an electron injection
Y. Shen, A. V. Artemyev, X. -J. Zhang +9
Electron injections are critical processes associated with magnetospheric substorms, which deposit significant electron energy into the ionosphere. Although wave scattering of 1…
Semiclassical limit problems with concurrent use of several clocks in quantum cosmology
Bruno Alexandre, João Magueijo
We revisit a recent proposal for a definition of time in quantum cosmology, to investigate the effects of having more than one possible type of clock "at the same time". We use as…
Comparative study of electric currents and energetic particle fluxes in a solar flare and Earth magnetospheric substorm
Anton Artemyev, Ivan Zimovets, Ivan Sharykin +20
Magnetic field-line reconnection is a universal plasma process responsible for the conversion of magnetic field energy to the plasma heating and charged particle acceleration. Sola…
Statistical study of auroral omega bands
Noora Partamies, James M. Weygand, Liisa Juusola
The presence of very few statistical studies on auroral omega bands motivated us to test-use a semi-automatic method for identifying large-scale undulations of the diffuse aurora b…
Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units
M. E. Ruiz, S. Dasso, W. H. Matthaeus +1
The solar wind is a structured and complex system, in which the fields vary strongly over a wide range of spatial and temporal scales. As an example, the turbulent activity in the…
Aging of anisotropy of solar wind magnetic fluctuations in the inner heliosphere
M. E. Ruiz, S. Dasso, W. H. Matthaeus +2
We analyze the evolution of the interplanetary magnetic field spatial structure by examining the inner heliospheric autocorrelation function, using Helios 1 and Helios 2 "in situ"…