Helioseismology in Space Weather - National Solar Observatory
Helioseismology in Space Weather - National Solar Observatory
Helioseismology in Space Weather - National Solar Observatory
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Emerg<strong>in</strong>g Active Regionsq Braun, D. C., Science, 336, 296. “Comment on Detection of Emerg<strong>in</strong>g SunspotRegions <strong>in</strong> <strong>Solar</strong> Interiorq Ilonidis, S., Zhao J. and Kosovichech, A. “Response to Comment on Detection ofEmerg<strong>in</strong>g Sunspot Regions <strong>in</strong> <strong>Solar</strong> Interiorü On the orig<strong>in</strong>g of the large time difference: “The observed phase-shifts can be causednot only by sound-speed and magnetic-field perturbations or plasma flows, but also by morecomplex effects such as absorption and scatter<strong>in</strong>g. There has been also evidence, both fromobservations and simulations, that submerged magnetic regions can modify the acoustic powerabove them”q Braun, D. C., 2012, <strong>Solar</strong> Physics, tmp 306B “Helioseismic Holography of anArtificial Submerged Sound Speed Perturbation and Implications for the Detection ofPre-emergence Signatures of Active Regions