Nonlinear Sciences – Chaotic Dynamics
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja....13975m&link_type=abstract
EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #13975
Nonlinear Sciences
Chaotic Dynamics
Scientific paper
Advances in understanding non-linear dynamics of many-body gravitation systems drive attention towards quantitative relations of orbital characteristics and planetary configurations in the Solar System, and to their implications on certain observable heliospheric and terrestrial phenomena. These are e.g. sunspot periodicities, auroral intensities, solar irradiance variations, climatic fluctuations, seismic and tectonic activity, etc. For some of them do exist historical records either directly measured or reconstructed and extended over the decade-to-millennial time-scales. Undoubtedly, part of these complex effects may be considered as mass and/or energy turbulences encountered both in the Sun and Earth due to tidal forces, thus being exemplifications of dissipative processes. Therefore, it seems both possible and justified to look for explanation of these phenomena in terms of the Prigogine concept of self-organisation in dissipative non-equilibrium systems. The submitted contribution is aimed to overview the existing evidence of such relationships, as well as to propose some new methodological approaches based on chaotic dynamics and fractal statistics.
No associations
LandOfFree
Selected self-organisation phenomena in the Solar System 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 Selected self-organisation phenomena in the Solar System, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Selected self-organisation phenomena in the Solar System will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-846018