Signature of the solar cycle in the low degree p-modes using Mark-I

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dc.creatorJiménez-Reyes, Sebastián J.
dc.creatorCorbard, Thierry
dc.creatorPallé, Pere L.
dc.date2000-11-22
dc.date.accessioned2026-07-07T01:56:38Z
dc.date.available2026-07-07T01:56:38Z
dc.descriptionHigh quality observations of the low degree p-modes exist for almost two complete solar cycles using the solar spectrophotometer Mark-I, located and operating at the Observatorio del Teide (Tenerife, Spain). In this work, the observations available have been re-analyzed over a much wider time interval than before. We analyze the time variation of the yearly frequency shift and its frequency dependence. This information will be used in order to average annual power spectra by removing the effect of the solar cycle. Using this average power spectrum, a new estimate of the rotational splittings is attempted.
dc.description4 pages, 5 figures, To appear in GONG-SOHO proceedings (ESA-SP464)
dc.identifierhttps://arxiv.org/abs/astro-ph/0011411
dc.identifierhttp://arxiv.org/abs/astro-ph/0011411
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2072
dc.subjectAstrophysics
dc.titleSignature of the solar cycle in the low degree p-modes using Mark-I
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