What does helioseismology tell us about solar cycle related structural changes in the Sun?

Simple item page
dc.creatorBasu, Sarbani
dc.date2002-05-03
dc.date.accessioned2026-07-07T02:03:33Z
dc.date.available2026-07-07T02:03:33Z
dc.descriptionSolar oscillations frequencies show a distinct change with solar activity. The changes in frequencies can be used to study the time variation of solar structure. We discuss constraints on the changes in solar structure with time as obtained with helioseismic data covering the last six years. The frequency variations appear to be dominated by changes in the near-surface layers rather than by changes in the structure of the deeper layers.
dc.descriptionTo appear in Proc. SOHO-11, `` From Solar Min to Max: Half a Solar Cycle with SOHO,'' ESA SP-508
dc.identifierhttps://arxiv.org/abs/astro-ph/0205049
dc.identifierhttp://arxiv.org/abs/astro-ph/0205049
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4422
dc.subjectAstrophysics
dc.titleWhat does helioseismology tell us about solar cycle related structural changes in the Sun?
dc.typetext

Files

Collections

arXiv