Mathematics – Probability
Scientific paper
Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..120c&link_type=abstract
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 120-123 (2010).
Mathematics
Probability
Solar Wind, Interplanetary Magnetic Fields, Magnetohydrodynamics, Probability, Magnetic Fields, Particle Emission, Solar Wind, Interplanetary Magnetic Fields, Magnetohydrodynamics And Plasmas, Probability Theory, Electric And Magnetic Fields, Solar Magnetism
Scientific paper
In the last two decades we have assisted at a growing interest in the study of complexity and complex dynamics in space plasmas. This is particularly true in the case of interplanetary and magnetospheric space plasmas which display turbulence, self organization and/or self-organized critical dynamics. Here, I present some preliminary results on the evolution of order in the radial evolution of solar wind magnetic field. In detail, using the criterion contained in the S-Theorem by Klimontovich [1], I compute the relative degree of order for the magnetic field intensity fluctuations at different radial distances as observed by interplanetary mission. The preliminary results seems to point toward and increase of order with the radial distance, suggesting the occurrence of structuring (formation of structures) in the course of the evolution.
No associations
LandOfFree
Relative degree of order in radial evolution of solar wind fluctuations 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 Relative degree of order in radial evolution of solar wind fluctuations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relative degree of order in radial evolution of solar wind fluctuations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1423486