Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2663
Title: A model of solar granulation through inverse cascade
Authors: Krishan, V
Keywords: Magnetohydrodynamic turbulence
Solar atmosphere
Solar granulation
Stellar structure
Kolmogoroff theory
Stellar models
Solar interior
Vortex breakdown
Issue Date: May-1991
Publisher: Royal Astronomical Society
Citation: Monthly Notices of Royal Astronomical Society, Vol. 250, No.1, pp. 50 - 53
Abstract: Nonlinear interactions between small fluid elements in an energetically open system facilitate the formation of large coherent stable structures. This is known as self-organization. Solar granulation on all scales is interpreted to be the result of self-organization processes occurring in the turbulent medium of the solar atmosphere. This mechanism provides explanations for the intrinsic weakness of mesogranulation and the rare appearance of giant cells in addition to the sizes and lifetimes of these structures. The entire energy spectrum from the smallest granules to the largest giant cells brings out the prevalence of Kolmogorov's K exp -5/3 law.
URI: http://hdl.handle.net/2248/2663
ISSN: 0035-8711
Appears in Collections:IIAP Publications

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