Fundamental issues on kappa-distributions in space plasmas and interplanetary proton distributions

Details Fundamental issues on kappa-distributions in space plasmas and interplanetary proton distributions Fundamental issues on kappa-distributions in space plasmas and interplanetary proton distributions

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004phpl...11.1308l&link_type=abstract

Physics of Plasmas, Volume 11, Issue 4, pp. 1308-1316 (2004).

Physics

90

Solar Wind Plasma, Sources Of Solar Wind, Particle Acceleration

Scientific paper

Numerous in situ observations indicate clearly the presence of nonthermal electron and ion structures as ubiquitous and persistent feature in a variety of astrophysical plasma environments. In particular, the detected suprathermal particle populations are accurately represented by the family of κ-distributions, a power-law in particle speed. After clarifying the characteristics of high-energy tail distributions under various space plasma conditions, different generation mechanisms of energetic particles are introduced where numerical simulations of wave-particle interaction based on a Fokker-Planck approach demonstrate how Landau interaction ultimately leads to κ-like distributions. Because of lack of theoretical justification, the use of the analytical form of κ-functions was frequently criticized. It is shown that these distributions turn out as consequence of an entropy generalization favored by nonextensive thermo-statistics, thus providing the missing link for powerlaw models of suprathermal tails from fundamental physics, along with a physical interpretation of the structure parameter κ. Moreover, with regard to the full nonextensive formalism, compatible also with negative values of κ, it is demonstrated that core-halo distribution structures, as observed for instance under typical interplanetary plasma conditions, are a natural content of the pseudo-additive entropy concept. The significance of the complete κ-distribution family with regard to observed core-halo electron and double-humped ion velocity space characteristics is illuminated, where the observed peak separation scale of interplanetary proton distributions is compatible with a maximum entropy condition.

Affiliated with

Also associated with

No associations

Rating

Fundamental issues on kappa-distributions in space plasmas and interplanetary proton distributions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Fundamental issues on kappa-distributions in space plasmas and interplanetary proton distributions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fundamental issues on kappa-distributions in space plasmas and interplanetary proton distributions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1461129