Abstract
Simultaneous measurements at different wavelengths offer the prospect of studying the sensitivity of helioseismic inferences to the choice of observing height both in quiet-Sun and magnetically active regions. In this context, we use observations from space-borne measurements from the Solar Dynamics Observatory and ground-based Global Oscillation Network Group to analyze high-degree acoustic mode parameters and sub-surface flows obtained with different observables. We also quantify differences and interpret results in the framework of the formation height in solar atmosphere. © 2013 Published under licence by IOP Publishing Ltd.
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CITATION STYLE
Jain, K., Tripathy, S., Basu, S., Bogart, R., Hernández, I. G., Hill, F., & Howe, R. (2013). Multi-spectral study of acoustic mode parameters and sub-surface flows. In Journal of Physics: Conference Series (Vol. 440). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/440/1/012012
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