Тип публикации: доклад, тезисы доклада, статья из сборника материалов конференций
Конференция: Symposium of the International-Astronomical-Union; Ioannina, GREECE; Ioannina, GREECE
Год издания: 2009
Идентификатор DOI: 10.1017/S1743921309029810
Ключевые слова: MHD; solar system: formation
Аннотация: 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 eneПоказать полностьюrgy 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.
Журнал: UNIVERSAL HELIOPHYSICAL PROCESSES
Выпуск журнала: Vol. 4, Is. 257
Номера страниц: 523-525
ISSN журнала: 17439213
Место издания: CAMBRIDGE
Издатель: CAMBRIDGE UNIV PRESS