Changes in the Subsurface Stratification of the Sun with the 11-Year Activity Cycle
Author(s) -
S. Lefebvre,
А. Г. Косовичев
Publication year - 2005
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/498305
Subject(s) - helioseismology , stratification (seeds) , physics , radius , solar radius , doppler effect , observatory , elevation angle , astrophysics , atmospheric sciences , astronomy , solar wind , plasma , coronal mass ejection , seed dormancy , germination , botany , computer security , quantum mechanics , dormancy , magnetic field , computer science , biology , azimuth
We report on the changes of the Sun's subsurface stratification inferred fromhelioseismology data. Using SOHO/MDI (SOlar and HeliosphericObservatory/Michelson Doppler Imager) data for the last 9 years and, moreprecisely, the temporal variation of f-mode frequencies, we have computed thevariation of the radius of subsurface layers of the Sun by applyinghelioseismic inversions. We have found a variability of the ``helioseismic''radius in antiphase with the solar activity, with the strongest variations ofthe stratification being just below the surface around 0.995$R_{\odot}$.Besides, the radius of the deeper layers of the Sun, between 0.975$R_{\odot}$and 0.99$R_{\odot}$ changes in phase with the 11-year cycle.Comment: 14 pages, 7 figures, accepted in ApJ
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