2019/07/12 by A. D. Agaltsov, T. Hohage, R. G. Novikov · 1 citation
Mathematics · #math.AP #msc:35J10 #msc:35R30 #msc:65N21 #msc:85A15
paper · pdf · doi:10.1088/1361-6420/ab77d9
arxiv created 2019/07/12 · arxiv updated 2020/06/24
We consider the inverse problem of recovering the spherically symmetric sound speed, density and attenuation in the Sun from the observations of the acoustic field randomly excited by turbulent convection. We show that observations at two heights above the photosphere and at two frequencies above the acoustic cutoff frequency uniquely determine the solar parameters. We also present numerical simulations which confirm this theoretical result.