In plasmas, Debye screening structures the possible correlations between particles. We identify a phase space minimum h* in non-equilibrium space plasmas that connects the energy of particles in a Debye sphere to an equivalent wave frequency. In particular, while there is no a priori reason to expect a single value of h* across plasmas, we find a very similar value of h* ≈ (7.5 ± 2.4)×10−22 J·s using four independent methods: (1) Ulysses solar wind measurements, (2) space plasmas that typically reside in stationary states out of thermal equilibrium and spanning a broad range of physical properties, (3) an entropic limit emerging from statistical mechanics, (4) waiting-time distributions of explosive events in space plasmas. Finding a quas...
In the majority of the literature on plasma shock waves, electrons play the role of “ghost particles...
Complex (or “dusty”) plasmas consist of electrons, ions, charged, mostly monodisperse, microparticl...
When \lambda_{T} << d_{T}, where \lambda_{T} is the de Broglie wavelength and d_{T}, the distance of...
The Boltzmann–Gibbs (BG) entropy has been used in a wide variety of problems for more than a century...
Unraveling the physics of the entire turbulent cascade of energy in space and astrophysical plasmas ...
The zeroth law of turbulence states that, for fixed energy input into large-scale motions, the stati...
Dissipative processes cause collisionless plasmas in many systems to develop nonthermal particle dis...
When applied to classical plasmas which are neutralized by a uniform background, the well known Deby...
The field-particle correlation technique utilizes single-point measurements to uncover signatures of...
Turbulent density fluctuations are investigated in the solar wind at sub-ion scales using calibrated...
The quasi-thermal noise spectroscopy is an accurate method of determination of density and temperatu...
We developed a model for the equation of state of fully ionized plasmas which we apply to hydrogen. ...
International audienceA weak continuous line has been recently discovered onboard Voyager 1 in the i...
As has been revealed in a number of more recent astrophysical papers, in most of the tenuous space p...
Boltzmann-Gibbs (BG) entropy has additive and extensive properties, but for certain physical systems...
In the majority of the literature on plasma shock waves, electrons play the role of “ghost particles...
Complex (or “dusty”) plasmas consist of electrons, ions, charged, mostly monodisperse, microparticl...
When \lambda_{T} << d_{T}, where \lambda_{T} is the de Broglie wavelength and d_{T}, the distance of...
The Boltzmann–Gibbs (BG) entropy has been used in a wide variety of problems for more than a century...
Unraveling the physics of the entire turbulent cascade of energy in space and astrophysical plasmas ...
The zeroth law of turbulence states that, for fixed energy input into large-scale motions, the stati...
Dissipative processes cause collisionless plasmas in many systems to develop nonthermal particle dis...
When applied to classical plasmas which are neutralized by a uniform background, the well known Deby...
The field-particle correlation technique utilizes single-point measurements to uncover signatures of...
Turbulent density fluctuations are investigated in the solar wind at sub-ion scales using calibrated...
The quasi-thermal noise spectroscopy is an accurate method of determination of density and temperatu...
We developed a model for the equation of state of fully ionized plasmas which we apply to hydrogen. ...
International audienceA weak continuous line has been recently discovered onboard Voyager 1 in the i...
As has been revealed in a number of more recent astrophysical papers, in most of the tenuous space p...
Boltzmann-Gibbs (BG) entropy has additive and extensive properties, but for certain physical systems...
In the majority of the literature on plasma shock waves, electrons play the role of “ghost particles...
Complex (or “dusty”) plasmas consist of electrons, ions, charged, mostly monodisperse, microparticl...
When \lambda_{T} << d_{T}, where \lambda_{T} is the de Broglie wavelength and d_{T}, the distance of...