Variation in p-mode power over solar cycle 23 as seen from BiSON and GOLF observations

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dc.creatorSimoniello, R.
dc.creatorSalabert, D.
dc.creatorGarcia, R. A.
dc.date2008-10-10
dc.date.accessioned2026-07-07T10:09:09Z
dc.date.available2026-07-07T10:09:09Z
dc.descriptionWe analyzed BiSON and GOLF/SoHO data with a new technique, to investigate p-mode power variation over solar cycle 23. We found a decrease in the mean velocity power of about 20% for BiSON during the ascending phase, in agreement with previous findings. We also found that GOLF, during the red-wing configuration, seems to be working at a different height than the theoretically computed one.
dc.description4 pages, 2 figures, Conference proceeding GONG 2008 / SOHO XXI Meeting
dc.identifierhttps://arxiv.org/abs/0810.1856
dc.identifierhttp://arxiv.org/abs/0810.1856
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/171234
dc.subjectAstrophysics
dc.titleVariation in p-mode power over solar cycle 23 as seen from BiSON and GOLF observations
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