Intermittency as a possible underlying mechanism for solar and stellar variability

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dc.creatorTavakol, Reza
dc.creatorCovas, Eurico
dc.date1999-04-28
dc.date.accessioned2026-07-07T02:31:25Z
dc.date.available2026-07-07T02:31:25Z
dc.descriptionWe briefly discuss the status of the intermittency hypothesis, according to which the grand minima type variability in solar-type stars may be understood in terms of dynamical intermittency. We review concrete examples which establish this hypothesis in the mean-field setting. We discuss some difficulties and open problems regarding the establishment of this hypothesis in more realistic settings as well as its operationally decidability.
dc.descriptionSubmitted to PASP, paper presented at the Workshop on Stellar Dynamos: Chaotic flows and nonlinearities. Full paper available at http://www.maths.qmw.ac.uk/~eoc
dc.identifierhttps://arxiv.org/abs/astro-ph/9904394
dc.identifierhttp://arxiv.org/abs/astro-ph/9904394
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14148
dc.subjectAstrophysics
dc.titleIntermittency as a possible underlying mechanism for solar and stellar variability
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