Authors: N I Kobanov A S Kustov S A Chupin V A Pulyaev
Publish Date: 2011/10/12
Volume: 273, Issue: 1, Pages: 39-49
Abstract
An analysis of lineofsight velocity oscillation in nine solar faculae was undertaken with the aim of studying phase relations between chromospheric He i 10830 Å line and photospheric Si i 10827 Å line fiveminute oscillations We found that the time lag of the chromospheric signal relative to photospheric one varies from −12 to 100 seconds and is about 50 seconds on average We assume that the small observed lag can have three possible explanations i convergence of formation levels of He i 10830 Å and Si i 10827 Å in faculae ii significant increase of fiveminute oscillation propagation velocity above faculae iii simultaneous presence of standing and travelling waves
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