Сибирский федеральный университет

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 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.

Журнал: UNIVERSAL HELIOPHYSICAL PROCESSES

Выпуск журнала: Vol. 4, Is. 257

Номера страниц: 523-525

ISSN журнала: 17439213

Место издания: CAMBRIDGE

Издатель: CAMBRIDGE UNIV PRESS

• Salmin VladimirV . (KRASNOYARSK STATE UNIV)

• Web of Science Core Collection