Self-organization processes on the sun - The heliosynergetics

dc.contributor.author	Krishan, V
dc.contributor.author	Mogilevskij, E. I
dc.date.accessioned	2008-09-10T12:33:03Z
dc.date.available	2008-09-10T12:33:03Z
dc.date.issued	1990
dc.identifier.citation	IAU Symposium, No. 142, pp. 125 - 133	en
dc.identifier.issn	0074-1809
dc.identifier.uri	http://hdl.handle.net/2248/3531
dc.description.abstract	A study by Levich and Tzvetkov (1985) is used to construct a model of solar granulation in its entirety. Solar granulation on all scales and the formation and evolution of some structures in active solar regions are interpreted to be the result of self-organization processes occurring in a turbulent medium. A Schroedinger-type equation that gives a full spectrum of discrete structures depending on the available free energy is used to search for sources of solar flares. A magnetoactive medium possessing helicity is found to submit itself to the formation of solitons which themselves could be the organized state of a nonlinear medium describable by a KDV equation. A gas composed of many solitons could get further organized into one big soliton which could carry enough energy for a big flare.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..142..125K	en
dc.subject	Nonlinear systems	en
dc.subject	Solar activity	en
dc.subject	Turbulence, Vortices	en
dc.subject	Navier-stokes equation	en
dc.subject	Solar flares	en
dc.title	Self-organization processes on the sun - The heliosynergetics	en
dc.type	Article	en