Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..523s&link_type=abstract
Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 523-525
Astronomy and Astrophysics
Astronomy
Mhd, Solar System: Formation
Scientific paper
Stereographic projection of Hopf field on the 3-sphere into Euclidean 3-space is used as a model of 3D steady flow of ideal compressible fluid in MHD. In such case, flow lines are Villarceau circles lying on tori corresponding to the levels of Bernoulli function. Existence of an optimal torus with minimal relative surface free energy is shown. Beat of oscillations with wave numbers corresponding to structural radii of optimal torus leads to scaling of optimal tori. Spatial intersection of homothetic tori within one torus result in formation of cluster with the size depending on scaling factor. Optimal tori are considered as precursors of planetary orbits.
No associations
LandOfFree
MHD Kamchatnov-Hopf soliton in the model of primordial solar nebula 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 MHD Kamchatnov-Hopf soliton in the model of primordial solar nebula, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MHD Kamchatnov-Hopf soliton in the model of primordial solar nebula will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-978564