Thermal metastabilities in the solar core

Simple item page
dc.creatorGrandpierre, Attila
dc.creatorAgoston, Gabor
dc.date2002-01-18
dc.date.accessioned2026-07-07T02:02:17Z
dc.date.available2026-07-07T02:02:17Z
dc.descriptionLinear stability analysis indicates that solar core is thermally stable for infinitesimal internal perturbations. For the first time, thermal metastabilities are found in the solar core when outer perturbations with significant amplitude are present. The obtained results show that hot bubbles generated by outer perturbations may travel a significant distance in the body of the Sun. These deep-origin hot bubbles have mass, energy, and chemical composition that may be related to solar flares. The results obtained may have remarkable relations to activity cycles in planets like Jupiter and also in extrasolar planetary systems.
dc.descriptionLaTex, 12 pages, 3 eps figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0201308
dc.identifierhttp://arxiv.org/abs/astro-ph/0201308
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4032
dc.subjectAstrophysics
dc.titleThermal metastabilities in the solar core
dc.typetext

Files

Collections

arXiv