LOWL p-mode frequencies and their variation with solar activity

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dc.creatorJiménez-Reyes, Sebastián J.
dc.creatorCorbard, Thierry
dc.creatorPallé, Pere L.
dc.creatorTomczyk, Steve
dc.date2000-11-22
dc.date.accessioned2026-07-07T01:56:38Z
dc.date.available2026-07-07T01:56:38Z
dc.descriptionWe present an analysis of the frequency shift and the even terms of the frequency splitting coefficients carried out using six years of LOWL data, starting in 1994. The temporal variations, and their dependences with the frequency and degree are addressed. The results are consistent with previous analysis.
dc.description4 pages, six figures. To appear in GONG-SOHO proceedings (ESA-SP464)
dc.identifierhttps://arxiv.org/abs/astro-ph/0011410
dc.identifierhttp://arxiv.org/abs/astro-ph/0011410
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2071
dc.subjectAstrophysics
dc.titleLOWL p-mode frequencies and their variation with solar activity
dc.typetext

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