Results 81 to 90 of about 89,978 (184)
Observations of Kappa Distributions in Solar Energetic Protons and Derived Thermodynamic Properties
In this paper, we model the high-energy tail of observed solar energetic proton energy distributions with a kappa distribution function. We employ a technique for deriving the thermodynamic parameters of solar energetic proton populations measured by the
M. E. Cuesta +15 more
doaj +1 more source
Kappa-like distribution functions inside magnetic clouds
En este trabajo estamos interesados en el estudio de la temperatura y el perfil de las colas supratermales de los electrones en nubes magnéticas. Para ello hemos modelado las funciones de distribución de velocidades de los electrones como superposición de dos poblaciones, core (Maxwellian) y halo (Tsallis o tipo kappa).
T. Nieves-Chinchilla, A. F. Viñas
openaire +3 more sources
Thermodynamic Constraints on Solar Wind Radial Profiles
In this paper, we use thermodynamics to develop the radial density profile of the solar wind, which is described by kappa distributions. First, we show the connection of kappa distributions with polytropic processes, emphasizing the two “paths”—i.e., a ...
G. Livadiotis, D. J. McComas
doaj +1 more source
The energy spectrum of energetic electrons is a key factor representing the dynamic variations of Earth’s Van Allen radiation belts. Increased measurements have indicated that the commonly used Maxwellian and Kappa distributions are inadequate for ...
LuHuai Jiao +5 more
doaj +1 more source
Heat-flux Instabilities of Regularized Kappa Distributed Strahl Electrons Resolved with ALPS
The fluid behavior of the solar wind is affected by the heat flux carried by the suprathermal electron populations, especially the electron strahl (or beam) that propagates along the magnetic field.
Dustin L. Schröder +3 more
doaj +1 more source
Continuation of Direct Products of Distributions
If, in some problems, one has to deal with the ``product'' of distributions $\rm f_i$ (also called generalized functions) $\rm\bar T = \Pi^m_{i=1} f_i$, this product has a priori no definite meaning as a functional $(\rm \bar T, \phi) $ for $\rm\phi \in ...
Petermann, A.
core
Introduction The kappa distribution was first introduced by Mielke (1973) and Mielke and Johnson (1973) for describing and analyzing precipitation data. This distribution is positively skewed and is widely applied when studying precipitation, wind speed ...
Maryam Sharafi +3 more
doaj
Context. Ganymede’s UV aurorae, observed by HST and Juno/UVS, trace interactions between its atmosphere and Jupiter’s magneto-sphere. These emissions, dominated by O I lines at 130.4 and 135.6 nm, are driven by electron impact on species such as H2O, O ...
Benmahi B. +20 more
doaj +1 more source
Quasi-linear approach of bi-Kappa distributed electrons with dynamic κ parameter
Context. In recent years, significant progress has been made in the velocity-moment-based quasi-linear (QL) theory of waves and instabilities in plasmas with nonequilibrium velocity distributions (VDs) of the Kappa (or κ) type.
Moya Pablo S. +5 more
doaj +1 more source

